This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW
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 31.3529 2461191.8529 8.69 01:56:38.10 +59:15:33.5
131.18820 -2.56332 galactic Cas Second-epoch detections are separated by 0.4" and 3.4 pix
The object was found in VSX 0" 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 01:56:38.10 +59:15:33.5: 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 01:56:38.10 +59:15:33.5: 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 31.3529* 01 56 38.10 +59 15 33.5 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,2461191.8529,8.69,0.05,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
X Cas 20260531.3529 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 31.3529 2461191.8529 9.29 01:43:36.46 +58:48:08.4
129.65675 -3.38658 galactic Cas Second-epoch detections are separated by 0.2" and 3.6 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 +58:48:08.4: 14.72 +/- 0.15 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 +58:48:08.4: 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 31.3529* 01 43 36.46 +58 48 08.4 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
V0917 Cas,2461191.8529,9.29,0.05,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
V0917 Cas 20260531.3529 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 31.3529 2461191.8529 10.67 00:30:33.64 +66:05:36.8
120.81574 3.30763 galactic Cas Second-epoch detections are separated by 1.2" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:30:33.64 +66:05:36.8 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:30:33.64 +66:05:36.8: 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 00:30:33.64 +66:05:36.8: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 31.3529* 00 30 33.64 +66 05 36.8 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.8529,10.67,0.05,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
target 20260531.3529 10.67CV 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 31.3529 2461191.8529 10.05 01:37:22.21 +59:19:56.8
128.76796 -3.01784 galactic Cas Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.3259+59.3273 | 01:37:22.21 +59:19:56.8 (user input) | dubious (ATLAS) | (ATLAS) | (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 01:37:22.21 +59:19:56.8: 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 01:37:22.21 +59:19:56.8: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 31.3529* 01 37 22.21 +59 19 56.8 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.3259+59.3273,2461191.8529,10.05,0.05,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 J024.3259+59.3273 20260531.3529 10.05CV 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 31.3529 2461191.8529 9.71 02:09:05.47 +57:29:28.7
133.24504 -3.81727 galactic Per Second-epoch detections are separated by 7.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J032.2772+57.4959 | 02:09:05.67 +57:29:33.8 (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 02:09:05.47 +57:29:28.7: 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 02:09:05.47 +57:29:28.7: 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 31.3529* 02 09 05.47 +57 29 28.7 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
ATO J032.2772+57.4959,2461191.8529,9.71,0.05,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
ATO J032.2772+57.4959 20260531.3529 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 31.3529 2461191.8529 9.62 02:25:12.14 +58:09:07.0
135.06065 -2.49459 galactic Per Second-epoch detections are separated by 7.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.3009+58.1486 | 02:25:12.34 +58:09:10.8 (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 02:25:12.14 +58:09:07.0: 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 02:25:12.14 +58:09:07.0: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 31.3529* 02 25 12.14 +58 09 07.0 9.6 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 J036.3009+58.1486,2461191.8529,9.62,0.05,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
ATO J036.3009+58.1486 20260531.3529 9.62CV 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 31.3529 2461191.8529 10.17 00:42:45.77 +63:38:26.5
121.96908 0.78516 galactic Cas Second-epoch detections are separated by 2.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 523948076961126400 | 00:42:47.96 +63:38:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.470+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:42:45.77 +63:38:26.5: 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 00:42:45.77 +63:38:26.5: 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 31.3529* 00 42 45.77 +63 38 26.5 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523948076961126400,2461191.8529,10.17,0.05,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 523948076961126400 20260531.3529 10.17CV 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 31.3529 2461191.8529 9.16 02:37:27.18 +57:28:29.8
136.82839 -2.50823 galactic Per Second-epoch detections are separated by 8.0" and 4.9 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 457916253319743616 | 02:37:31.82 +57:28:17.3 (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 02:37:27.18 +57:28:29.8: 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 02:37:27.18 +57:28:29.8: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 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 31.3529* 02 37 27.18 +57 28 29.8 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 457916253319743616,2461191.8529,9.16,0.05,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 457916253319743616 20260531.3529 9.16CV 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 31.3529 2461191.8529 9.36 00:36:55.27 +62:40:47.8
121.26714 -0.14487 galactic Cas Second-epoch detections are separated by 0.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 00:36:55.27 +62:40:47.8: 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 00:36:55.27 +62:40:47.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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 31.3529* 00 36 55.27 +62 40 47.8 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
Gaia DR3 430706329831264640,2461191.8529,9.36,0.05,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
Gaia DR3 430706329831264640 20260531.3529 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 31.3529 2461191.8529 8.72 02:19:45.14 +57:01:17.6
134.76446 -3.80743 galactic Per Second-epoch detections are separated by 0.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458361216240219648 | 02:19:47.59 +57:00:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.070+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:45.14 +57:01:17.6: 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 02:19:45.14 +57:01:17.6: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 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 31.3529* 02 19 45.14 +57 01 17.6 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 458361216240219648,2461191.8529,8.72,0.05,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 458361216240219648 20260531.3529 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 31.3529 2461191.8529 6.71 02:29:09.11 +56:37:12.5
136.11226 -3.73027 galactic Per Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457593928911905280 | 02:29:09.04 +56:37:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 02:29:09.11 +56:37:12.5: 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 02:29:09.11 +56:37:12.5: 9.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.24 +/- 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 31.3529* 02 29 09.11 +56 37 12.5 6.7 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 457593928911905280,2461191.8529,6.71,0.05,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
Gaia DR3 457593928911905280 20260531.3529 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 31.3529 2461191.8529 6.78 02:25:27.59 +56:46:56.3
135.58007 -3.76271 galactic Per Second-epoch detections are separated by 0.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:25:27.59 +56:46:56.3: 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 02:25:27.59 +56:46:56.3: 9.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.69 +/- 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 31.3529* 02 25 27.59 +56 46 56.3 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+56.7792,2461191.8529,6.78,0.05,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
ATO J036.3787+56.7792 20260531.3529 6.78CV 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 31.3529 2461191.8529 6.75 02:32:05.00 +56:39:58.8
136.46943 -3.53673 galactic Per Second-epoch detections are separated by 0.5" and 4.0 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 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 J-Ks=0.033+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:05.00 +56:39:58.8: 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 02:32:05.00 +56:39:58.8: 9.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.33 +/- 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 31.3529* 02 32 05.00 +56 39 58.8 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 J038.0368+56.6612,2461191.8529,6.75,0.05,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 J038.0368+56.6612 20260531.3529 6.75CV 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 31.3529 2461191.8529 6.81 02:32:34.50 +57:29:15.5
136.21889 -2.75160 galactic Per Second-epoch detections are separated by 0.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458019817868936448 | 02:32:34.57 +57:29:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8III 1978A&AS...32...25R BD+56 650 J-Ks=0.631+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:34.50 +57:29:15.5: 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 02:32:34.50 +57:29:15.5: 9.46 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.46 +/- 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 31.3529* 02 32 34.50 +57 29 15.5 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
Gaia DR3 458019817868936448,2461191.8529,6.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458019817868936448 20260531.3529 6.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 6.83 02:27:57.93 +56:02:37.4
136.17092 -4.32682 galactic Per Second-epoch detections are separated by 0.3" and 4.0 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 J037.0041+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
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:57.93 +56:02:37.4: 12.10 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:57.93 +56:02:37.4: 9.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.52 +/- 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 31.3529* 02 27 57.93 +56 02 37.4 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 J037.0041+56.0452,2461191.8529,6.83,0.05,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
ATO J037.0041+56.0452 20260531.3529 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 31.3529 2461191.8529 6.91 02:29:09.98 +56:27:11.8
136.17582 -3.88463 galactic Per Second-epoch detections are separated by 0.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:29:09.98 +56:27:11.8: 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 02:29:09.98 +56:27:11.8: 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 31.3529* 02 29 09.98 +56 27 11.8 6.9 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 457590355506120064,2461191.8529,6.91,0.05,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
Gaia DR3 457590355506120064 20260531.3529 6.91CV 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 31.3529 2461191.8529 6.88 02:31:25.66 +55:59:07.0
136.64320 -4.20159 galactic Per Second-epoch detections are separated by 1.2" and 3.8 pix
The object was found in VSX19" 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 02:31:25.66 +55:59:07.0: 12.30 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:25.66 +55:59:07.0: 9.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.56 +/- 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 31.3529* 02 31 25.66 +55 59 07.0 6.9 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 457343205908261760,2461191.8529,6.88,0.05,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 457343205908261760 20260531.3529 6.88CV 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 31.3529 2461191.8529 6.97 02:22:03.80 +56:31:26.9
135.23224 -4.16782 galactic Per Second-epoch detections are separated by 0.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.5283+56.5245 | 02:22:03.78 +56:31:27.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.139+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:03.80 +56:31:26.9: 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 02:22:03.80 +56:31:26.9: 9.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.51 +/- 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 31.3529* 02 22 03.80 +56 31 26.9 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 J035.5283+56.5245,2461191.8529,6.97,0.05,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 J035.5283+56.5245 20260531.3529 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 31.3529 2461191.8529 6.91 02:34:10.16 +55:50:00.1
137.05739 -4.19525 galactic Per Second-epoch detections are separated by 2.0" and 4.0 pix
The object was found in VSX 8" 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 02:34:10.16 +55:50:00.1: 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 02:34:10.16 +55:50:00.1: 9.73 +/- 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 31.3529* 02 34 10.16 +55 50 00.1 6.9 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 457311320070532608,2461191.8529,6.91,0.05,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
Gaia DR3 457311320070532608 20260531.3529 6.91CV 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 31.3529 2461191.8529 6.99 02:32:46.00 +56:48:25.9
136.50259 -3.37082 galactic Per Second-epoch detections are separated by 0.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 J-Ks=0.090+/-0.047 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:46.00 +56:48:25.9: 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 02:32:46.00 +56:48:25.9: 9.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.56 +/- 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 31.3529* 02 32 46.00 +56 48 25.9 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 J038.2081+56.8041,2461191.8529,6.99,0.05,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
ATO J038.2081+56.8041 20260531.3529 6.99CV 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 31.3529 2461191.8529 7.00 02:34:34.19 +56:21:55.6
136.90242 -3.68307 galactic Per Second-epoch detections are separated by 0.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:34:34.19 +56:21:55.6: 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 02:34:34.19 +56:21:55.6: 9.62 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.62 +/- 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 31.3529* 02 34 34.19 +56 21 55.6 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
Gaia DR3 457749475453771648,2461191.8529,7.00,0.05,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
Gaia DR3 457749475453771648 20260531.3529 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 31.3529 2461191.8529 7.02 02:35:37.81 +57:29:13.2
136.59828 -2.59377 galactic Per Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458101181736200448 | 02:35:37.84 +57:29:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1928AnHar.100...49C HD 236971 J-Ks=0.171+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:37.81 +57:29:13.2: 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 02:35:37.81 +57:29:13.2: 9.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.60 +/- 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 31.3529* 02 35 37.81 +57 29 13.2 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
Gaia DR3 458101181736200448,2461191.8529,7.02,0.05,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
Gaia DR3 458101181736200448 20260531.3529 7.02CV 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 31.3529 2461191.8529 7.09 02:25:20.43 +56:51:13.3
135.53935 -3.70179 galactic Per Second-epoch detections are separated by 0.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457640417645156608 | 02:25:20.39 +56:51:13.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +56 49 J-Ks=0.067+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:20.43 +56:51:13.3: 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 02:25:20.43 +56:51:13.3: 9.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.67 +/- 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 31.3529* 02 25 20.43 +56 51 13.3 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 457640417645156608,2461191.8529,7.09,0.05,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
Gaia DR3 457640417645156608 20260531.3529 7.09CV 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 31.3529 2461191.8529 7.07 02:34:43.96 +56:06:06.8
137.02586 -3.91717 galactic Per Second-epoch detections are separated by 1.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:34:43.96 +56:06:06.8: 12.33 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:43.96 +56:06:06.8: 9.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.77 +/- 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 31.3529* 02 34 43.96 +56 06 06.8 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
ATO J038.6785+56.0961,2461191.8529,7.07,0.05,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
ATO J038.6785+56.0961 20260531.3529 7.07CV 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 31.3529 2461191.8529 7.05 02:27:24.36 +56:23:03.8
135.97400 -4.03780 galactic Per Second-epoch detections are separated by 0.1" and 3.9 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 +56:23:03.8: 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 02:27:24.36 +56:23:03.8: 9.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.60 +/- 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 31.3529* 02 27 24.36 +56 23 03.8 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
Gaia DR3 457563554909169536,2461191.8529,7.05,0.05,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
Gaia DR3 457563554909169536 20260531.3529 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 31.3529 2461191.8529 7.11 02:30:53.64 +56:14:28.0
136.47763 -3.99252 galactic Per Second-epoch detections are separated by 0.2" and 4.0 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 457384093997742208 | 02:30:54.14 +56:14:26.8 (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 02:30:53.64 +56:14:28.0: 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 02:30:53.64 +56:14:28.0: 10.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.03 +/- 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 31.3529* 02 30 53.64 +56 14 28.0 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 457384093997742208,2461191.8529,7.11,0.05,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 457384093997742208 20260531.3529 7.11CV 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 31.3529 2461191.8529 7.11 02:33:34.24 +55:54:24.4
136.95131 -4.15991 galactic Per Second-epoch detections are separated by 2.5" and 4.0 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 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 02:33:34.24 +55:54:24.4: 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 02:33:34.24 +55:54:24.4: 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 31.3529* 02 33 34.24 +55 54 24.4 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
ATO J038.3939+55.9184,2461191.8529,7.11,0.05,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
ATO J038.3939+55.9184 20260531.3529 7.11CV 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 31.3529 2461191.8529 7.18 02:24:11.84 +56:35:43.1
135.48382 -3.99891 galactic Per Second-epoch detections are separated by 1.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:24:11.84 +56:35:43.1: 8.78 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:11.84 +56:35:43.1: 9.78 +/- 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 31.3529* 02 24 11.84 +56 35 43.1 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 457537269710765824,2461191.8529,7.18,0.05,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 457537269710765824 20260531.3529 7.18CV 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 31.3529 2461191.8529 7.22 02:23:35.43 +56:34:27.3
135.41276 -4.04790 galactic Per Second-epoch detections are separated by 0.9" and 3.9 pix
The object was found in VSX 1" V0361 Per
Type: GCAS
# Max. Min./Amp. JD0 Period
9.060 V 9.640 V B1.5IIIpe
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 02:23:35.43 +56:34:27.3: 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 02:23:35.43 +56:34:27.3: 9.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.51 +/- 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 31.3529* 02 23 35.43 +56 34 27.3 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
V0361 Per,2461191.8529,7.22,0.05,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
V0361 Per 20260531.3529 7.22CV 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 31.3529 2461191.8529 7.24 02:37:08.47 +57:25:21.7
136.81061 -2.57284 galactic Per Second-epoch detections are separated by 0.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:37:08.47 +57:25:21.7: 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 02:37:08.47 +57:25:21.7: 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 31.3529* 02 37 08.47 +57 25 21.7 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
ATO J039.2772+57.4158,2461191.8529,7.24,0.05,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 J039.2772+57.4158 20260531.3529 7.24CV 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 31.3529 2461191.8529 7.24 02:36:28.42 +57:11:45.9
136.81743 -2.81662 galactic Per Second-epoch detections are separated by 0.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457813144048325248 | 02:36:28.37 +57:11:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1928AnHar.100...49C HD 236972 J-Ks=0.167+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:28.42 +57:11:45.9: 12.91 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:28.42 +57:11:45.9: 9.88 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.88 +/- 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 31.3529* 02 36 28.42 +57 11 45.9 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 457813144048325248,2461191.8529,7.24,0.05,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 457813144048325248 20260531.3529 7.24CV 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 31.3529 2461191.8529 7.33 02:35:52.02 +57:47:22.1
136.50892 -2.30304 galactic Cas Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:35:52.02 +57:47:22.1: 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 02:35:52.02 +57:47:22.1: 9.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.95 +/- 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 31.3529* 02 35 52.02 +57 47 22.1 7.3 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 458114582034037760,2461191.8529,7.33,0.05,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 458114582034037760 20260531.3529 7.33CV 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 31.3529 2461191.8529 7.33 02:23:26.39 +56:06:42.0
135.55503 -4.48868 galactic Per Second-epoch detections are separated by 1.1" and 4.0 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 457520296000263808 | 02:23:26.45 +56:06:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.676+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:26.39 +56:06:42.0: 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 02:23:26.39 +56:06:42.0: 10.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.06 +/- 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 31.3529* 02 23 26.39 +56 06 42.0 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
Gaia DR3 457520296000263808,2461191.8529,7.33,0.05,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 457520296000263808 20260531.3529 7.33CV 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 31.3529 2461191.8529 7.38 02:36:33.26 +57:54:38.3
136.54538 -2.15568 galactic Cas Second-epoch detections are separated by 1.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:36:33.26 +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 02:36:33.26 +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 31.3529* 02 36 33.26 +57 54 38.3 7.4 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 458140386197476352,2461191.8529,7.38,0.05,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 458140386197476352 20260531.3529 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 31.3529 2461191.8529 7.34 02:27:20.56 +56:01:48.1
136.09466 -4.37122 galactic Per Second-epoch detections are separated by 0.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457461162889223552 | 02:27:20.64 +56:01:46.2 (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 02:27:20.56 +56:01:48.1: 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 02:27:20.56 +56:01:48.1: 10.16 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.16 +/- 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 31.3529* 02 27 20.56 +56 01 48.1 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
Gaia DR3 457461162889223552,2461191.8529,7.34,0.05,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
Gaia DR3 457461162889223552 20260531.3529 7.34CV 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 31.3529 2461191.8529 7.35 02:36:36.25 +57:46:59.1
136.60183 -2.27028 galactic Cas Second-epoch detections are separated by 0.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:36:36.25 +57:46:59.1: 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 02:36:36.25 +57:46:59.1: 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 31.3529* 02 36 36.25 +57 46 59.1 7.3 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 458112864047109120,2461191.8529,7.35,0.05,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 458112864047109120 20260531.3529 7.35CV 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 31.3529 2461191.8529 7.38 02:18:01.27 +56:15:42.4
134.79255 -4.60311 galactic Per Second-epoch detections are separated by 0.7" and 4.0 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 456810595604427392 | 02:18:01.38 +56:15:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 2013AJ....145..102L PM J02180+5616
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:01.27 +56:15:42.4: 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 02:18:01.27 +56:15:42.4: 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 31.3529* 02 18 01.27 +56 15 42.4 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 456810595604427392,2461191.8529,7.38,0.05,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 456810595604427392 20260531.3529 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 31.3529 2461191.8529 7.38 02:32:05.68 +57:22:03.0
136.20469 -2.88729 galactic Per Second-epoch detections are separated by 0.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:32:05.68 +57:22:03.0: 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 02:32:05.68 +57:22:03.0: 10.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.20 +/- 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 31.3529* 02 32 05.68 +57 22 03.0 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+57.3766,2461191.8529,7.38,0.05,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
ATO J038.0242+57.3766 20260531.3529 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 31.3529 2461191.8529 7.39 02:19:46.66 +56:22:25.8
134.98557 -4.41646 galactic Per Second-epoch detections are separated by 1.0" and 4.0 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 458272121436434944 | 02:19:46.67 +56:22:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.132+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:46.66 +56:22:25.8: 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 02:19:46.66 +56:22:25.8: 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 31.3529* 02 19 46.66 +56 22 25.8 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 458272121436434944,2461191.8529,7.39,0.05,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 458272121436434944 20260531.3529 7.39CV 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 31.3529 2461191.8529 7.42 02:34:05.22 +56:25:31.7
136.81741 -3.65358 galactic Per Second-epoch detections are separated by 0.5" and 4.0 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 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 02:34:05.22 +56:25:31.7: 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 02:34:05.22 +56:25:31.7: 10.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.20 +/- 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 31.3529* 02 34 05.22 +56 25 31.7 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 457750815483540992,2461191.8529,7.42,0.05,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 457750815483540992 20260531.3529 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 31.3529 2461191.8529 7.47 02:21:55.21 +56:25:08.8
135.24980 -4.27324 galactic Per Second-epoch detections are separated by 0.6" and 4.0 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 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 02:21:55.21 +56:25:08.8: 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 02:21:55.21 +56:25:08.8: 10.01 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.01 +/- 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 31.3529* 02 21 55.21 +56 25 08.8 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 J035.4640+56.4218,2461191.8529,7.47,0.05,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 J035.4640+56.4218 20260531.3529 7.47CV 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 31.3529 2461191.8529 7.42 02:29:11.88 +56:17:58.5
136.23676 -4.02586 galactic Per Second-epoch detections are separated by 0.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:29:11.88 +56:17:58.5: 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 02:29:11.88 +56:17:58.5: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.26 +/- 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 31.3529* 02 29 11.88 +56 17 58.5 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
ATO J037.2903+56.3099,2461191.8529,7.42,0.05,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
ATO J037.2903+56.3099 20260531.3529 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 31.3529 2461191.8529 7.45 02:31:25.67 +56:07:05.3
136.59299 -4.07852 galactic Per Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:31:25.67 +56:07:05.3: 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 02:31:25.67 +56:07:05.3: 10.68 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.68 +/- 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 31.3529* 02 31 25.67 +56 07 05.3 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 457379661591549312,2461191.8529,7.45,0.05,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 457379661591549312 20260531.3529 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 31.3529 2461191.8529 7.47 02:32:15.38 +56:38:50.2
136.49871 -3.54534 galactic Per Second-epoch detections are separated by 0.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:32:15.38 +56:38:50.2: 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 02:32:15.38 +56:38:50.2: 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 31.3529* 02 32 15.38 +56 38 50.2 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 457772187240678912,2461191.8529,7.47,0.05,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
Gaia DR3 457772187240678912 20260531.3529 7.47CV 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 31.3529 2461191.8529 7.49 02:30:44.93 +56:56:12.3
136.19785 -3.35505 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:30:44.93 +56:56:12.3: 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 02:30:44.93 +56:56:12.3: 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 31.3529* 02 30 44.93 +56 56 12.3 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 J037.6828+56.9432,2461191.8529,7.49,0.05,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 J037.6828+56.9432 20260531.3529 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 31.3529 2461191.8529 7.52 02:21:50.35 +56:34:31.6
135.18549 -4.13023 galactic Per Second-epoch detections are separated by 0.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458284662741800064 | 02:21:50.31 +56:34:32.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +56 35 J-Ks=0.027+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:50.35 +56:34:31.6: 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 02:21:50.35 +56:34:31.6: 10.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.08 +/- 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 31.3529* 02 21 50.35 +56 34 31.6 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
Gaia DR3 458284662741800064,2461191.8529,7.52,0.05,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 458284662741800064 20260531.3529 7.52CV 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 31.3529 2461191.8529 7.53 02:26:59.12 +56:01:57.0
136.04710 -4.38699 galactic Per Second-epoch detections are separated by 0.3" and 4.0 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 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 02:26:59.12 +56:01:57.0: 12.18 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:59.12 +56:01:57.0: 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 31.3529* 02 26 59.12 +56 01 57.0 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 457460991090535808,2461191.8529,7.53,0.05,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 457460991090535808 20260531.3529 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 31.3529 2461191.8529 7.57 02:22:35.34 +56:18:13.6
135.37685 -4.34961 galactic Per Second-epoch detections are separated by 0.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458276622563145984 | 02:22:35.42 +56:18:12.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.639+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:35.34 +56:18:13.6: 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 02:22:35.34 +56:18:13.6: 10.31 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.31 +/- 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 31.3529* 02 22 35.34 +56 18 13.6 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 458276622563145984,2461191.8529,7.57,0.05,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 458276622563145984 20260531.3529 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 31.3529 2461191.8529 7.54 02:26:48.88 +55:59:11.6
136.04143 -4.43845 galactic Per Second-epoch detections are separated by 0.5" and 4.0 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 457459444902338944 | 02:26:48.89 +55:59:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.073+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:48.88 +55:59:11.6: 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 02:26:48.88 +55:59:11.6: 10.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.20 +/- 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 31.3529* 02 26 48.88 +55 59 11.6 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
Gaia DR3 457459444902338944,2461191.8529,7.54,0.05,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
Gaia DR3 457459444902338944 20260531.3529 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 31.3529 2461191.8529 7.59 02:32:55.20 +56:39:40.1
136.57791 -3.49778 galactic Per Second-epoch detections are separated by 0.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2188+56.6593 | 02:32:55.49 +56:39:40.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.759+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:55.20 +56:39:40.1: 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 02:32:55.20 +56:39:40.1: 10.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.33 +/- 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 31.3529* 02 32 55.20 +56 39 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
ATO J038.2188+56.6593,2461191.8529,7.59,0.05,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
ATO J038.2188+56.6593 20260531.3529 7.59CV 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 31.3529 2461191.8529 7.63 02:33:01.81 +57:02:07.5
136.44858 -3.14616 galactic Per Second-epoch detections are separated by 0.3" and 3.8 pix
The object was found in VSX 3" 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 02:33:01.81 +57:02:07.5: 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 02:33:01.81 +57:02:07.5: 10.91 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 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 31.3529* 02 33 01.81 +57 02 07.5 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
GSC 03695-01369,2461191.8529,7.63,0.05,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
GSC 03695-01369 20260531.3529 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 31.3529 2461191.8529 7.63 02:20:54.06 +56:16:37.3
135.16537 -4.45500 galactic Per Second-epoch detections are separated by 1.1" and 3.8 pix
The object was found in VSX 3" 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 02:20:54.06 +56:16:37.3: 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 02:20:54.06 +56:16:37.3: 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 31.3529* 02 20 54.06 +56 16 37.3 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+561634.7,2461191.8529,7.63,0.05,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
ASASSN-V J022054.22+561634.7 20260531.3529 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 31.3529 2461191.8529 7.65 02:31:06.51 +56:30:41.5
136.40346 -3.73073 galactic Per Second-epoch detections are separated by 0.8" and 4.0 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 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 02:31:06.51 +56:30:41.5: 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 02:31:06.51 +56:30:41.5: 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 31.3529* 02 31 06.51 +56 30 41.5 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 457581971731866368,2461191.8529,7.65,0.05,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 457581971731866368 20260531.3529 7.65CV 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 31.3529 2461191.8529 7.71 02:24:43.69 +56:59:33.9
135.41171 -3.60134 galactic Per Second-epoch detections are separated by 0.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.1697+56.9953 | 02:24:43.70 +56:59:33.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +56 44 J-Ks=-0.015+/-0.033 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:43.69 +56:59:33.9: 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 02:24:43.69 +56:59:33.9: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 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 31.3529* 02 24 43.69 +56 59 33.9 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 J036.1697+56.9953,2461191.8529,7.71,0.05,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 J036.1697+56.9953 20260531.3529 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 31.3529 2461191.8529 7.71 02:38:46.64 +57:49:57.9
136.84772 -2.10945 galactic Cas Second-epoch detections are separated by 1.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 J-Ks=0.250+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:46.64 +57:49:57.9: 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 02:38:46.64 +57:49:57.9: 10.35 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.35 +/- 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 31.3529* 02 38 46.64 +57 49 57.9 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 457946459832991616,2461191.8529,7.71,0.05,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
Gaia DR3 457946459832991616 20260531.3529 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 31.3529 2461191.8529 7.72 02:37:36.83 +57:51:16.3
136.69702 -2.15141 galactic Cas Second-epoch detections are separated by 0.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:37:36.83 +57:51:16.3: 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 02:37:36.83 +57:51:16.3: 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 31.3529* 02 37 36.83 +57 51 16.3 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
ATO J039.3909+57.8574,2461191.8529,7.72,0.05,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
ATO J039.3909+57.8574 20260531.3529 7.72CV 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 31.3529 2461191.8529 7.72 02:37:55.04 +57:39:03.5
136.81537 -2.32197 galactic Cas Second-epoch detections are separated by 0.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.4658+57.6504 | 02:37:55.25 +57:39:01.7 (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 02:37:55.04 +57:39:03.5: 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 02:37:55.04 +57:39:03.5: 10.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.49 +/- 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 31.3529* 02 37 55.04 +57 39 03.5 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
ATO J039.4658+57.6504,2461191.8529,7.72,0.05,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
ATO J039.4658+57.6504 20260531.3529 7.72CV 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 31.3529 2461191.8529 7.71 02:22:06.87 +56:07:53.3
135.37435 -4.53409 galactic Per Second-epoch detections are separated by 0.3" and 3.9 pix
The object was found in VSX 0" V0758 Per
Type: EA
# Max. Min./Amp. JD0 Period
10.600 R1 10.900 R1 2451450.61000 5.675130000000
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 02:22:06.87 +56:07:53.3: 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 02:22:06.87 +56:07:53.3: 10.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.49 +/- 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 31.3529* 02 22 06.87 +56 07 53.3 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
V0758 Per,2461191.8529,7.71,0.05,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
V0758 Per 20260531.3529 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 31.3529 2461191.8529 7.69 02:34:03.56 +56:30:43.8
136.78033 -3.57509 galactic Per Second-epoch detections are separated by 1.3" and 4.0 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 02:34:03.56 +56:30:43.8: 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 02:34:03.56 +56:30:43.8: 10.35 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.35 +/- 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 31.3529* 02 34 03.56 +56 30 43.8 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 457755763285796480,2461191.8529,7.69,0.05,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 457755763285796480 20260531.3529 7.69CV 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 31.3529 2461191.8529 7.79 02:21:20.56 +56:29:12.2
135.15142 -4.23702 galactic Per Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458294214749131648 | 02:21:20.46 +56:29:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.785+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:20.56 +56:29:12.2: 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 02:21:20.56 +56:29:12.2: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.58 +/- 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 31.3529* 02 21 20.56 +56 29 12.2 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 458294214749131648,2461191.8529,7.79,0.05,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 458294214749131648 20260531.3529 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 31.3529 2461191.8529 7.76 02:32:04.85 +56:49:24.8
136.40941 -3.39137 galactic Per Second-epoch detections are separated by 0.7" and 4.0 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 457963193027127424 | 02:32:04.79 +56:49:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.077+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:04.85 +56:49:24.8: 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 02:32:04.85 +56:49:24.8: 10.35 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.35 +/- 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 31.3529* 02 32 04.85 +56 49 24.8 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 457963193027127424,2461191.8529,7.76,0.05,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
Gaia DR3 457963193027127424 20260531.3529 7.76CV 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 31.3529 2461191.8529 7.74 02:30:12.39 +56:11:25.0
136.40783 -4.07540 galactic Per Second-epoch detections are separated by 0.1" and 3.9 pix
The object was found in VSX22" 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 02:30:12.39 +56:11:25.0: 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 02:30:12.39 +56:11:25.0: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.58 +/- 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 31.3529* 02 30 12.39 +56 11 25.0 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
ZTF J023014.84+561117.4,2461191.8529,7.74,0.05,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
ZTF J023014.84+561117.4 20260531.3529 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 31.3529 2461191.8529 7.83 02:22:10.20 +56:24:23.0
135.28672 -4.27331 galactic Per Second-epoch detections are separated by 1.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:22:10.20 +56:24:23.0: 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 02:22:10.20 +56:24:23.0: 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 31.3529* 02 22 10.20 +56 24 23.0 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 458278477988992384,2461191.8529,7.83,0.05,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
Gaia DR3 458278477988992384 20260531.3529 7.83CV 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 31.3529 2461191.8529 7.85 02:27:48.50 +57:05:55.4
135.76540 -3.35225 galactic Per Second-epoch detections are separated by 0.6" and 3.8 pix
The object was found in VSX 5" DP Per
Type: LB
# Max. Min./Amp. JD0 Period
14.200 pg 15.100 pg 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 02:27:48.50 +57:05:55.4: 10.27 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:48.50 +57:05:55.4: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 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 31.3529* 02 27 48.50 +57 05 55.4 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
DP Per,2461191.8529,7.85,0.05,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
DP Per 20260531.3529 7.85CV 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 31.3529 2461191.8529 7.78 02:28:50.78 +56:20:48.8
136.17385 -3.99984 galactic Per Second-epoch detections are separated by 0.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457554415218933120 | 02:28:50.80 +56:20:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.101+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:50.78 +56:20:48.8: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:50.78 +56:20:48.8: 10.62 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.62 +/- 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 31.3529* 02 28 50.78 +56 20 48.8 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 457554415218933120,2461191.8529,7.78,0.05,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
Gaia DR3 457554415218933120 20260531.3529 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 31.3529 2461191.8529 7.79 02:33:48.46 +57:01:46.2
136.54867 -3.11104 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4387+57.0274 | 02:33:48.47 +57:01:46.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.306+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:48.46 +57:01:46.2: 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 02:33:48.46 +57:01:46.2: 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 31.3529* 02 33 48.46 +57 01 46.2 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 J038.4387+57.0274,2461191.8529,7.79,0.05,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
ATO J038.4387+57.0274 20260531.3529 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 31.3529 2461191.8529 7.83 02:19:52.94 +56:15:40.6
135.03720 -4.51760 galactic Per Second-epoch detections are separated by 1.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:19:52.94 +56:15:40.6: 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 02:19:52.94 +56:15:40.6: 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 31.3529* 02 19 52.94 +56 15 40.6 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 458262328911050880,2461191.8529,7.83,0.05,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
Gaia DR3 458262328911050880 20260531.3529 7.83CV 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 31.3529 2461191.8529 7.79 02:25:28.14 +56:11:20.3
135.79293 -4.31675 galactic Per Second-epoch detections are separated by 0.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:25:28.14 +56:11:20.3: 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 02:25:28.14 +56:11:20.3: 10.41 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.41 +/- 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 31.3529* 02 25 28.14 +56 11 20.3 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 J036.3836+56.1834,2461191.8529,7.79,0.05,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
ATO J036.3836+56.1834 20260531.3529 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 31.3529 2461191.8529 7.88 02:33:49.33 +57:35:12.0
136.33573 -2.59606 galactic Per Second-epoch detections are separated by 1.0" and 3.9 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 02:33:49.33 +57:35:12.0: 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 02:33:49.33 +57:35:12.0: 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 31.3529* 02 33 49.33 +57 35 12.0 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 J023348.90+573530.8,2461191.8529,7.88,0.05,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
ZTF J023348.90+573530.8 20260531.3529 7.88CV 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 31.3529 2461191.8529 7.87 02:19:48.61 +56:23:45.8
134.98234 -4.39401 galactic Per Second-epoch detections are separated by 0.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458272258875379968 | 02:19:48.70 +56:23:44.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:48.61 +56:23:45.8: 13.20 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:48.61 +56:23:45.8: 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 31.3529* 02 19 48.61 +56 23 45.8 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 458272258875379968,2461191.8529,7.87,0.05,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
Gaia DR3 458272258875379968 20260531.3529 7.87CV 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 31.3529 2461191.8529 7.84 02:25:20.33 +56:12:13.7
135.77067 -4.30933 galactic Per Second-epoch detections are separated by 0.7" and 4.0 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 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 02:25:20.33 +56:12:13.7: 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 02:25:20.33 +56:12:13.7: 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 31.3529* 02 25 20.33 +56 12 13.7 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 457513149174786176,2461191.8529,7.84,0.05,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
Gaia DR3 457513149174786176 20260531.3529 7.84CV 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 31.3529 2461191.8529 7.92 02:24:41.99 +56:55:48.0
135.43028 -3.66141 galactic Per Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:24:41.99 +56:55:48.0: 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 02:24:41.99 +56:55:48.0: 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 31.3529* 02 24 41.99 +56 55 48.0 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+56.9296,2461191.8529,7.92,0.05,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
ATO J036.1620+56.9296 20260531.3529 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 31.3529 2461191.8529 7.92 02:31:11.98 +57:09:48.2
136.16963 -3.12197 galactic Per Second-epoch detections are separated by 0.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:31:11.98 +57:09:48.2: 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 02:31:11.98 +57:09:48.2: 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 31.3529* 02 31 11.98 +57 09 48.2 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
ATO J037.7864+57.1721,2461191.8529,7.92,0.05,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
ATO J037.7864+57.1721 20260531.3529 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 31.3529 2461191.8529 7.89 02:19:36.43 +56:14:20.7
135.00855 -4.55133 galactic Per Second-epoch detections are separated by 1.9" and 4.0 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 J034.8921+56.2341 | 02:19:36.45 +56:14:19.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +56 44 J-Ks=-0.055+/-0.032 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:36.43 +56:14:20.7: 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 02:19:36.43 +56:14:20.7: 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 31.3529* 02 19 36.43 +56 14 20.7 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 J034.8921+56.2341,2461191.8529,7.89,0.05,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 J034.8921+56.2341 20260531.3529 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 31.3529 2461191.8529 7.91 02:18:48.83 +56:19:01.6
134.87832 -4.51451 galactic Per Second-epoch detections are separated by 1.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.7162+56.3174 | 02:18:48.78 +56:19:01.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5) J-Ks=0.259+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:48.83 +56:19:01.6: 12.15 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:48.83 +56:19:01.6: 10.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.60 +/- 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 31.3529* 02 18 48.83 +56 19 01.6 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
ATO J034.7162+56.3174,2461191.8529,7.91,0.05,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 J034.7162+56.3174 20260531.3529 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 31.3529 2461191.8529 7.89 02:32:45.28 +57:08:07.9
136.37566 -3.06792 galactic Per Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:32:45.28 +57:08:07.9: 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 02:32:45.28 +57:08:07.9: 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 31.3529* 02 32 45.28 +57 08 07.9 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 J038.1901+57.1255,2461191.8529,7.89,0.05,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 J038.1901+57.1255 20260531.3529 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 31.3529 2461191.8529 7.92 02:18:48.46 +56:17:54.5
134.88372 -4.53238 galactic Per Second-epoch detections are separated by 0.4" and 3.9 pix
The object was found in VSX11" Gaia DR3 458265180769332096
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.240 G 14.270 G 0.029804400000 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 02:18:48.46 +56:17:54.5: 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 02:18:48.46 +56:17:54.5: 10.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.56 +/- 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 31.3529* 02 18 48.46 +56 17 54.5 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 458265180769332096,2461191.8529,7.92,0.05,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 458265180769332096 20260531.3529 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 31.3529 2461191.8529 7.96 02:35:33.89 +57:09:19.1
136.72005 -2.90248 galactic Per Second-epoch detections are separated by 0.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457812216335433344 | 02:35:34.20 +57:09:17.0 (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 02:35:33.89 +57:09:19.1: 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 02:35:33.89 +57:09:19.1: 10.92 +/- 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 31.3529* 02 35 33.89 +57 09 19.1 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 457812216335433344,2461191.8529,7.96,0.05,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 457812216335433344 20260531.3529 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 31.3529 2461191.8529 7.92 02:36:19.72 +57:15:27.8
136.77506 -2.76770 galactic Per Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:36:19.72 +57:15:27.8: 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 02:36:19.72 +57:15:27.8: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.58 +/- 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 31.3529* 02 36 19.72 +57 15 27.8 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 457907358450596352,2461191.8529,7.92,0.05,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 457907358450596352 20260531.3529 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 31.3529 2461191.8529 7.92 02:31:37.57 +56:33:36.1
136.45140 -3.65892 galactic Per Second-epoch detections are separated by 1.2" and 4.0 pix
The object was found in VSX16" 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 02:31:37.57 +56:33:36.1: 12.42 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:37.57 +56:33:36.1: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.77 +/- 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 31.3529* 02 31 37.57 +56 33 36.1 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 457583792795921664,2461191.8529,7.92,0.05,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 457583792795921664 20260531.3529 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 31.3529 2461191.8529 7.95 02:27:07.76 +56:33:53.6
135.87276 -3.88340 galactic Per Second-epoch detections are separated by 0.8" and 4.0 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 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 02:27:07.76 +56:33:53.6: 12.92 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:07.76 +56:33:53.6: 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 31.3529* 02 27 07.76 +56 33 53.6 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 457618423109114880,2461191.8529,7.95,0.05,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
Gaia DR3 457618423109114880 20260531.3529 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 31.3529 2461191.8529 7.94 02:30:51.92 +57:04:10.4
136.16277 -3.22597 galactic Per Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:30:51.92 +57:04:10.4: 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 02:30:51.92 +57:04:10.4: 10.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.56 +/- 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 31.3529* 02 30 51.92 +57 04 10.4 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 J037.7008+57.0647,2461191.8529,7.94,0.05,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
ATO J037.7008+57.0647 20260531.3529 7.94CV 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 31.3529 2461191.8529 7.97 02:23:42.80 +56:07:10.6
135.58808 -4.46792 galactic Per Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457520158561303680 | 02:23:42.86 +56:07:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:42.80 +56:07:10.6: 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 02:23:42.80 +56:07:10.6: 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 31.3529* 02 23 42.80 +56 07 10.6 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 457520158561303680,2461191.8529,7.97,0.05,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
Gaia DR3 457520158561303680 20260531.3529 7.97CV 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 31.3529 2461191.8529 7.98 02:20:32.12 +56:10:01.0
135.15484 -4.57580 galactic Per Second-epoch detections are separated by 1.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458249512728852864 | 02:20:32.03 +56:09:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.234+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:32.12 +56:10:01.0: 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 02:20:32.12 +56:10:01.0: 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 31.3529* 02 20 32.12 +56 10 01.0 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
Gaia DR3 458249512728852864,2461191.8529,7.98,0.05,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 458249512728852864 20260531.3529 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 31.3529 2461191.8529 8.02 02:24:09.75 +56:34:02.5
135.48916 -4.02676 galactic Per Second-epoch detections are separated by 1.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 31.3529* 02 24 09.75 +56 34 02.5 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
Gaia DR3 457537063552340736,2461191.8529,8.02,0.05,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
Gaia DR3 457537063552340736 20260531.3529 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 31.3529 2461191.8529 7.99 02:25:33.83 +56:34:21.8
135.66822 -3.95348 galactic Per Second-epoch detections are separated by 1.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:25:33.83 +56:34:21.8: 11.90 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:33.83 +56:34:21.8: 10.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.61 +/- 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 31.3529* 02 25 33.83 +56 34 21.8 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 J036.4026+56.5763,2461191.8529,7.99,0.05,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
ATO J036.4026+56.5763 20260531.3529 7.99CV 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 31.3529 2461191.8529 8.05 02:35:18.49 +57:31:39.8
136.54251 -2.57317 galactic Per Second-epoch detections are separated by 0.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458102246888080768 | 02:35:18.44 +57:31:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.222+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:18.49 +57:31:39.8: 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 02:35:18.49 +57:31:39.8: 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 31.3529* 02 35 18.49 +57 31 39.8 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 458102246888080768,2461191.8529,8.05,0.05,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
Gaia DR3 458102246888080768 20260531.3529 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 31.3529 2461191.8529 8.03 02:20:55.01 +56:23:18.7
135.12945 -4.34938 galactic Per Second-epoch detections are separated by 1.5" and 3.6 pix
The object was found in VSX 1" Gaia DR3 458269991132811904
Type: BE|GCAS|S
# Max. Min./Amp. JD0 Period
10.440 G 10.590 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 02:20:55.01 +56:23:18.7: 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 02:20:55.01 +56:23:18.7: 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 31.3529* 02 20 55.01 +56 23 18.7 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 458269991132811904,2461191.8529,8.03,0.05,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
Gaia DR3 458269991132811904 20260531.3529 8.03CV 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 31.3529 2461191.8529 8.05 02:33:30.04 +57:42:18.6
136.25040 -2.50319 galactic Per Second-epoch detections are separated by 0.8" and 3.8 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 02:33:30.04 +57:42:18.6: 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 02:33:30.04 +57:42:18.6: 10.68 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.68 +/- 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 31.3529* 02 33 30.04 +57 42 18.6 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 458028957566623360,2461191.8529,8.05,0.05,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
Gaia DR3 458028957566623360 20260531.3529 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 31.3529 2461191.8529 8.00 02:31:18.30 +55:53:50.8
136.66045 -4.28941 galactic Per Second-epoch detections are separated by 2.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.8193+55.8908 | 02:31:18.96 +55:53:50.0 (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 02:31:18.30 +55:53:50.8: 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 02:31:18.30 +55:53:50.8: 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 31.3529* 02 31 18.30 +55 53 50.8 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 J037.8193+55.8908,2461191.8529,8.00,0.05,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 J037.8193+55.8908 20260531.3529 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 31.3529 2461191.8529 8.01 02:31:38.41 +57:13:47.7
136.19988 -3.03787 galactic Per Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:31:38.41 +57:13:47.7: 9.41 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:38.41 +57:13:47.7: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.56 +/- 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 31.3529* 02 31 38.41 +57 13 47.7 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 457989856183731328,2461191.8529,8.01,0.05,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 457989856183731328 20260531.3529 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 31.3529 2461191.8529 8.01 02:27:33.21 +56:13:10.2
136.05313 -4.18401 galactic Per Second-epoch detections are separated by 0.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:27:33.21 +56:13:10.2: 11.42 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:33.21 +56:13:10.2: 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 31.3529* 02 27 33.21 +56 13 10.2 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 457557060918681856,2461191.8529,8.01,0.05,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 457557060918681856 20260531.3529 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 31.3529 2461191.8529 8.11 02:36:35.00 +57:36:36.2
136.66759 -2.43037 galactic Cas Second-epoch detections are separated by 0.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457921720823408384 | 02:36:35.02 +57:36:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9pSi? 1971AN....293..163Z BD+56 664 J-Ks=0.303+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:35.00 +57:36:36.2: 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 02:36:35.00 +57:36:36.2: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.71 +/- 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 31.3529* 02 36 35.00 +57 36 36.2 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 457921720823408384,2461191.8529,8.11,0.05,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 457921720823408384 20260531.3529 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 31.3529 2461191.8529 8.09 02:22:04.44 +57:10:39.1
135.00858 -3.55371 galactic Per Second-epoch detections are separated by 1.8" and 4.1 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 02:22:04.44 +57:10:39.1: 11.49 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:04.44 +57:10:39.1: 10.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.66 +/- 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 31.3529* 02 22 04.44 +57 10 39.1 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
NSV 800,2461191.8529,8.09,0.05,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 800 20260531.3529 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 31.3529 2461191.8529 8.04 02:31:58.58 +56:42:23.0
136.44061 -3.50522 galactic Per Second-epoch detections are separated by 1.2" and 4.0 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 J038.0032+56.7143 | 02:31:58.77 +56:42:23.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.052+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:58.58 +56:42:23.0: 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 02:31:58.58 +56:42:23.0: 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 31.3529* 02 31 58.58 +56 42 23.0 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 J038.0032+56.7143,2461191.8529,8.04,0.05,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 J038.0032+56.7143 20260531.3529 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 31.3529 2461191.8529 8.10 02:29:17.15 +57:14:29.9
135.89956 -3.14588 galactic Per Second-epoch detections are separated by 0.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458035554638504832 | 02:29:17.11 +57:14:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.781+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:17.15 +57:14:29.9: 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 02:29:17.15 +57:14:29.9: 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 31.3529* 02 29 17.15 +57 14 29.9 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 458035554638504832,2461191.8529,8.10,0.05,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 458035554638504832 20260531.3529 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 31.3529 2461191.8529 8.06 02:36:56.54 +57:06:44.6
136.90898 -2.86840 galactic Per Second-epoch detections are separated by 1.4" and 4.0 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 J039.2495+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 02:36:56.54 +57:06:44.6: 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 02:36:56.54 +57:06:44.6: 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 31.3529* 02 36 56.54 +57 06 44.6 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 J039.2495+57.1096,2461191.8529,8.06,0.05,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
ATO J039.2495+57.1096 20260531.3529 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 31.3529 2461191.8529 8.11 02:24:06.51 +56:29:59.7
135.50591 -4.09253 galactic Per Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:24:06.51 +56:29:59.7: 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 02:24:06.51 +56:29:59.7: 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 31.3529* 02 24 06.51 +56 29 59.7 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
ATO J036.0447+56.4918,2461191.8529,8.11,0.05,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
ATO J036.0447+56.4918 20260531.3529 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 31.3529 2461191.8529 8.15 02:24:33.48 +56:57:19.3
135.40318 -3.64450 galactic Per Second-epoch detections are separated by 0.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458392724117836672 | 02:24:33.44 +56:57:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.063+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:33.48 +56:57:19.3: 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 02:24:33.48 +56:57:19.3: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 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 31.3529* 02 24 33.48 +56 57 19.3 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
Gaia DR3 458392724117836672,2461191.8529,8.15,0.05,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
Gaia DR3 458392724117836672 20260531.3529 8.15CV 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 31.3529 2461191.8529 8.11 02:32:18.19 +56:21:26.4
136.61507 -3.81109 galactic Per Second-epoch detections are separated by 0.7" and 4.0 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 457388938720751616 | 02:32:18.57 +56:21:26.2 (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 02:32:18.19 +56:21:26.4: 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 02:32:18.19 +56:21:26.4: 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 31.3529* 02 32 18.19 +56 21 26.4 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 457388938720751616,2461191.8529,8.11,0.05,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 457388938720751616 20260531.3529 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 31.3529 2461191.8529 8.15 02:19:39.63 +56:20:11.7
134.98277 -4.45699 galactic Per Second-epoch detections are separated by 0.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.9014+56.3302 | 02:19:39.69 +56:20:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.622+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:39.63 +56:20:11.7: 9.86 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:39.63 +56:20:11.7: 10.93 +/- 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 31.3529* 02 19 39.63 +56 20 11.7 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
ATO J034.9014+56.3302,2461191.8529,8.15,0.05,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
ATO J034.9014+56.3302 20260531.3529 8.15CV 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 31.3529 2461191.8529 8.14 02:30:32.08 +57:11:25.7
136.07579 -3.13062 galactic Per Second-epoch detections are separated by 1.2" and 4.0 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 457986145332046080 | 02:30:32.15 +57:11:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.196+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:32.08 +57:11:25.7: 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 02:30:32.08 +57:11:25.7: 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 31.3529* 02 30 32.08 +57 11 25.7 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
Gaia DR3 457986145332046080,2461191.8529,8.14,0.05,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 457986145332046080 20260531.3529 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 31.3529 2461191.8529 8.16 02:26:13.32 +56:36:46.9
135.73860 -3.88347 galactic Per Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457622310064448128 | 02:26:13.35 +56:36:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.082+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:13.32 +56:36:46.9: 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 02:26:13.32 +56:36:46.9: 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 31.3529* 02 26 13.32 +56 36 46.9 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 457622310064448128,2461191.8529,8.16,0.05,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 457622310064448128 20260531.3529 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 31.3529 2461191.8529 8.15 02:30:33.06 +56:53:09.3
136.19181 -3.41229 galactic Per Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:30:33.06 +56:53:09.3: 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 02:30:33.06 +56:53:09.3: 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 31.3529* 02 30 33.06 +56 53 09.3 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
Gaia DR3 457978483110691456,2461191.8529,8.15,0.05,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
Gaia DR3 457978483110691456 20260531.3529 8.15CV 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 31.3529 2461191.8529 8.17 02:35:20.15 +57:29:29.6
136.56006 -2.60503 galactic Per Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8552+57.4916 | 02:35:20.17 +57:29:30.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.125+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:20.15 +57:29:29.6: 12.94 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:20.15 +57:29:29.6: 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 31.3529* 02 35 20.15 +57 29 29.6 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 J038.8552+57.4916,2461191.8529,8.17,0.05,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 J038.8552+57.4916 20260531.3529 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 31.3529 2461191.8529 8.16 02:26:07.39 +56:25:11.4
135.79524 -4.06872 galactic Per Second-epoch detections are separated by 1.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:26:07.39 +56:25:11.4: 11.87 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:07.39 +56:25:11.4: 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 31.3529* 02 26 07.39 +56 25 11.4 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 457610077996536576,2461191.8529,8.16,0.05,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 457610077996536576 20260531.3529 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 31.3529 2461191.8529 8.21 02:30:00.36 +57:28:19.5
135.90444 -2.89585 galactic Per Second-epoch detections are separated by 0.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458046721552378240 | 02:30:00.47 +57:28:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: em 1975AbaOB..47....3D [D75b] Em* 02-080 J-Ks=1.283+/-0.036 (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 02:30:00.36 +57:28:19.5: 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 02:30:00.36 +57:28:19.5: 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 31.3529* 02 30 00.36 +57 28 19.5 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 458046721552378240,2461191.8529,8.21,0.05,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 458046721552378240 20260531.3529 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 31.3529 2461191.8529 8.16 02:29:32.65 +55:57:16.0
136.40967 -4.32869 galactic Per Second-epoch detections are separated by 1.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:29:32.65 +55:57:16.0: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:32.65 +55:57:16.0: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.23 +/- 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 31.3529* 02 29 32.65 +55 57 16.0 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 457351177367649536,2461191.8529,8.16,0.05,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 457351177367649536 20260531.3529 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 31.3529 2461191.8529 8.20 02:31:05.86 +56:37:18.2
136.36059 -3.62917 galactic Per Second-epoch detections are separated by 1.3" and 4.0 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
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:05.86 +56:37:18.2: 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 02:31:05.86 +56:37:18.2: 10.91 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 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 31.3529* 02 31 05.86 +56 37 18.2 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 457585132825664640,2461191.8529,8.20,0.05,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 457585132825664640 20260531.3529 8.20CV 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 31.3529 2461191.8529 8.28 02:24:32.58 +57:00:45.4
135.38105 -3.59165 galactic Per Second-epoch detections are separated by 1.0" and 3.6 pix
The object was found in VSX 1" Barlad V48
Type:
# Max. Min./Amp. JD0 Period
10.990 V Y 0.280 TESS 2457271.73600 0.662760000000 B3e
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 02:24:32.58 +57:00:45.4: 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 02:24:32.58 +57:00:45.4: 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 31.3529* 02 24 32.58 +57 00 45.4 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
Barlad V48,2461191.8529,8.28,0.05,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
Barlad V48 20260531.3529 8.28CV 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 31.3529 2461191.8529 8.28 02:19:56.59 +56:13:25.6
135.05783 -4.55008 galactic Per Second-epoch detections are separated by 1.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458261469917614080 | 02:19:56.64 +56:13:24.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.056+/-0.041 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:56.59 +56:13:25.6: 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 02:19:56.59 +56:13:25.6: 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 31.3529* 02 19 56.59 +56 13 25.6 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 458261469917614080,2461191.8529,8.28,0.05,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
Gaia DR3 458261469917614080 20260531.3529 8.28CV 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 31.3529 2461191.8529 8.22 02:36:08.58 +57:39:34.6
136.59384 -2.40802 galactic Cas Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:36:08.58 +57:39:34.6: 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 02:36:08.58 +57:39:34.6: 10.91 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 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 31.3529* 02 36 08.58 +57 39 34.6 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
ATO J039.0481+57.6598,2461191.8529,8.22,0.05,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
ATO J039.0481+57.6598 20260531.3529 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 31.3529 2461191.8529 8.21 02:29:40.57 +56:18:39.2
136.29433 -3.99082 galactic Per Second-epoch detections are separated by 0.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457550601287980160 | 02:29:40.90 +56:18:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: em 1950ApJ...112...72M BD+55 633
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:40.57 +56:18:39.2: 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 02:29:40.57 +56:18:39.2: 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 31.3529* 02 29 40.57 +56 18 39.2 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 457550601287980160,2461191.8529,8.21,0.05,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 457550601287980160 20260531.3529 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 31.3529 2461191.8529 8.21 02:30:37.28 +56:22:56.7
136.38943 -3.87566 galactic Per Second-epoch detections are separated by 0.1" and 3.9 pix
The object was found in VSX19" 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 02:30:37.28 +56:22:56.7: 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 02:30:37.28 +56:22:56.7: 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 31.3529* 02 30 37.28 +56 22 56.7 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
Gaia DR3 457575031062827776,2461191.8529,8.21,0.05,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 457575031062827776 20260531.3529 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 31.3529 2461191.8529 8.27 02:31:20.20 +57:33:46.6
136.03633 -2.74479 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458067234316909312 | 02:31:20.25 +57:33:46.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.337+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:20.20 +57:33:46.6: 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 02:31:20.20 +57:33:46.6: 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 31.3529* 02 31 20.20 +57 33 46.6 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 458067234316909312,2461191.8529,8.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458067234316909312 20260531.3529 8.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.22 02:30:49.36 +56:11:02.6
136.48987 -4.04913 galactic Per Second-epoch detections are separated by 0.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457383716040658304 | 02:30:49.82 +56:11:02.2 (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 02:30:49.36 +56:11:02.6: 12.96 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:49.36 +56:11:02.6: 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 31.3529* 02 30 49.36 +56 11 02.6 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 457383716040658304,2461191.8529,8.22,0.05,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 457383716040658304 20260531.3529 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 31.3529 2461191.8529 8.25 02:34:28.42 +56:22:24.6
136.88699 -3.68081 galactic Per Second-epoch detections are separated by 0.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6214+56.3728 | 02:34:29.15 +56:22:22.4 (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 02:34:28.42 +56:22:24.6: 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 02:34:28.42 +56:22:24.6: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 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 31.3529* 02 34 28.42 +56 22 24.6 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 J038.6214+56.3728,2461191.8529,8.25,0.05,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
ATO J038.6214+56.3728 20260531.3529 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 31.3529 2461191.8529 8.31 02:24:18.90 +56:54:02.0
135.39142 -3.70747 galactic Per Second-epoch detections are separated by 0.2" and 3.7 pix
The object was found in VSX19" Gaia DR3 458386298846823680
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
17.620 G 17.700 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 02:24:18.90 +56:54:02.0: 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 02:24:18.90 +56:54:02.0: 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 31.3529* 02 24 18.90 +56 54 02.0 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
Gaia DR3 458386298846823680,2461191.8529,8.31,0.05,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
Gaia DR3 458386298846823680 20260531.3529 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 31.3529 2461191.8529 8.29 02:29:50.49 +56:19:09.0
136.31259 -3.97462 galactic Per Second-epoch detections are separated by 0.4" and 4.0 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
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:50.49 +56:19:09.0: 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 02:29:50.49 +56:19:09.0: 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 31.3529* 02 29 50.49 +56 19 09.0 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 J037.4614+56.3323,2461191.8529,8.29,0.05,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
ATO J037.4614+56.3323 20260531.3529 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 31.3529 2461191.8529 8.29 02:29:40.82 +56:20:03.6
136.28615 -3.96883 galactic Per Second-epoch detections are separated by 1.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:29:40.82 +56:20:03.6: 10.63 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:40.82 +56:20:03.6: 11.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 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 31.3529* 02 29 40.82 +56 20 03.6 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 457550704367181056,2461191.8529,8.29,0.05,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 457550704367181056 20260531.3529 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 31.3529 2461191.8529 8.33 02:25:00.79 +56:51:32.4
135.49554 -3.71270 galactic Per Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457640348919934336 | 02:25:00.75 +56:51:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.114+/-0.042 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:00.79 +56:51:32.4: 13.18 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:00.79 +56:51:32.4: 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 31.3529* 02 25 00.79 +56 51 32.4 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 457640348919934336,2461191.8529,8.33,0.05,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 457640348919934336 20260531.3529 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 31.3529 2461191.8529 8.31 02:32:13.87 +55:56:23.6
136.76478 -4.20104 galactic Per Second-epoch detections are separated by 1.0" and 4.0 pix
The object was found in VSX 6" V1071 Per
Type: EW
# Max. Min./Amp. JD0 Period
10.940 V 11.240 V 2457070.72700 0.359847600000
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 02:32:13.87 +55:56:23.6: 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 02:32:13.87 +55:56:23.6: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 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 31.3529* 02 32 13.87 +55 56 23.6 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
V1071 Per,2461191.8529,8.31,0.05,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
V1071 Per 20260531.3529 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 31.3529 2461191.8529 8.29 02:29:28.33 +56:33:05.7
136.17871 -3.77769 galactic Per Second-epoch detections are separated by 0.3" and 3.9 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 02:29:28.33 +56:33:05.7: 12.89 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:28.33 +56:33:05.7: 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 31.3529* 02 29 28.33 +56 33 05.7 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 457591145780012800,2461191.8529,8.29,0.05,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 457591145780012800 20260531.3529 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 31.3529 2461191.8529 8.31 02:28:09.55 +56:10:49.3
136.14608 -4.18976 galactic Per Second-epoch detections are separated by 1.2" and 4.0 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 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 02:28:09.55 +56:10:49.3: 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 02:28:09.55 +56:10:49.3: 10.98 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.98 +/- 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 31.3529* 02 28 09.55 +56 10 49.3 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 457545687845511808,2461191.8529,8.31,0.05,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
Gaia DR3 457545687845511808 20260531.3529 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 31.3529 2461191.8529 8.32 02:33:09.16 +57:00:38.4
136.47348 -3.16265 galactic Per Second-epoch detections are separated by 1.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:33:09.16 +57:00:38.4: 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 02:33:09.16 +57:00:38.4: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.96 +/- 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 31.3529* 02 33 09.16 +57 00 38.4 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 J038.2979+57.0026,2461191.8529,8.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260531.3529 8.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.34 02:21:04.80 +56:15:33.0
135.19490 -4.46335 galactic Per Second-epoch detections are separated by 0.9" and 3.7 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 02:21:04.80 +56:15:33.0: 12.42 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:04.80 +56:15:33.0: 11.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.07 +/- 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 31.3529* 02 21 04.80 +56 15 33.0 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
Gaia DR3 458255319524584576,2461191.8529,8.34,0.05,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
Gaia DR3 458255319524584576 20260531.3529 8.34CV 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 31.3529 2461191.8529 8.32 02:37:41.06 +57:33:22.4
136.82453 -2.42130 galactic Cas Second-epoch detections are separated by 2.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:37:41.06 +57:33:22.4: 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 02:37:41.06 +57:33:22.4: 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 31.3529* 02 37 41.06 +57 33 22.4 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
ATO J039.4083+57.5560,2461191.8529,8.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260531.3529 8.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.39 02:28:48.94 +56:07:35.3
136.25117 -4.20637 galactic Per Second-epoch detections are separated by 3.3" and 3.7 pix
The object was found in VSX 5" 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 02:28:48.94 +56:07:35.3: 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 02:28:48.94 +56:07:35.3: 11.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.21 +/- 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 31.3529* 02 28 48.94 +56 07 35.3 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 457541805195095296,2461191.8529,8.39,0.05,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 457541805195095296 20260531.3529 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 31.3529 2461191.8529 8.38 02:21:59.12 +56:30:01.8
135.23025 -4.19371 galactic Per Second-epoch detections are separated by 0.9" and 3.7 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 02:21:59.12 +56:30:01.8: 11.32 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:59.12 +56:30:01.8: 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 31.3529* 02 21 59.12 +56 30 01.8 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
TYC 3694-1258-1,2461191.8529,8.38,0.05,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
TYC 3694-1258-1 20260531.3529 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 31.3529 2461191.8529 8.40 02:30:30.77 +57:30:27.1
135.95450 -2.83760 galactic Per Second-epoch detections are separated by 0.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458046515393935744 | 02:30:30.94 +57:30:26.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.350+/-0.035 (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 02:30:30.77 +57:30:27.1: 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 02:30:30.77 +57:30:27.1: 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 31.3529* 02 30 30.77 +57 30 27.1 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 458046515393935744,2461191.8529,8.40,0.05,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 458046515393935744 20260531.3529 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 31.3529 2461191.8529 8.30 02:22:31.56 +56:14:11.4
135.39193 -4.41576 galactic Per Second-epoch detections are separated by 0.6" and 3.8 pix
The object was found in VSX16" 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 02:22:31.56 +56:14:11.4: 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 02:22:31.56 +56:14:11.4: 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 31.3529* 02 22 31.56 +56 14 11.4 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 457502291496530304,2461191.8529,8.30,0.05,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
Gaia DR3 457502291496530304 20260531.3529 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 31.3529 2461191.8529 8.34 02:34:25.96 +56:29:13.8
136.83762 -3.57822 galactic Per Second-epoch detections are separated by 0.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:34:25.96 +56:29:13.8: 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 02:34:25.96 +56:29:13.8: 11.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 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 31.3529* 02 34 25.96 +56 29 13.8 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 457752877067783040,2461191.8529,8.34,0.05,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
Gaia DR3 457752877067783040 20260531.3529 8.34CV 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 31.3529 2461191.8529 8.30 02:33:33.86 +56:11:46.9
136.83886 -3.89293 galactic Per Second-epoch detections are separated by 1.6" and 3.7 pix
The object was found in VSX10" Gaia DR3 457371518333663744
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.980 G 11.010 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 02:33:33.86 +56:11:46.9: 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 02:33:33.86 +56:11:46.9: 11.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.18 +/- 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 31.3529* 02 33 33.86 +56 11 46.9 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
Gaia DR3 457371518333663744,2461191.8529,8.30,0.05,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
Gaia DR3 457371518333663744 20260531.3529 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 31.3529 2461191.8529 8.34 02:35:42.45 +56:44:19.0
136.90131 -3.27832 galactic Per Second-epoch detections are separated by 1.2" and 3.8 pix
The object was found in VSX 4" 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 02:35:42.45 +56:44:19.0: 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 02:35:42.45 +56:44:19.0: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 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 31.3529* 02 35 42.45 +56 44 19.0 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
Gaia DR3 457785175221622144,2461191.8529,8.34,0.05,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
Gaia DR3 457785175221622144 20260531.3529 8.34CV 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 31.3529 2461191.8529 8.45 02:16:48.70 +56:16:11.9
134.63067 -4.65030 galactic Per Second-epoch detections are separated by 3.5" and 3.4 pix
The object was found in VSX23" ZTF J021647.41+561551.1
Type: RS
# Max. Min./Amp. JD0 Period
17.561 r Y 0.116 r 2458434.71030 4.236074900000
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 02:16:48.70 +56:16:11.9: 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 02:16:48.70 +56:16:11.9: 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 31.3529* 02 16 48.70 +56 16 11.9 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
ZTF J021647.41+561551.1,2461191.8529,8.45,0.05,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
ZTF J021647.41+561551.1 20260531.3529 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 31.3529 2461191.8529 8.41 02:36:22.60 +57:40:05.9
136.61917 -2.38774 galactic Cas Second-epoch detections are separated by 1.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458109771665185536 | 02:36:22.54 +57:40:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.267+/-0.047 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:22.60 +57:40:05.9: 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 02:36:22.60 +57:40:05.9: 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 31.3529* 02 36 22.60 +57 40 05.9 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
Gaia DR3 458109771665185536,2461191.8529,8.41,0.05,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
Gaia DR3 458109771665185536 20260531.3529 8.41CV 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 31.3529 2461191.8529 8.43 02:23:48.04 +56:47:01.7
135.36646 -3.84147 galactic Per Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458383962384697856 | 02:23:48.06 +56:47:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.091+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:48.04 +56:47:01.7: 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 02:23:48.04 +56:47:01.7: 11.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.07 +/- 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 31.3529* 02 23 48.04 +56 47 01.7 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 458383962384697856,2461191.8529,8.43,0.05,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
Gaia DR3 458383962384697856 20260531.3529 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 31.3529 2461191.8529 8.40 02:26:10.78 +56:48:29.0
135.66311 -3.70348 galactic Per Second-epoch detections are separated by 0.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:26:10.78 +56:48:29.0: 10.58 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:10.78 +56:48:29.0: 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 31.3529* 02 26 10.78 +56 48 29.0 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
ATO J036.5437+56.8208,2461191.8529,8.40,0.05,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
ATO J036.5437+56.8208 20260531.3529 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 31.3529 2461191.8529 8.40 02:35:30.16 +57:03:30.3
136.75020 -2.99496 galactic Per Second-epoch detections are separated by 0.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8893+57.0658 | 02:35:30.27 +57:03:32.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.419+/-0.068 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:30.16 +57:03:30.3: 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 02:35:30.16 +57:03:30.3: 11.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.07 +/- 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 31.3529* 02 35 30.16 +57 03 30.3 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 J038.8893+57.0658,2461191.8529,8.40,0.05,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
ATO J038.8893+57.0658 20260531.3529 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 31.3529 2461191.8529 8.42 02:18:23.94 +56:23:20.9
134.79999 -4.46560 galactic Per Second-epoch detections are separated by 1.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458313421843558528 | 02:18:24.08 +56:23:24.9 (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 02:18:23.94 +56:23:20.9: 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 02:18:23.94 +56:23:20.9: 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 31.3529* 02 18 23.94 +56 23 20.9 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 458313421843558528,2461191.8529,8.42,0.05,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 458313421843558528 20260531.3529 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 31.3529 2461191.8529 8.38 02:26:55.66 +56:30:19.4
135.86833 -3.94892 galactic Per Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:26:55.66 +56:30:19.4: 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 02:26:55.66 +56:30:19.4: 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 31.3529* 02 26 55.66 +56 30 19.4 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
Gaia DR3 457617843297470592,2461191.8529,8.38,0.05,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
Gaia DR3 457617843297470592 20260531.3529 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 31.3529 2461191.8529 8.36 02:25:03.10 +56:56:58.5
135.46832 -3.62613 galactic Per Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458393273873643392 | 02:25:03.15 +56:56:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.947+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:03.10 +56:56:58.5: 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 02:25:03.10 +56:56:58.5: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.13 +/- 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 31.3529* 02 25 03.10 +56 56 58.5 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 458393273873643392,2461191.8529,8.36,0.05,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
Gaia DR3 458393273873643392 20260531.3529 8.36CV 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 31.3529 2461191.8529 8.45 02:23:02.10 +56:30:28.6
135.36395 -4.13671 galactic Per Second-epoch detections are separated by 1.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458285624814498048 | 02:23:02.07 +56:30:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965LS....C05....0H LS V +56 40 J-Ks=-0.038+/-0.034 (B)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:02.10 +56:30:28.6: 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 02:23:02.10 +56:30:28.6: 11.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 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 31.3529* 02 23 02.10 +56 30 28.6 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 458285624814498048,2461191.8529,8.45,0.05,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 458285624814498048 20260531.3529 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 31.3529 2461191.8529 8.33 02:33:05.09 +56:13:01.1
136.76922 -3.89948 galactic Per Second-epoch detections are separated by 0.6" and 4.0 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 457372446046599424 | 02:33:05.74 +56:12:59.5 (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 02:33:05.09 +56:13:01.1: 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 02:33:05.09 +56:13:01.1: 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 31.3529* 02 33 05.09 +56 13 01.1 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 457372446046599424,2461191.8529,8.33,0.05,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 457372446046599424 20260531.3529 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 31.3529 2461191.8529 8.40 02:37:50.53 +57:45:50.6
136.76101 -2.22228 galactic Cas Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:37:50.53 +57:45:50.6: 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 02:37:50.53 +57:45:50.6: 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 31.3529* 02 37 50.53 +57 45 50.6 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
ATO J039.4571+57.7717,2461191.8529,8.40,0.05,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
ATO J039.4571+57.7717 20260531.3529 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 31.3529 2461191.8529 8.42 02:35:28.70 +56:28:21.1
136.97656 -3.53552 galactic Per Second-epoch detections are separated by 1.5" and 3.7 pix
The object was found in VSX 5" Gaia DR3 457711026906434048
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.890 G 10.920 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 02:35:28.70 +56:28:21.1: 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 02:35:28.70 +56:28:21.1: 11.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 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 31.3529* 02 35 28.70 +56 28 21.1 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 457711026906434048,2461191.8529,8.42,0.05,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 457711026906434048 20260531.3529 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 31.3529 2461191.8529 8.42 02:32:25.76 +56:47:11.8
136.46766 -3.40744 galactic Per Second-epoch detections are separated by 0.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1078+56.7931 | 02:32:26.17 +56:47:10.5 (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 02:32:25.76 +56:47:11.8: 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 02:32:25.76 +56:47:11.8: 11.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 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 31.3529* 02 32 25.76 +56 47 11.8 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
ATO J038.1078+56.7931,2461191.8529,8.42,0.05,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 J038.1078+56.7931 20260531.3529 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 31.3529 2461191.8529 8.47 02:31:09.67 +57:16:15.4
136.12432 -3.02425 galactic Per Second-epoch detections are separated by 1.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:31:09.67 +57:16:15.4: 12.64 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:09.67 +57:16:15.4: 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 31.3529* 02 31 09.67 +57 16 15.4 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 457993944995787520,2461191.8529,8.47,0.05,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
Gaia DR3 457993944995787520 20260531.3529 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 31.3529 2461191.8529 8.43 02:34:12.78 +56:12:36.7
136.91693 -3.84538 galactic Per Second-epoch detections are separated by 1.9" and 4.2 pix
The object was found in VSX 5" Gaia DR3 457326232196815232
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.910 G 10.930 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 02:34:12.78 +56:12:36.7: 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 02:34:12.78 +56:12:36.7: 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 31.3529* 02 34 12.78 +56 12 36.7 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 457326232196815232,2461191.8529,8.43,0.05,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
Gaia DR3 457326232196815232 20260531.3529 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 31.3529 2461191.8529 8.45 02:26:43.12 +56:24:13.3
135.87811 -4.05419 galactic Per Second-epoch detections are separated by 1.2" and 4.0 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 J036.6811+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 02:26:43.12 +56:24:13.3: 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 02:26:43.12 +56:24:13.3: 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 31.3529* 02 26 43.12 +56 24 13.3 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 J036.6811+56.4136,2461191.8529,8.45,0.05,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
ATO J036.6811+56.4136 20260531.3529 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 31.3529 2461191.8529 8.39 02:34:04.55 +56:42:30.3
136.70653 -3.39318 galactic Per Second-epoch detections are separated by 0.9" and 3.8 pix
The object was found in VSX21" 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 02:34:04.55 +56:42:30.3: 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 02:34:04.55 +56:42:30.3: 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 31.3529* 02 34 04.55 +56 42 30.3 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 457775687633336704,2461191.8529,8.39,0.05,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 457775687633336704 20260531.3529 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 31.3529 2461191.8529 8.55 02:23:17.87 +56:42:24.1
135.32868 -3.93779 galactic Per Second-epoch detections are separated by 0.7" and 3.9 pix
The object was found in VSX 0" Gaia DR3 458289473105316864
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.020 G 11.050 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 02:23:17.87 +56:42:24.1: 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 02:23:17.87 +56:42:24.1: 11.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 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 31.3529* 02 23 17.87 +56 42 24.1 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 458289473105316864,2461191.8529,8.55,0.05,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 458289473105316864 20260531.3529 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 31.3529 2461191.8529 8.55 02:25:55.90 +56:58:59.9
135.56860 -3.55194 galactic Per Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.4932+56.9802 | 02:25:55.90 +56:58:58.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.464+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:55.90 +56:58:59.9: 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 02:25:55.90 +56:58:59.9: 11.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.25 +/- 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 31.3529* 02 25 55.90 +56 58 59.9 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 J036.4932+56.9802,2461191.8529,8.55,0.05,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
ATO J036.4932+56.9802 20260531.3529 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 31.3529 2461191.8529 8.48 02:27:59.47 +56:29:43.8
136.00899 -3.90488 galactic Per Second-epoch detections are separated by 0.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457570907893144576 | 02:27:59.65 +56:29:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.153+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:59.47 +56:29:43.8: 13.02 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:59.47 +56:29:43.8: 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 31.3529* 02 27 59.47 +56 29 43.8 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 457570907893144576,2461191.8529,8.48,0.05,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 457570907893144576 20260531.3529 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 31.3529 2461191.8529 8.52 02:25:48.33 +56:55:12.6
135.57509 -3.61706 galactic Per Second-epoch detections are separated by 1.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457641826394416640 | 02:25:48.39 +56:55:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.079+/-0.029 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:48.33 +56:55:12.6: 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 02:25:48.33 +56:55:12.6: 11.16 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.16 +/- 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 31.3529* 02 25 48.33 +56 55 12.6 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 457641826394416640,2461191.8529,8.52,0.05,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 457641826394416640 20260531.3529 8.52CV 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 31.3529 2461191.8529 8.49 02:29:58.05 +56:08:50.3
136.39291 -4.12767 galactic Per Second-epoch detections are separated by 1.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:29:58.05 +56:08:50.3: 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 02:29:58.05 +56:08:50.3: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 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 31.3529* 02 29 58.05 +56 08 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 457359423705242368,2461191.8529,8.49,0.05,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 457359423705242368 20260531.3529 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 31.3529 2461191.8529 8.51 02:33:40.64 +57:26:09.7
136.37577 -2.74259 galactic Per Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458009784832780544 | 02:33:40.74 +57:26:10.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965LS....C05....0H LS V +57 51 J-Ks=0.185+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:40.64 +57:26:09.7: 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 02:33:40.64 +57:26:09.7: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.13 +/- 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 31.3529* 02 33 40.64 +57 26 09.7 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 458009784832780544,2461191.8529,8.51,0.05,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 458009784832780544 20260531.3529 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 31.3529 2461191.8529 8.59 02:35:08.68 +57:36:15.0
136.49247 -2.51132 galactic Cas Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:35:08.68 +57:36:15.0: 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 02:35:08.68 +57:36:15.0: 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 31.3529* 02 35 08.68 +57 36 15.0 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 458105717221633536,2461191.8529,8.59,0.05,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 458105717221633536 20260531.3529 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 31.3529 2461191.8529 8.64 02:34:48.58 +57:38:04.9
136.43923 -2.50064 galactic Per Second-epoch detections are separated by 0.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.7029+57.6276 | 02:34:48.60 +57:38:04.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 70 J-Ks=0.170+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:48.58 +57:38:04.9: 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 02:34:48.58 +57:38:04.9: 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 31.3529* 02 34 48.58 +57 38 04.9 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 J038.7029+57.6276,2461191.8529,8.64,0.05,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 J038.7029+57.6276 20260531.3529 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 31.3529 2461191.8529 8.49 02:30:03.56 +56:22:32.1
136.31965 -3.91103 galactic Per Second-epoch detections are separated by 2.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457574309510238464 | 02:30:04.15 +56:22:32.2 (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 02:30:03.56 +56:22:32.1: 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 02:30:03.56 +56:22:32.1: 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 31.3529* 02 30 03.56 +56 22 32.1 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 457574309510238464,2461191.8529,8.49,0.05,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 457574309510238464 20260531.3529 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 31.3529 2461191.8529 8.58 02:32:59.21 +57:28:34.1
136.27451 -2.74113 galactic Per Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:32:59.21 +57:28:34.1: 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 02:32:59.21 +57:28:34.1: 11.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 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 31.3529* 02 32 59.21 +57 28 34.1 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 458022738454361216,2461191.8529,8.58,0.05,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
Gaia DR3 458022738454361216 20260531.3529 8.58CV 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 31.3529 2461191.8529 8.54 02:28:57.12 +57:06:16.3
135.90804 -3.29001 galactic Per Second-epoch detections are separated by 1.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457659212422846976 | 02:28:57.82 +57:06:20.5 (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 02:28:57.12 +57:06:16.3: 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 02:28:57.12 +57:06:16.3: 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 31.3529* 02 28 57.12 +57 06 16.3 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 457659212422846976,2461191.8529,8.54,0.05,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 457659212422846976 20260531.3529 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 31.3529 2461191.8529 8.57 02:30:18.83 +55:54:55.5
136.52456 -4.32484 galactic Per Second-epoch detections are separated by 0.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457348084991505152 | 02:30:19.49 +55:54:55.1 (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 02:30:18.83 +55:54:55.5: 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 02:30:18.83 +55:54:55.5: 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 31.3529* 02 30 18.83 +55 54 55.5 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 457348084991505152,2461191.8529,8.57,0.05,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
Gaia DR3 457348084991505152 20260531.3529 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 31.3529 2461191.8529 8.59 02:19:36.34 +56:23:22.7
134.95776 -4.40955 galactic Per Second-epoch detections are separated by 1.3" and 4.1 pix
The object was found in VSX 5" 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 02:19:36.34 +56:23:22.7: 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 02:19:36.34 +56:23:22.7: 11.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.28 +/- 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 31.3529* 02 19 36.34 +56 23 22.7 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 458272396314337536,2461191.8529,8.59,0.05,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 458272396314337536 20260531.3529 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 31.3529 2461191.8529 8.55 02:31:29.13 +57:11:55.8
136.19220 -3.07455 galactic Per Second-epoch detections are separated by 1.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457988344355269888 | 02:31:29.21 +57:11:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:29.13 +57:11:55.8: 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 02:31:29.13 +57:11:55.8: 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 31.3529* 02 31 29.13 +57 11 55.8 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 457988344355269888,2461191.8529,8.55,0.05,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 457988344355269888 20260531.3529 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 31.3529 2461191.8529 8.53 02:30:59.05 +56:08:44.3
136.52521 -4.07630 galactic Per Second-epoch detections are separated by 1.1" and 4.0 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 457380619359718400 | 02:30:59.49 +56:08:45.2 (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 02:30:59.05 +56:08:44.3: 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 02:30:59.05 +56:08:44.3: 11.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 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 31.3529* 02 30 59.05 +56 08 44.3 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 457380619359718400,2461191.8529,8.53,0.05,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 457380619359718400 20260531.3529 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 31.3529 2461191.8529 8.61 02:16:52.45 +56:18:44.9
134.62503 -4.60729 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.2189+56.3127 | 02:16:52.55 +56:18:45.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.251+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:52.45 +56:18:44.9: 11.79 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:52.45 +56:18:44.9: 11.45 +/- 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 31.3529* 02 16 52.45 +56 18 44.9 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 J034.2189+56.3127,2461191.8529,8.61,0.05,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
ATO J034.2189+56.3127 20260531.3529 8.61CV 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 31.3529 2461191.8529 8.63 02:31:00.03 +56:00:28.9
136.57914 -4.20298 galactic Per Second-epoch detections are separated by 0.8" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457355163097206784 | 02:31:00.46 +56:00:31.5 (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 02:31:00.03 +56:00:28.9: 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 02:31:00.03 +56:00:28.9: 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 31.3529* 02 31 00.03 +56 00 28.9 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 457355163097206784,2461191.8529,8.63,0.05,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 457355163097206784 20260531.3529 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 31.3529 2461191.8529 8.60 02:32:17.76 +57:17:09.4
136.26084 -2.95244 galactic Per Second-epoch detections are separated by 1.1" and 3.6 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 02:32:17.76 +57:17:09.4: 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 02:32:17.76 +57:17:09.4: 11.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.25 +/- 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 31.3529* 02 32 17.76 +57 17 09.4 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 458013701843090176,2461191.8529,8.60,0.05,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
Gaia DR3 458013701843090176 20260531.3529 8.60CV 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 31.3529 2461191.8529 8.64 02:26:11.61 +56:56:03.9
135.61952 -3.58483 galactic Per Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457665122298061184 | 02:26:11.60 +56:56:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.042+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:11.61 +56:56:03.9: 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 02:26:11.61 +56:56:03.9: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.24 +/- 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 31.3529* 02 26 11.61 +56 56 03.9 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 457665122298061184,2461191.8529,8.64,0.05,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 457665122298061184 20260531.3529 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 31.3529 2461191.8529 8.54 02:34:43.40 +56:34:06.2
136.84307 -3.48781 galactic Per Second-epoch detections are separated by 1.7" and 4.0 pix
The object was found in VSX 3" Gaia DR3 457759061822261632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.990 G 11.080 G 0.079441300000 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 02:34:43.40 +56:34:06.2: 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 02:34:43.40 +56:34:06.2: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.23 +/- 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 31.3529* 02 34 43.40 +56 34 06.2 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 457759061822261632,2461191.8529,8.54,0.05,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 457759061822261632 20260531.3529 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 31.3529 2461191.8529 8.64 02:21:34.57 +56:26:43.6
135.19595 -4.26480 galactic Per Second-epoch detections are separated by 1.3" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.4115+56.4466 | 02:21:34.45 +56:26:43.9 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.038+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:34.57 +56:26:43.6: 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 02:21:34.57 +56:26:43.6: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.24 +/- 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 31.3529* 02 21 34.57 +56 26 43.6 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
ATO J035.4115+56.4466,2461191.8529,8.64,0.05,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 J035.4115+56.4466 20260531.3529 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 31.3529 2461191.8529 8.65 02:36:59.39 +57:56:28.2
136.58646 -2.10480 galactic Cas Second-epoch detections are separated by 1.3" and 3.6 pix
The object was found in VSX21" 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 02:36:59.39 +57:56:28.2: 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 02:36:59.39 +57:56:28.2: 11.45 +/- 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 31.3529* 02 36 59.39 +57 56 28.2 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
Gaia DR3 458140695435098880,2461191.8529,8.65,0.05,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 458140695435098880 20260531.3529 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 31.3529 2461191.8529 8.64 02:35:04.69 +57:26:54.1
136.54498 -2.65830 galactic Per Second-epoch detections are separated by 1.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:35:04.69 +57:26:54.1: 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 02:35:04.69 +57:26:54.1: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 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 31.3529* 02 35 04.69 +57 26 54.1 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 458007791968161280,2461191.8529,8.64,0.05,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 458007791968161280 20260531.3529 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 31.3529 2461191.8529 8.74 02:37:50.74 +57:57:57.3
136.68088 -2.03698 galactic Cas Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458138766987060992 | 02:37:50.73 +57:57:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.147+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.74 +57:57:57.3: 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 02:37:50.74 +57:57:57.3: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 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 31.3529* 02 37 50.74 +57 57 57.3 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 458138766987060992,2461191.8529,8.74,0.05,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 458138766987060992 20260531.3529 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 31.3529 2461191.8529 8.65 02:33:03.17 +57:03:28.2
136.44284 -3.12427 galactic Per Second-epoch detections are separated by 1.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:33:03.17 +57:03:28.2: 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 02:33:03.17 +57:03:28.2: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 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 31.3529* 02 33 03.17 +57 03 28.2 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 J038.2584+57.0472,2461191.8529,8.65,0.05,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 J038.2584+57.0472 20260531.3529 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 31.3529 2461191.8529 8.70 02:38:18.06 +57:37:36.9
136.87209 -2.32349 galactic Cas Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457942474103581568 | 02:38:18.15 +57:37:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.117+/-0.027 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:18.06 +57:37:36.9: 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 02:38:18.06 +57:37:36.9: 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 31.3529* 02 38 18.06 +57 37 36.9 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 457942474103581568,2461191.8529,8.70,0.05,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 457942474103581568 20260531.3529 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 31.3529 2461191.8529 8.59 02:36:07.69 +57:21:39.9
136.70944 -2.68332 galactic Per Second-epoch detections are separated by 2.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:36:07.69 +57:21:39.9: 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 02:36:07.69 +57:21:39.9: 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 31.3529* 02 36 07.69 +57 21 39.9 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 457911653417858560,2461191.8529,8.59,0.05,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 457911653417858560 20260531.3529 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 31.3529 2461191.8529 8.64 02:20:18.71 +56:31:49.9
135.00238 -4.24407 galactic Per Second-epoch detections are separated by 2.6" and 3.5 pix
The object was found in VSX17" ZTF J022018.55+563206.7
Type: SR
# Max. Min./Amp. JD0 Period
14.253 r Y 0.230 r 2458375.81050 70.681770000000
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 02:20:18.71 +56:31:49.9: 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 02:20:18.71 +56:31:49.9: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 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 31.3529* 02 20 18.71 +56 31 49.9 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
ZTF J022018.55+563206.7,2461191.8529,8.64,0.05,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
ZTF J022018.55+563206.7 20260531.3529 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 31.3529 2461191.8529 8.73 02:37:26.82 +58:01:13.3
136.61070 -2.00806 galactic Cas Second-epoch detections are separated by 2.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.3716+58.0183 | 02:37:26.68 +58:01:14.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.083+/-0.026 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:26.82 +58:01:13.3: 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 02:37:26.82 +58:01:13.3: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 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 31.3529* 02 37 26.82 +58 01 13.3 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
ATO J039.3716+58.0183,2461191.8529,8.73,0.05,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 J039.3716+58.0183 20260531.3529 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 31.3529 2461191.8529 8.67 02:34:24.38 +57:28:25.9
136.45172 -2.66987 galactic Per Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:34:24.38 +57:28:25.9: 10.07 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:24.38 +57:28:25.9: 11.33 +/- 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 31.3529* 02 34 24.38 +57 28 25.9 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
ATO J038.5831+57.4740,2461191.8529,8.67,0.05,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
ATO J038.5831+57.4740 20260531.3529 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 31.3529 2461191.8529 8.63 02:28:34.73 +56:13:02.0
136.18700 -4.13408 galactic Per Second-epoch detections are separated by 1.8" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457551872598387456 | 02:28:35.19 +56:13:03.3 (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 02:28:34.73 +56:13:02.0: 12.88 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:34.73 +56:13:02.0: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 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 31.3529* 02 28 34.73 +56 13 02.0 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 457551872598387456,2461191.8529,8.63,0.05,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 457551872598387456 20260531.3529 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 31.3529 2461191.8529 8.70 02:38:13.41 +57:50:16.7
136.77806 -2.13422 galactic Cas Second-epoch detections are separated by 0.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.5732+57.8385 | 02:38:13.32 +57:50:17.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.231+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:13.41 +57:50:16.7: 13.13 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:13.41 +57:50:16.7: 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 31.3529* 02 38 13.41 +57 50 16.7 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
ATO J039.5732+57.8385,2461191.8529,8.70,0.05,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
ATO J039.5732+57.8385 20260531.3529 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 31.3529 2461191.8529 8.69 02:24:01.97 +56:49:23.4
135.38247 -3.79347 galactic Per Second-epoch detections are separated by 0.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458385405493688832 | 02:24:01.94 +56:49:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965LS....C05....0H LS V +56 41 J-Ks=0.057+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:01.97 +56:49:23.4: 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 02:24:01.97 +56:49:23.4: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 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 31.3529* 02 24 01.97 +56 49 23.4 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 458385405493688832,2461191.8529,8.69,0.05,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 458385405493688832 20260531.3529 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 31.3529 2461191.8529 8.76 02:33:33.49 +55:49:25.7
136.98169 -4.23717 galactic Per Second-epoch detections are separated by 1.3" and 4.0 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 J038.3792+55.8236 | 02:33:34.38 +55:49:28.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.609+/-0.144 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:33.49 +55:49:25.7: 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 02:33:33.49 +55:49:25.7: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 31.3529* 02 33 33.49 +55 49 25.7 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
ATO J038.3792+55.8236,2461191.8529,8.76,0.05,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 J038.3792+55.8236 20260531.3529 8.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.76 02:27:23.30 +55:57:43.1
136.12539 -4.43232 galactic Per Second-epoch detections are separated by 0.4" and 3.9 pix
The object was found in VSX 6" NSVS J0227240+555737
Type: SR
# Max. Min./Amp. JD0 Period
14.275 g Y 1.459 g 2458459.81350 290.578666400000
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 02:27:23.30 +55:57:43.1: 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 02:27:23.30 +55:57:43.1: 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 31.3529* 02 27 23.30 +55 57 43.1 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
NSVS J0227240+555737,2461191.8529,8.76,0.05,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
NSVS J0227240+555737 20260531.3529 8.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.73 02:33:10.54 +57:32:53.9
136.27034 -2.66475 galactic Per Second-epoch detections are separated by 0.7" and 3.8 pix
The object was found in ASASSN-V 0" ASASSN-V J023310.55+573254.1
Type: VAR
MeanMag 11.23 m Amp. 1.35 m Period 514.391279 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 02:33:10.54 +57:32:53.9: 12.73 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:10.54 +57:32:53.9: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 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 31.3529* 02 33 10.54 +57 32 53.9 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
VARIABLE_NAME,2461191.8529,8.73,0.05,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
VARIABLE_NAME 20260531.3529 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 31.3529 2461191.8529 8.72 02:37:30.47 +57:39:32.1
136.76192 -2.33650 galactic Cas Second-epoch detections are separated by 1.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457923026491093376 | 02:37:30.47 +57:39:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.186+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:30.47 +57:39:32.1: 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 02:37:30.47 +57:39:32.1: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 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 31.3529* 02 37 30.47 +57 39 32.1 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 457923026491093376,2461191.8529,8.72,0.05,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 457923026491093376 20260531.3529 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 31.3529 2461191.8529 8.76 02:28:31.63 +56:00:35.4
136.25659 -4.32965 galactic Per Second-epoch detections are separated by 0.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457539537452434560 | 02:28:32.37 +56:00:37.4 (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 02:28:31.63 +56:00:35.4: 12.52 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:31.63 +56:00:35.4: 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 31.3529* 02 28 31.63 +56 00 35.4 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 457539537452434560,2461191.8529,8.76,0.05,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
Gaia DR3 457539537452434560 20260531.3529 8.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.73 02:24:33.99 +56:52:59.9
135.42972 -3.71152 galactic Per Second-epoch detections are separated by 1.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458391177929671040 | 02:24:34.08 +56:53:01.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.213+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:33.99 +56:52:59.9: 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 02:24:33.99 +56:52:59.9: 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 31.3529* 02 24 33.99 +56 52 59.9 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 458391177929671040,2461191.8529,8.73,0.05,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 458391177929671040 20260531.3529 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 31.3529 2461191.8529 8.77 02:25:56.77 +56:07:50.4
135.87603 -4.34751 galactic Per Second-epoch detections are separated by 1.8" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457464942460413568 | 02:25:56.69 +56:07:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:56.77 +56:07:50.4: 13.14 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:56.77 +56:07:50.4: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 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 31.3529* 02 25 56.77 +56 07 50.4 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 457464942460413568,2461191.8529,8.77,0.05,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
Gaia DR3 457464942460413568 20260531.3529 8.77CV 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 31.3529 2461191.8529 8.69 02:18:05.16 +56:15:08.3
134.80421 -4.60908 galactic Per Second-epoch detections are separated by 0.7" and 4.0 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 456810595604427392 | 02:18:01.38 +56:15:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 2013AJ....145..102L PM J02180+5616
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:05.16 +56:15:08.3: 11.86 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:05.16 +56:15:08.3: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 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 31.3529* 02 18 05.16 +56 15 08.3 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
Gaia DR3 456810595604427392,2461191.8529,8.69,0.05,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 456810595604427392 20260531.3529 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 31.3529 2461191.8529 8.86 02:29:57.46 +56:36:50.9
136.21768 -3.69480 galactic Per Second-epoch detections are separated by 0.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:29:57.46 +56:36:50.9: 10.25 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:57.46 +56:36:50.9: 11.66 +/- 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 31.3529* 02 29 57.46 +56 36 50.9 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 457581490693447040,2461191.8529,8.86,0.05,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 457581490693447040 20260531.3529 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 31.3529 2461191.8529 8.84 02:35:47.68 +57:10:24.3
136.74165 -2.87362 galactic Per Second-epoch detections are separated by 1.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.9488+57.1647 | 02:35:47.91 +57:10:23.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.759+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:47.68 +57:10:24.3: 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 02:35:47.68 +57:10:24.3: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 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 31.3529* 02 35 47.68 +57 10 24.3 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 J038.9488+57.1647,2461191.8529,8.84,0.05,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 J038.9488+57.1647 20260531.3529 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 31.3529 2461191.8529 8.79 02:28:48.14 +56:30:08.1
136.11091 -3.85761 galactic Per Second-epoch detections are separated by 1.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457567987315527296 | 02:28:48.02 +56:30:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.190+/-0.040 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:48.14 +56:30:08.1: 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 02:28:48.14 +56:30:08.1: 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 31.3529* 02 28 48.14 +56 30 08.1 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 457567987315527296,2461191.8529,8.79,0.05,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 457567987315527296 20260531.3529 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 31.3529 2461191.8529 8.77 02:20:07.37 +56:27:51.6
135.00014 -4.31518 galactic Per Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:20:07.37 +56:27:51.6: 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 02:20:07.37 +56:27:51.6: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 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 31.3529* 02 20 07.37 +56 27 51.6 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
Gaia DR3 458274320459648000,2461191.8529,8.77,0.05,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
Gaia DR3 458274320459648000 20260531.3529 8.77CV 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 31.3529 2461191.8529 8.76 02:25:04.18 +56:13:07.6
135.73025 -4.30862 galactic Per Second-epoch detections are separated by 4.1" and 4.4 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 457515824930594816 | 02:25:04.36 +56:13:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.337+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:04.18 +56:13:07.6: 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 02:25:04.18 +56:13:07.6: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 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 31.3529* 02 25 04.18 +56 13 07.6 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
Gaia DR3 457515824930594816,2461191.8529,8.76,0.05,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
Gaia DR3 457515824930594816 20260531.3529 8.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.86 02:31:11.42 +56:38:16.1
136.36636 -3.60948 galactic Per Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457585167185382272 | 02:31:11.79 +56:38:14.9 (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 02:31:11.42 +56:38:16.1: 11.52 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:11.42 +56:38:16.1: 11.75 +/- 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 31.3529* 02 31 11.42 +56 38 16.1 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 457585167185382272,2461191.8529,8.86,0.05,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 457585167185382272 20260531.3529 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 31.3529 2461191.8529 8.79 02:34:12.55 +56:11:53.5
136.92109 -3.85666 galactic Per Second-epoch detections are separated by 2.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457326232196815232 | 02:34:13.32 +56:12:39.2 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:12.55 +56:11:53.5: 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 02:34:12.55 +56:11:53.5: 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 31.3529* 02 34 12.55 +56 11 53.5 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
Gaia DR3 457326232196815232,2461191.8529,8.79,0.05,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 457326232196815232 20260531.3529 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 31.3529 2461191.8529 8.82 02:25:45.47 +56:26:30.9
135.74004 -4.06615 galactic Per Second-epoch detections are separated by 0.7" and 4.0 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 457613239092461312 | 02:25:45.40 +56:26:32.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.083+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:45.47 +56:26:30.9: 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 02:25:45.47 +56:26:30.9: 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 31.3529* 02 25 45.47 +56 26 30.9 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
Gaia DR3 457613239092461312,2461191.8529,8.82,0.05,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 457613239092461312 20260531.3529 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 31.3529 2461191.8529 8.76 02:26:15.74 +56:04:34.8
135.93683 -4.38245 galactic Per Second-epoch detections are separated by 1.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457463774229697408 | 02:26:15.80 +56:04:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.817+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:15.74 +56:04:34.8: 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 02:26:15.74 +56:04:34.8: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 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 31.3529* 02 26 15.74 +56 04 34.8 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 457463774229697408,2461191.8529,8.76,0.05,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
Gaia DR3 457463774229697408 20260531.3529 8.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.84 02:31:02.85 +57:39:55.6
135.96185 -2.66434 galactic Per Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.7765+57.6674 | 02:31:03.00 +57:39:54.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.190+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:02.85 +57:39:55.6: 12.72 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:02.85 +57:39:55.6: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 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 31.3529* 02 31 02.85 +57 39 55.6 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
ATO J037.7765+57.6674,2461191.8529,8.84,0.05,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 J037.7765+57.6674 20260531.3529 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 31.3529 2461191.8529 8.80 02:37:02.13 +57:41:38.8
136.68994 -2.32926 galactic Cas Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.2456+57.6870 | 02:37:02.20 +57:41:38.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.198+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:02.13 +57:41:38.8: 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 02:37:02.13 +57:41:38.8: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 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 31.3529* 02 37 02.13 +57 41 38.8 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 J039.2456+57.6870,2461191.8529,8.80,0.05,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
ATO J039.2456+57.6870 20260531.3529 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 31.3529 2461191.8529 8.82 02:23:55.69 +56:44:44.9
135.39619 -3.87095 galactic Per Second-epoch detections are separated by 0.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.9890+56.7447 | 02:23:55.57 +56:44:45.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.057+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:55.69 +56:44:44.9: 12.13 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:55.69 +56:44:44.9: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 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 31.3529* 02 23 55.69 +56 44 44.9 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 J035.9890+56.7447,2461191.8529,8.82,0.05,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
ATO J035.9890+56.7447 20260531.3529 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 31.3529 2461191.8529 8.82 02:30:39.36 +57:13:43.1
136.07676 -3.08908 galactic Per Second-epoch detections are separated by 1.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457992158286225408 | 02:30:39.37 +57:13:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.224+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:39.36 +57:13:43.1: 12.60 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:39.36 +57:13:43.1: 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 31.3529* 02 30 39.36 +57 13 43.1 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 457992158286225408,2461191.8529,8.82,0.05,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 457992158286225408 20260531.3529 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 31.3529 2461191.8529 8.86 02:31:10.50 +57:30:48.1
136.03486 -2.79889 galactic Per Second-epoch detections are separated by 0.9" and 3.9 pix
The object was found in VSX12" Gaia DR3 458067062518240768
Type: RS
# Max. Min./Amp. JD0 Period
16.780 G 16.930 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 02:31:10.50 +57:30:48.1: 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 02:31:10.50 +57:30:48.1: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 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 31.3529* 02 31 10.50 +57 30 48.1 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 458067062518240768,2461191.8529,8.86,0.05,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 458067062518240768 20260531.3529 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 31.3529 2461191.8529 8.80 02:29:26.52 +56:00:56.6
136.37360 -4.27706 galactic Per Second-epoch detections are separated by 0.6" and 4.0 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 457352620476607360 | 02:29:27.28 +56:00:57.1 (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 02:29:26.52 +56:00:56.6: 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 02:29:26.52 +56:00:56.6: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 31.3529* 02 29 26.52 +56 00 56.6 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
Gaia DR3 457352620476607360,2461191.8529,8.80,0.05,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
Gaia DR3 457352620476607360 20260531.3529 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 31.3529 2461191.8529 8.88 02:31:29.40 +56:26:22.3
136.47953 -3.77761 galactic Per Second-epoch detections are separated by 1.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457393749084094976 | 02:31:29.77 +56:26:22.6 (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 02:31:29.40 +56:26:22.3: 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 02:31:29.40 +56:26:22.3: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 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 31.3529* 02 31 29.40 +56 26 22.3 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 457393749084094976,2461191.8529,8.88,0.05,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 457393749084094976 20260531.3529 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 31.3529 2461191.8529 8.80 02:33:48.37 +56:47:59.7
136.63702 -3.32300 galactic Per Second-epoch detections are separated by 1.2" and 4.0 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 J038.4638+56.7985 | 02:33:48.59 +56:48:00.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.158+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:48.37 +56:47:59.7: 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 02:33:48.37 +56:47:59.7: 11.45 +/- 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 31.3529* 02 33 48.37 +56 47 59.7 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
ATO J038.4638+56.7985,2461191.8529,8.80,0.05,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
ATO J038.4638+56.7985 20260531.3529 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 31.3529 2461191.8529 8.88 02:33:43.66 +57:36:01.4
136.31875 -2.58826 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4540+57.5966 | 02:33:43.70 +57:36:02.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5) J-Ks=0.139+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:43.66 +57:36:01.4: 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 02:33:43.66 +57:36:01.4: 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 31.3529* 02 33 43.66 +57 36 01.4 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
ATO J038.4540+57.5966,2461191.8529,8.88,0.05,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
ATO J038.4540+57.5966 20260531.3529 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 31.3529 2461191.8529 8.86 02:34:13.61 +56:18:42.4
136.87933 -3.75096 galactic Per Second-epoch detections are separated by 2.5" and 4.3 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 457749097496685824 | 02:34:14.13 +56:18:41.0 (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 02:34:13.61 +56:18:42.4: 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 02:34:13.61 +56:18:42.4: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 31.3529* 02 34 13.61 +56 18 42.4 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 457749097496685824,2461191.8529,8.86,0.05,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 457749097496685824 20260531.3529 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 31.3529 2461191.8529 8.87 02:29:38.97 +56:11:32.5
136.33494 -4.10227 galactic Per Second-epoch detections are separated by 0.7" and 3.9 pix
The object was found in VSX 7" 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 02:29:38.97 +56:11:32.5: 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 02:29:38.97 +56:11:32.5: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 31.3529* 02 29 38.97 +56 11 32.5 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
NSV 15519,2461191.8529,8.87,0.05,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
NSV 15519 20260531.3529 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 31.3529 2461191.8529 8.82 02:30:43.84 +55:58:10.7
136.55850 -4.25273 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.6774+55.9705 | 02:30:44.39 +55:58:12.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:43.84 +55:58:10.7: 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 02:30:43.84 +55:58:10.7: 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 31.3529* 02 30 43.84 +55 58 10.7 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
ATO J037.6774+55.9705,2461191.8529,8.82,0.05,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
ATO J037.6774+55.9705 20260531.3529 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 31.3529 2461191.8529 8.86 02:26:00.85 +56:46:18.6
135.65490 -3.74541 galactic Per Second-epoch detections are separated by 1.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:26:00.85 +56:46:18.6: 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 02:26:00.85 +56:46:18.6: 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 31.3529* 02 26 00.85 +56 46 18.6 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 457636122678005120,2461191.8529,8.86,0.05,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 457636122678005120 20260531.3529 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 31.3529 2461191.8529 8.80 02:27:59.54 +56:09:19.1
136.13358 -4.22156 galactic Per Second-epoch detections are separated by 1.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457545614823486720 | 02:27:59.64 +56:09:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.917+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:59.54 +56:09:19.1: 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 02:27:59.54 +56:09:19.1: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 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 31.3529* 02 27 59.54 +56 09 19.1 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 457545614823486720,2461191.8529,8.80,0.05,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
Gaia DR3 457545614823486720 20260531.3529 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 31.3529 2461191.8529 8.97 02:30:51.75 +57:15:44.4
136.09007 -3.04738 galactic Per Second-epoch detections are separated by 1.3" and 4.0 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 457992604962793984 | 02:30:51.79 +57:15:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.287+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:51.75 +57:15:44.4: 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 02:30:51.75 +57:15:44.4: 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 31.3529* 02 30 51.75 +57 15 44.4 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
Gaia DR3 457992604962793984,2461191.8529,8.97,0.05,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
Gaia DR3 457992604962793984 20260531.3529 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 31.3529 2461191.8529 8.93 02:21:55.10 +56:20:50.0
135.27431 -4.34085 galactic Per Second-epoch detections are separated by 1.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458277893873461120 | 02:21:55.07 +56:20:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:55.10 +56:20:50.0: 8.61 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:55.10 +56:20:50.0: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.03 +/- 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 31.3529* 02 21 55.10 +56 20 50.0 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
Gaia DR3 458277893873461120,2461191.8529,8.93,0.05,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
Gaia DR3 458277893873461120 20260531.3529 8.93CV 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 31.3529 2461191.8529 8.89 02:31:12.59 +57:00:49.8
136.22721 -3.26004 galactic Per Second-epoch detections are separated by 0.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457980098018246784 | 02:31:12.49 +57:00:49.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.263+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:12.59 +57:00:49.8: 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 02:31:12.59 +57:00:49.8: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 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 31.3529* 02 31 12.59 +57 00 49.8 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 457980098018246784,2461191.8529,8.89,0.05,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
Gaia DR3 457980098018246784 20260531.3529 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 31.3529 2461191.8529 8.91 02:26:08.81 +56:16:07.7
135.85256 -4.20854 galactic Per Second-epoch detections are separated by 4.1" and 4.4 pix
The object was found in VSX23" ZTF J022611.58+561604.9
Type: RS
# Max. Min./Amp. JD0 Period
19.739 r Y 0.357 r 2458514.61170 3.605615400000
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 02:26:08.81 +56:16:07.7: 10.53 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:08.81 +56:16:07.7: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 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 31.3529* 02 26 08.81 +56 16 07.7 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
ZTF J022611.58+561604.9,2461191.8529,8.91,0.05,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
ZTF J022611.58+561604.9 20260531.3529 8.91CV 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 31.3529 2461191.8529 8.96 02:30:41.06 +55:56:25.5
136.56345 -4.28225 galactic Per Second-epoch detections are separated by 1.2" and 4.1 pix
The object was found in VSX 8" ASASSN-V J023041.92+555622.1
Type: L
# Max. Min./Amp. JD0 Period
12.500 V 12.680 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 02:30:41.06 +55:56:25.5: 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 02:30:41.06 +55:56:25.5: 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 31.3529* 02 30 41.06 +55 56 25.5 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 J023041.92+555622.1,2461191.8529,8.96,0.05,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 J023041.92+555622.1 20260531.3529 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 31.3529 2461191.8529 8.87 02:35:00.16 +56:43:10.4
136.81962 -3.33361 galactic Per Second-epoch detections are separated by 1.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457764520717250560 | 02:35:00.38 +56:43:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.105+/-0.026 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:00.16 +56:43:10.4: 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 02:35:00.16 +56:43:10.4: 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 31.3529* 02 35 00.16 +56 43 10.4 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 457764520717250560,2461191.8529,8.87,0.05,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
Gaia DR3 457764520717250560 20260531.3529 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 31.3529 2461191.8529 8.93 02:24:32.07 +56:43:35.5
135.48100 -3.85978 galactic Per Second-epoch detections are separated by 1.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457633511337779584 | 02:24:32.08 +56:43:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.763+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:32.07 +56:43:35.5: 11.70 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:32.07 +56:43:35.5: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 31.3529* 02 24 32.07 +56 43 35.5 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
Gaia DR3 457633511337779584,2461191.8529,8.93,0.05,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
Gaia DR3 457633511337779584 20260531.3529 8.93CV 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 31.3529 2461191.8529 8.85 02:32:18.81 +56:15:24.2
136.65472 -3.90361 galactic Per Second-epoch detections are separated by 1.0" and 3.8 pix
The object was found in VSX 5" Gaia DR3 457388045367612800
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.410 G 11.440 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 02:32:18.81 +56:15:24.2: 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 02:32:18.81 +56:15:24.2: 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 31.3529* 02 32 18.81 +56 15 24.2 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 457388045367612800,2461191.8529,8.85,0.05,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 457388045367612800 20260531.3529 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 31.3529 2461191.8529 9.01 02:30:17.06 +56:38:11.7
136.25109 -3.65725 galactic Per Second-epoch detections are separated by 2.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:30:17.06 +56:38:11.7: 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 02:30:17.06 +56:38:11.7: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 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 31.3529* 02 30 17.06 +56 38 11.7 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
Gaia DR3 457587263129458432,2461191.8529,9.01,0.05,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 457587263129458432 20260531.3529 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 31.3529 2461191.8529 8.82 02:23:38.16 +56:39:53.3
135.38694 -3.96086 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458288476672646272 | 02:23:38.16 +56:39:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.043+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:38.16 +56:39:53.3: 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 02:23:38.16 +56:39:53.3: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 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 31.3529* 02 23 38.16 +56 39 53.3 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 458288476672646272,2461191.8529,8.82,0.05,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 458288476672646272 20260531.3529 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 31.3529 2461191.8529 8.96 02:24:25.95 +56:32:57.3
135.53045 -4.03064 galactic Per Second-epoch detections are separated by 0.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.1043+56.5466 | 02:24:25.88 +56:32:56.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.365+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:25.95 +56:32:57.3: 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 02:24:25.95 +56:32:57.3: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 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 31.3529* 02 24 25.95 +56 32 57.3 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 J036.1043+56.5466,2461191.8529,8.96,0.05,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
ATO J036.1043+56.5466 20260531.3529 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 31.3529 2461191.8529 8.95 02:28:40.95 +56:12:03.5
136.20643 -4.14390 galactic Per Second-epoch detections are separated by 3.2" and 3.9 pix
The object was found in VSX 6" 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 02:28:40.95 +56:12:03.5: 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 02:28:40.95 +56:12:03.5: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 31.3529* 02 28 40.95 +56 12 03.5 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
ASASSN-V J022841.63+561200.9,2461191.8529,8.95,0.05,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
ASASSN-V J022841.63+561200.9 20260531.3529 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 31.3529 2461191.8529 8.91 02:28:21.40 +55:58:55.7
136.24453 -4.36415 galactic Per Second-epoch detections are separated by 1.1" and 4.0 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 | ZTF J022823.76+555916.0 | 02:28:22.11 +55:58:55.9 (Gaia DR3) | EW (local) | 2458432.78280 (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 02:28:21.40 +55:58:55.7: 11.12 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:21.40 +55:58:55.7: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 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 31.3529* 02 28 21.40 +55 58 55.7 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
ZTF J022823.76+555916.0,2461191.8529,8.91,0.05,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
ZTF J022823.76+555916.0 20260531.3529 8.91CV 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 31.3529 2461191.8529 8.88 02:33:50.71 +55:59:56.9
136.95120 -4.05987 galactic Per Second-epoch detections are separated by 1.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457322349546464896 | 02:33:51.13 +55:59:55.4 (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 02:33:50.71 +55:59:56.9: 12.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:50.71 +55:59:56.9: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 31.3529* 02 33 50.71 +55 59 56.9 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 457322349546464896,2461191.8529,8.88,0.05,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 457322349546464896 20260531.3529 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 31.3529 2461191.8529 9.03 02:31:51.47 +56:45:50.3
136.40370 -3.45808 galactic Per Second-epoch detections are separated by 1.0" and 4.0 pix
The object was found in VSX 5" 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 02:31:51.47 +56:45:50.3: 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 02:31:51.47 +56:45:50.3: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 31.3529* 02 31 51.47 +56 45 50.3 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
NSV 15534,2461191.8529,9.03,0.05,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
NSV 15534 20260531.3529 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 31.3529 2461191.8529 8.94 02:31:03.02 +55:52:01.4
136.63873 -4.33101 galactic Per Second-epoch detections are separated by 2.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457340938165655808 | 02:31:03.60 +55:52:02.6 (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 02:31:03.02 +55:52:01.4: 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 02:31:03.02 +55:52:01.4: 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 31.3529* 02 31 03.02 +55 52 01.4 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 457340938165655808,2461191.8529,8.94,0.05,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 457340938165655808 20260531.3529 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 31.3529 2461191.8529 8.96 02:35:12.95 +57:56:23.8
136.37030 -2.19838 galactic Cas Second-epoch detections are separated by 3.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.7838+57.9436 | 02:35:13.01 +57:56:24.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.393+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:12.95 +57:56:23.8: 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 02:35:12.95 +57:56:23.8: 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 31.3529* 02 35 12.95 +57 56 23.8 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
ATO J038.7838+57.9436,2461191.8529,8.96,0.05,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
ATO J038.7838+57.9436 20260531.3529 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 31.3529 2461191.8529 8.99 02:30:23.25 +56:23:34.2
136.35545 -3.87809 galactic Per Second-epoch detections are separated by 1.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457574584386224384 | 02:30:23.48 +56:23:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.092+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:23.25 +56:23:34.2: 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 02:30:23.25 +56:23:34.2: 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 31.3529* 02 30 23.25 +56 23 34.2 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 457574584386224384,2461191.8529,8.99,0.05,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
Gaia DR3 457574584386224384 20260531.3529 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 31.3529 2461191.8529 9.06 02:37:31.30 +57:29:01.8
136.83332 -2.49640 galactic Per Second-epoch detections are separated by 0.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457916253319743616 | 02:37:31.82 +57:28:17.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.869+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:31.30 +57:29:01.8: 10.25 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:31.30 +57:29:01.8: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 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 31.3529* 02 37 31.30 +57 29 01.8 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 457916253319743616,2461191.8529,9.06,0.05,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
Gaia DR3 457916253319743616 20260531.3529 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 31.3529 2461191.8529 8.96 02:24:47.85 +56:36:57.7
135.55397 -3.95042 galactic Per Second-epoch detections are separated by 1.2" and 4.0 pix
The object was found in VSX 1" Gaia DR3 457630522034972416
Type: ROT
# Max. Min./Amp. JD0 Period
11.410 G 11.460 G 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 02:24:47.85 +56:36:57.7: 12.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:47.85 +56:36:57.7: 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 31.3529* 02 24 47.85 +56 36 57.7 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
Gaia DR3 457630522034972416,2461191.8529,8.96,0.05,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
Gaia DR3 457630522034972416 20260531.3529 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 31.3529 2461191.8529 8.88 02:34:03.05 +56:00:36.1
136.97358 -4.03873 galactic Per Second-epoch detections are separated by 3.7" and 4.6 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 457322280826978560 | 02:34:03.58 +56:00:36.7 (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 02:34:03.05 +56:00:36.1: 12.92 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:03.05 +56:00:36.1: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 31.3529* 02 34 03.05 +56 00 36.1 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 457322280826978560,2461191.8529,8.88,0.05,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 457322280826978560 20260531.3529 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 31.3529 2461191.8529 9.06 02:26:59.37 +57:14:45.3
135.60836 -3.25528 galactic Per Second-epoch detections are separated by 1.4" and 4.0 pix
The object was found in VSX 3" ASASSN-V J022659.55+571443.3
Type: SR
# Max. Min./Amp. JD0 Period
13.400 g Y 0.150 g 2458680.08400 226.000000000000
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 02:26:59.37 +57:14:45.3: 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 02:26:59.37 +57:14:45.3: 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 31.3529* 02 26 59.37 +57 14 45.3 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
ASASSN-V J022659.55+571443.3,2461191.8529,9.06,0.05,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
ASASSN-V J022659.55+571443.3 20260531.3529 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 31.3529 2461191.8529 8.94 02:33:48.54 +55:57:07.4
136.96472 -4.10527 galactic Per Second-epoch detections are separated by 0.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4666+55.9563 | 02:33:49.36 +55:57:06.8 (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 02:33:48.54 +55:57:07.4: 12.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:48.54 +55:57:07.4: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 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 31.3529* 02 33 48.54 +55 57 07.4 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
ATO J038.4666+55.9563,2461191.8529,8.94,0.05,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
ATO J038.4666+55.9563 20260531.3529 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 31.3529 2461191.8529 8.97 02:33:37.62 +57:40:24.0
136.27824 -2.52610 galactic Per Second-epoch detections are separated by 1.9" and 4.0 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 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 02:33:37.62 +57:40:24.0: 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 02:33:37.62 +57:40:24.0: 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 31.3529* 02 33 37.62 +57 40 24.0 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
ATO J038.4074+57.6734,2461191.8529,8.97,0.05,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
ATO J038.4074+57.6734 20260531.3529 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 31.3529 2461191.8529 9.07 02:24:38.05 +56:49:55.5
135.45650 -3.75619 galactic Per Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458384958817070464 | 02:24:38.24 +56:49:54.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.102+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:38.05 +56:49:55.5: 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 02:24:38.05 +56:49:55.5: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 31.3529* 02 24 38.05 +56 49 55.5 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
Gaia DR3 458384958817070464,2461191.8529,9.07,0.05,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 458384958817070464 20260531.3529 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 31.3529 2461191.8529 9.03 02:24:18.80 +56:19:50.2
135.59216 -4.24108 galactic Per Second-epoch detections are separated by 0.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.0889+56.3355 | 02:24:18.85 +56:19:48.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.954+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:18.80 +56:19:50.2: 12.21 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:18.80 +56:19:50.2: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 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 31.3529* 02 24 18.80 +56 19 50.2 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 J036.0889+56.3355,2461191.8529,9.03,0.05,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 J036.0889+56.3355 20260531.3529 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 31.3529 2461191.8529 9.12 02:37:24.10 +57:31:04.5
136.80496 -2.47154 galactic Per Second-epoch detections are separated by 1.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.3502+57.5182 | 02:37:24.05 +57:31:05.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.187+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:24.10 +57:31:04.5: 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 02:37:24.10 +57:31:04.5: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 31.3529* 02 37 24.10 +57 31 04.5 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 J039.3502+57.5182,2461191.8529,9.12,0.05,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
ATO J039.3502+57.5182 20260531.3529 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 31.3529 2461191.8529 8.96 02:32:35.10 +57:32:19.9
136.20062 -2.70372 galactic Per Second-epoch detections are separated by 2.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1472+57.5426 | 02:32:35.23 +57:32:21.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +57 44 J-Ks=0.136+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:35.10 +57:32:19.9: 12.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:35.10 +57:32:19.9: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 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 31.3529* 02 32 35.10 +57 32 19.9 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 J038.1472+57.5426,2461191.8529,8.96,0.05,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
ATO J038.1472+57.5426 20260531.3529 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 31.3529 2461191.8529 8.99 02:28:56.59 +56:11:02.8
136.24645 -4.14625 galactic Per Second-epoch detections are separated by 0.9" and 3.7 pix
The object was found in VSX13" ZTF J022856.73+561050.0
Type: RS
# Max. Min./Amp. JD0 Period
16.955 r Y 0.059 r 2458475.80570 0.641758300000
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 02:28:56.59 +56:11:02.8: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:56.59 +56:11:02.8: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 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 31.3529* 02 28 56.59 +56 11 02.8 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
ZTF J022856.73+561050.0,2461191.8529,8.99,0.05,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
ZTF J022856.73+561050.0 20260531.3529 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 31.3529 2461191.8529 8.91 02:25:30.05 +56:16:52.2
135.76416 -4.22903 galactic Per Second-epoch detections are separated by 1.4" and 4.1 pix
The object was found in VSX15" 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 02:25:30.05 +56:16:52.2: 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 02:25:30.05 +56:16:52.2: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 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 31.3529* 02 25 30.05 +56 16 52.2 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 457517925178383616,2461191.8529,8.91,0.05,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
Gaia DR3 457517925178383616 20260531.3529 8.91CV 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 31.3529 2461191.8529 9.05 02:26:02.34 +56:21:00.8
135.80933 -4.13788 galactic Per Second-epoch detections are separated by 1.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.5102+56.3494 | 02:26:02.46 +56:20:57.9 (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 02:26:02.34 +56:21:00.8: 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 02:26:02.34 +56:21:00.8: 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 31.3529* 02 26 02.34 +56 21 00.8 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+56.3494,2461191.8529,9.05,0.05,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 J036.5102+56.3494 20260531.3529 9.05CV 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 31.3529 2461191.8529 9.11 02:27:34.54 +56:16:51.2
136.03364 -4.12570 galactic Per Second-epoch detections are separated by 1.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.8823+56.2862 | 02:27:34.40 +56:16:53.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.111+/-0.025 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:34.54 +56:16:51.2: 10.89 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:34.54 +56:16:51.2: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 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 31.3529* 02 27 34.54 +56 16 51.2 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 J036.8823+56.2862,2461191.8529,9.11,0.05,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
ATO J036.8823+56.2862 20260531.3529 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 31.3529 2461191.8529 9.05 02:33:57.28 +57:00:01.2
136.57842 -3.13025 galactic Per Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457807062374815488 | 02:33:57.36 +57:00:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.235+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:57.28 +57:00:01.2: 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 02:33:57.28 +57:00:01.2: 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 31.3529* 02 33 57.28 +57 00 01.2 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 457807062374815488,2461191.8529,9.05,0.05,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
Gaia DR3 457807062374815488 20260531.3529 9.05CV 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 31.3529 2461191.8529 9.08 02:25:48.44 +56:32:34.9
135.71025 -3.96926 galactic Per Second-epoch detections are separated by 1.3" and 3.7 pix
The object was found in VSX 9" ZTF J022547.44+563230.2
Type: EW
# Max. Min./Amp. JD0 Period
18.914 g Y 0.532 g 2458358.95060 0.320093600000
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 02:25:48.44 +56:32:34.9: 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 02:25:48.44 +56:32:34.9: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 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 31.3529* 02 25 48.44 +56 32 34.9 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
ZTF J022547.44+563230.2,2461191.8529,9.08,0.05,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
ZTF J022547.44+563230.2 20260531.3529 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 31.3529 2461191.8529 9.12 02:32:31.36 +57:38:51.5
136.15146 -2.60630 galactic Per Second-epoch detections are separated by 3.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1455+57.6377 | 02:32:31.40 +57:38:50.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.746+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:31.36 +57:38:51.5: 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 02:32:31.36 +57:38:51.5: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 31.3529* 02 32 31.36 +57 38 51.5 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 J038.1455+57.6377,2461191.8529,9.12,0.05,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
ATO J038.1455+57.6377 20260531.3529 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 31.3529 2461191.8529 9.07 02:29:55.76 +56:55:49.8
136.09629 -3.40253 galactic Per Second-epoch detections are separated by 2.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.4814+56.9308 | 02:29:55.55 +56:55:50.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +56 50 J-Ks=0.125+/-0.063 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:55.76 +56:55:49.8: 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 02:29:55.76 +56:55:49.8: 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 31.3529* 02 29 55.76 +56 55 49.8 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 J037.4814+56.9308,2461191.8529,9.07,0.05,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
ATO J037.4814+56.9308 20260531.3529 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 31.3529 2461191.8529 9.05 02:25:32.72 +56:32:56.9
135.67425 -3.97643 galactic Per Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457626261433241088 | 02:25:32.86 +56:32:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.674+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:32.72 +56:32:56.9: 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 02:25:32.72 +56:32:56.9: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 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 31.3529* 02 25 32.72 +56 32 56.9 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 457626261433241088,2461191.8529,9.05,0.05,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
Gaia DR3 457626261433241088 20260531.3529 9.05CV 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 31.3529 2461191.8529 9.09 02:32:23.05 +57:38:37.3
136.13580 -2.61699 galactic Per Second-epoch detections are separated by 0.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458074312422945920 | 02:32:23.20 +57:38:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5) J-Ks=1.170+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:23.05 +57:38:37.3: 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 02:32:23.05 +57:38:37.3: 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 31.3529* 02 32 23.05 +57 38 37.3 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 458074312422945920,2461191.8529,9.09,0.05,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
Gaia DR3 458074312422945920 20260531.3529 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 31.3529 2461191.8529 9.13 02:27:37.42 +57:04:56.0
135.74801 -3.37674 galactic Per Second-epoch detections are separated by 3.9" and 4.0 pix
The object was found in VSX13" ASASSN-V J022738.67+570504.7
Type: EA
# Max. Min./Amp. JD0 Period
12.000 V 12.960 V 2458021.91000 0.604640000000
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 02:27:37.42 +57:04:56.0: 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 02:27:37.42 +57:04:56.0: 12.03 +/- 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 31.3529* 02 27 37.42 +57 04 56.0 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
ASASSN-V J022738.67+570504.7,2461191.8529,9.13,0.05,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
ASASSN-V J022738.67+570504.7 20260531.3529 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 31.3529 2461191.8529 9.22 02:33:44.26 +56:59:33.8
136.55404 -3.14866 galactic Per Second-epoch detections are separated by 1.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457783766472214656 | 02:33:44.33 +56:59:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:44.26 +56:59:33.8: 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 02:33:44.26 +56:59:33.8: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 31.3529* 02 33 44.26 +56 59 33.8 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 457783766472214656,2461191.8529,9.22,0.05,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 457783766472214656 20260531.3529 9.22CV 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 31.3529 2461191.8529 9.04 02:27:52.24 +56:29:30.2
135.99485 -3.91446 galactic Per Second-epoch detections are separated by 1.3" and 4.0 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 457570186338640384 | 02:27:52.24 +56:29:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.085+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:52.24 +56:29:30.2: 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 02:27:52.24 +56:29:30.2: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 31.3529* 02 27 52.24 +56 29 30.2 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 457570186338640384,2461191.8529,9.04,0.05,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
Gaia DR3 457570186338640384 20260531.3529 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 31.3529 2461191.8529 9.06 02:38:39.71 +57:47:02.7
136.85320 -2.16019 galactic Cas Second-epoch detections are separated by 0.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457945738276700928 | 02:38:39.74 +57:47:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.156+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:39.71 +57:47:02.7: 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 02:38:39.71 +57:47:02.7: 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 31.3529* 02 38 39.71 +57 47 02.7 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
Gaia DR3 457945738276700928,2461191.8529,9.06,0.05,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
Gaia DR3 457945738276700928 20260531.3529 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 31.3529 2461191.8529 9.07 02:25:11.61 +56:17:21.6
135.72128 -4.23656 galactic Per Second-epoch detections are separated by 0.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457518062614937344 | 02:25:11.61 +56:17:21.6 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.730+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:11.61 +56:17:21.6: 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 02:25:11.61 +56:17:21.6: 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 31.3529* 02 25 11.61 +56 17 21.6 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
Large-amplitude variable Gaia DR2 457518062614937344,2461191.8529,9.07,0.05,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
Large-amplitude variable Gaia DR2 457518062614937344 20260531.3529 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 31.3529 2461191.8529 9.11 02:30:00.33 +57:11:29.3
136.00879 -3.15640 galactic Per Second-epoch detections are separated by 3.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458032874577920256 | 02:30:00.30 +57:11:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.154+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:00.33 +57:11:29.3: 12.61 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:00.33 +57:11:29.3: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 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 31.3529* 02 30 00.33 +57 11 29.3 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 458032874577920256,2461191.8529,9.11,0.05,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
Gaia DR3 458032874577920256 20260531.3529 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 31.3529 2461191.8529 8.95 02:33:42.17 +55:51:19.1
136.98833 -4.20028 galactic Per Second-epoch detections are separated by 1.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457312453941894912 | 02:33:43.08 +55:51:18.6 (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 02:33:42.17 +55:51:19.1: 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 02:33:42.17 +55:51:19.1: 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 31.3529* 02 33 42.17 +55 51 19.1 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 457312453941894912,2461191.8529,8.95,0.05,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
Gaia DR3 457312453941894912 20260531.3529 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 31.3529 2461191.8529 9.19 02:32:49.37 +57:34:23.1
136.21709 -2.65993 galactic Per Second-epoch detections are separated by 2.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2179+57.5617 | 02:32:49.16 +57:34:21.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.222+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:49.37 +57:34:23.1: 10.36 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:49.37 +57:34:23.1: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 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 31.3529* 02 32 49.37 +57 34 23.1 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
ATO J038.2179+57.5617,2461191.8529,9.19,0.05,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
ATO J038.2179+57.5617 20260531.3529 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 31.3529 2461191.8529 9.13 02:30:32.60 +57:32:13.7
135.94723 -2.80860 galactic Per Second-epoch detections are separated by 2.0" and 4.0 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 J037.6273+57.5323 | 02:30:32.62 +57:32:13.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1965LS....C05....0H LS V +57 40 J-Ks=0.149+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:32.60 +57:32:13.7: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:32.60 +57:32:13.7: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 31.3529* 02 30 32.60 +57 32 13.7 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 J037.6273+57.5323,2461191.8529,9.13,0.05,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
ATO J037.6273+57.5323 20260531.3529 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 31.3529 2461191.8529 9.02 02:30:00.36 +56:17:43.0
136.34272 -3.98832 galactic Per Second-epoch detections are separated by 0.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457549639215308800 | 02:30:00.77 +56:17:41.2 (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 02:30:00.36 +56:17:43.0: 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 02:30:00.36 +56:17:43.0: 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 31.3529* 02 30 00.36 +56 17 43.0 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
Gaia DR3 457549639215308800,2461191.8529,9.02,0.05,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
Gaia DR3 457549639215308800 20260531.3529 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 31.3529 2461191.8529 9.09 02:35:26.59 +57:46:13.0
136.46440 -2.34281 galactic Cas Second-epoch detections are separated by 2.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:35:26.59 +57:46:13.0 (user input) | T | P | (position from user input) J-Ks=0.609+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:26.59 +57:46:13.0: 10.44 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:26.59 +57:46:13.0: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 31.3529* 02 35 26.59 +57 46 13.0 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
target,2461191.8529,9.09,0.05,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
target 20260531.3529 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 31.3529 2461191.8529 9.01 02:30:38.21 +56:11:54.0
136.46048 -4.04557 galactic Per Second-epoch detections are separated by 0.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457360523216287616 | 02:30:38.75 +56:11:55.5 (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 02:30:38.21 +56:11:54.0: 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 02:30:38.21 +56:11:54.0: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 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 31.3529* 02 30 38.21 +56 11 54.0 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
Gaia DR3 457360523216287616,2461191.8529,9.01,0.05,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 457360523216287616 20260531.3529 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 31.3529 2461191.8529 9.08 02:36:19.07 +57:07:02.5
136.82904 -2.89730 galactic Per Second-epoch detections are separated by 0.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457800671463350272 | 02:36:19.22 +57:06:56.9 (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 02:36:19.07 +57:07:02.5: 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 02:36:19.07 +57:07:02.5: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 31.3529* 02 36 19.07 +57 07 02.5 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
Gaia DR3 457800671463350272,2461191.8529,9.08,0.05,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 457800671463350272 20260531.3529 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 31.3529 2461191.8529 9.01 02:36:27.53 +56:56:51.3
136.91367 -3.04579 galactic Per Second-epoch detections are separated by 0.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.1156+56.9471 | 02:36:27.75 +56:56:49.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.105+/-0.040 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:27.53 +56:56:51.3: 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 02:36:27.53 +56:56:51.3: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 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 31.3529* 02 36 27.53 +56 56 51.3 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 J039.1156+56.9471,2461191.8529,9.01,0.05,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
ATO J039.1156+56.9471 20260531.3529 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 31.3529 2461191.8529 9.27 02:23:11.07 +56:11:20.3
135.49459 -4.42860 galactic Per Second-epoch detections are separated by 1.4" and 4.0 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 J035.7975+56.1884 | 02:23:11.42 +56:11:18.4 (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 02:23:11.07 +56:11:20.3: 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 02:23:11.07 +56:11:20.3: 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 31.3529* 02 23 11.07 +56 11 20.3 9.3 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 J035.7975+56.1884,2461191.8529,9.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J035.7975+56.1884 20260531.3529 9.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.14 02:22:11.90 +56:20:47.6
135.31107 -4.32814 galactic Per Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.5526+56.3433 | 02:22:11.88 +56:20:47.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.152+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:11.90 +56:20:47.6: 12.47 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:11.90 +56:20:47.6: 11.76 +/- 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 31.3529* 02 22 11.90 +56 20 47.6 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 J035.5526+56.3433,2461191.8529,9.14,0.05,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 J035.5526+56.3433 20260531.3529 9.14CV 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 31.3529 2461191.8529 9.21 02:29:10.75 +55:58:47.7
136.35264 -4.32391 galactic Per Second-epoch detections are separated by 2.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457352135136621312 | 02:29:11.56 +55:58:47.1 (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 02:29:10.75 +55:58:47.7: 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 02:29:10.75 +55:58:47.7: 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 31.3529* 02 29 10.75 +55 58 47.7 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 457352135136621312,2461191.8529,9.21,0.05,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
Gaia DR3 457352135136621312 20260531.3529 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 31.3529 2461191.8529 9.12 02:30:45.38 +57:06:30.4
136.13443 -3.19546 galactic Per Second-epoch detections are separated by 1.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457984835359661824 | 02:30:45.30 +57:06:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.083+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:45.38 +57:06:30.4: 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 02:30:45.38 +57:06:30.4: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 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 31.3529* 02 30 45.38 +57 06 30.4 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 457984835359661824,2461191.8529,9.12,0.05,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 457984835359661824 20260531.3529 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 31.3529 2461191.8529 9.11 02:36:19.41 +57:59:11.1
136.48735 -2.09809 galactic Cas Second-epoch detections are separated by 2.0" and 3.5 pix
The object was found in VSX 2" Gaia DR3 458141623148023296
Type: ROT
# Max. Min./Amp. JD0 Period
12.480 G 12.520 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 02:36:19.41 +57:59:11.1: 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 02:36:19.41 +57:59:11.1: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 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 31.3529* 02 36 19.41 +57 59 11.1 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 458141623148023296,2461191.8529,9.11,0.05,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
Gaia DR3 458141623148023296 20260531.3529 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 31.3529 2461191.8529 9.09 02:33:28.12 +56:18:30.6
136.78337 -3.79451 galactic Per Second-epoch detections are separated by 1.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3673+56.3061 | 02:33:28.77 +56:18:31.0 (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 02:33:28.12 +56:18:30.6: 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 02:33:28.12 +56:18:30.6: 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 31.3529* 02 33 28.12 +56 18 30.6 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 J038.3673+56.3061,2461191.8529,9.09,0.05,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
ATO J038.3673+56.3061 20260531.3529 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 31.3529 2461191.8529 9.05 02:27:07.63 +56:00:29.5
136.07444 -4.40248 galactic Per Second-epoch detections are separated by 1.7" and 4.2 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 J036.7922+56.0057 | 02:27:07.59 +56:00:28.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.227+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:07.63 +56:00:29.5: 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 02:27:07.63 +56:00:29.5: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 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 31.3529* 02 27 07.63 +56 00 29.5 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 J036.7922+56.0057,2461191.8529,9.05,0.05,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 J036.7922+56.0057 20260531.3529 9.05CV 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 31.3529 2461191.8529 9.28 02:34:32.01 +57:40:32.0
136.38929 -2.47730 galactic Per Second-epoch detections are separated by 0.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458118877000959872 | 02:34:32.11 +57:40:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.185+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:32.01 +57:40:32.0: 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 02:34:32.01 +57:40:32.0: 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 31.3529* 02 34 32.01 +57 40 32.0 9.3 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 458118877000959872,2461191.8529,9.28,0.05,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
Gaia DR3 458118877000959872 20260531.3529 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 31.3529 2461191.8529 9.11 02:24:52.39 +56:43:11.8
135.52689 -3.84954 galactic Per Second-epoch detections are separated by 1.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457632652344319616 | 02:24:52.42 +56:43:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.731+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:52.39 +56:43:11.8: 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 02:24:52.39 +56:43:11.8: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 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 31.3529* 02 24 52.39 +56 43 11.8 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 457632652344319616,2461191.8529,9.11,0.05,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
Gaia DR3 457632652344319616 20260531.3529 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 31.3529 2461191.8529 9.24 02:23:08.55 +56:20:25.7
135.43627 -4.28859 galactic Per Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457527816479322752 | 02:23:08.49 +56:20:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.050+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:08.55 +56:20:25.7: 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 02:23:08.55 +56:20:25.7: 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 31.3529* 02 23 08.55 +56 20 25.7 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 457527816479322752,2461191.8529,9.24,0.05,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 457527816479322752 20260531.3529 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 31.3529 2461191.8529 9.09 02:30:28.93 +56:19:35.0
136.39251 -3.93483 galactic Per Second-epoch detections are separated by 1.1" and 4.0 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 457573381795409408 | 02:30:29.42 +56:19:34.1 (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 02:30:28.93 +56:19:35.0: 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 02:30:28.93 +56:19:35.0: 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 31.3529* 02 30 28.93 +56 19 35.0 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 457573381795409408,2461191.8529,9.09,0.05,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
Gaia DR3 457573381795409408 20260531.3529 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 31.3529 2461191.8529 9.15 02:34:13.74 +56:19:38.4
136.87358 -3.73650 galactic Per Second-epoch detections are separated by 2.1" and 4.2 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 J038.5642+56.3253 | 02:34:14.03 +56:19:38.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.205+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.74 +56:19:38.4: 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 02:34:13.74 +56:19:38.4: 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 31.3529* 02 34 13.74 +56 19 38.4 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
ATO J038.5642+56.3253,2461191.8529,9.15,0.05,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
ATO J038.5642+56.3253 20260531.3529 9.15CV 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 31.3529 2461191.8529 9.28 02:29:11.14 +57:21:01.2
135.84681 -3.04984 galactic Per Second-epoch detections are separated by 1.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458038745789149824 | 02:29:11.20 +57:20:59.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.788+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:11.14 +57:21:01.2: 12.77 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:11.14 +57:21:01.2: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 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 31.3529* 02 29 11.14 +57 21 01.2 9.3 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 458038745789149824,2461191.8529,9.28,0.05,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
Gaia DR3 458038745789149824 20260531.3529 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 31.3529 2461191.8529 9.21 02:36:41.43 +57:37:08.6
136.67723 -2.41644 galactic Cas Second-epoch detections are separated by 2.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.1865+57.6232 | 02:36:41.37 +57:37:09.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.293+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:41.43 +57:37:08.6: 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 02:36:41.43 +57:37:08.6: 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 31.3529* 02 36 41.43 +57 37 08.6 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
ATO J039.1865+57.6232,2461191.8529,9.21,0.05,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
ATO J039.1865+57.6232 20260531.3529 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 31.3529 2461191.8529 9.26 02:22:47.61 +56:11:10.3
135.44439 -4.45009 galactic Per Second-epoch detections are separated by 0.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7007+56.1904 | 02:22:47.64 +56:11:09.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.443+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:47.61 +56:11:10.3: 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 02:22:47.61 +56:11:10.3: 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 31.3529* 02 22 47.61 +56 11 10.3 9.3 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 J035.7007+56.1904,2461191.8529,9.26,0.05,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
ATO J035.7007+56.1904 20260531.3529 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 31.3529 2461191.8529 9.18 02:24:38.48 +56:20:47.1
135.62922 -4.21027 galactic Per Second-epoch detections are separated by 2.1" and 4.2 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 J036.1775+56.3470 | 02:24:38.69 +56:20:47.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:38.48 +56:20:47.1: 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 02:24:38.48 +56:20:47.1: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 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 31.3529* 02 24 38.48 +56 20 47.1 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
ATO J036.1775+56.3470,2461191.8529,9.18,0.05,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
ATO J036.1775+56.3470 20260531.3529 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 31.3529 2461191.8529 9.19 02:32:04.85 +56:53:51.0
136.38133 -3.32294 galactic Per Second-epoch detections are separated by 1.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457966972598282368 | 02:32:05.00 +56:53:49.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.151+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:04.85 +56:53:51.0: 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 02:32:04.85 +56:53:51.0: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 31.3529* 02 32 04.85 +56 53 51.0 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 457966972598282368,2461191.8529,9.19,0.05,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
Gaia DR3 457966972598282368 20260531.3529 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 31.3529 2461191.8529 9.13 02:27:42.05 +56:12:16.6
136.07769 -4.19043 galactic Per Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457557713753714944 | 02:27:42.19 +56:12:18.8 (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 02:27:42.05 +56:12:16.6: 13.04 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:42.05 +56:12:16.6: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 31.3529* 02 27 42.05 +56 12 16.6 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 457557713753714944,2461191.8529,9.13,0.05,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 457557713753714944 20260531.3529 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 31.3529 2461191.8529 9.34 02:30:07.04 +56:30:20.7
136.27854 -3.78723 galactic Per Second-epoch detections are separated by 3.5" and 3.7 pix
The object was found in VSX 4" ASASSN-V J023007.46+563018.2
Type: L
# Max. Min./Amp. JD0 Period
12.620 V 12.910 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 02:30:07.04 +56:30:20.7: 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 02:30:07.04 +56:30:20.7: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 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 31.3529* 02 30 07.04 +56 30 20.7 9.3 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
ASASSN-V J023007.46+563018.2,2461191.8529,9.34,0.05,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 J023007.46+563018.2 20260531.3529 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 31.3529 2461191.8529 9.20 02:23:56.97 +56:11:52.3
135.59148 -4.38311 galactic Per Second-epoch detections are separated by 6.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.9838+56.2016 | 02:23:57.00 +56:11:54.9 (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 02:23:56.97 +56:11:52.3: 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 02:23:56.97 +56:11:52.3: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 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 31.3529* 02 23 56.97 +56 11 52.3 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
ATO J035.9838+56.2016,2461191.8529,9.20,0.05,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
ATO J035.9838+56.2016 20260531.3529 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 31.3529 2461191.8529 9.14 02:27:15.92 +56:00:28.3
136.09262 -4.39580 galactic Per Second-epoch detections are separated by 0.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457460750572377984 | 02:27:16.14 +56:00:27.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.958+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:15.92 +56:00:28.3: 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 02:27:15.92 +56:00:28.3: 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 31.3529* 02 27 15.92 +56 00 28.3 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 457460750572377984,2461191.8529,9.14,0.05,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 457460750572377984 20260531.3529 9.14CV 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 31.3529 2461191.8529 9.22 02:32:37.22 +56:00:39.6
136.78812 -4.11456 galactic Per Second-epoch detections are separated by 2.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457363443795236736 | 02:32:37.60 +56:00:41.0 (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 02:32:37.22 +56:00:39.6: 12.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:37.22 +56:00:39.6: 11.99 +/- 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 31.3529* 02 32 37.22 +56 00 39.6 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 457363443795236736,2461191.8529,9.22,0.05,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 457363443795236736 20260531.3529 9.22CV 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 31.3529 2461191.8529 9.46 01:40:01.01 +60:52:39.3
128.81048 -1.43849 galactic Cas Second-epoch detections are separated by 0.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J013956.73+605213.0 | 01:39:56.73 +60:52:13.0 (Gaia DR3) | SR (local) | 450.000000000000 (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 01:40:01.01 +60:52:39.3: 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 01:40:01.01 +60:52:39.3: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 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 31.3529* 01 40 01.01 +60 52 39.3 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 J013956.73+605213.0,2461191.8529,9.46,0.05,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 J013956.73+605213.0 20260531.3529 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 31.3529 2461191.8529 9.19 02:22:16.01 +56:22:42.1
135.30902 -4.29501 galactic Per Second-epoch detections are separated by 1.4" and 4.0 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 458278203113550720 | 02:22:15.95 +56:22:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.043+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:16.01 +56:22:42.1: 13.00 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:16.01 +56:22:42.1: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 31.3529* 02 22 16.01 +56 22 42.1 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 458278203113550720,2461191.8529,9.19,0.05,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
Gaia DR3 458278203113550720 20260531.3529 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 31.3529 2461191.8529 9.21 02:23:07.52 +56:41:45.7
135.31014 -3.95602 galactic Per Second-epoch detections are separated by 1.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7879+56.6943 | 02:23:07.31 +56:41:39.7 (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 02:23:07.52 +56:41:45.7: 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 02:23:07.52 +56:41:45.7: 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 31.3529* 02 23 07.52 +56 41 45.7 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
ATO J035.7879+56.6943,2461191.8529,9.21,0.05,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
ATO J035.7879+56.6943 20260531.3529 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 31.3529 2461191.8529 9.19 02:34:09.36 +56:41:02.1
136.72617 -3.41153 galactic Per Second-epoch detections are separated by 1.5" and 3.7 pix
The object was found in VSX 8" Gaia DR3 457775240955622912
Type: ROT
# Max. Min./Amp. JD0 Period
11.750 G 11.790 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 02:34:09.36 +56:41:02.1: 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 02:34:09.36 +56:41:02.1: 12.03 +/- 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 31.3529* 02 34 09.36 +56 41 02.1 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 457775240955622912,2461191.8529,9.19,0.05,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
Gaia DR3 457775240955622912 20260531.3529 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 31.3529 2461191.8529 9.24 02:31:19.74 +56:52:40.3
136.29353 -3.37991 galactic Per Second-epoch detections are separated by 2.8" and 4.0 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 J037.8317+56.8856 | 02:31:19.65 +56:52:39.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.120+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:19.74 +56:52:40.3: 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 02:31:19.74 +56:52:40.3: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 31.3529* 02 31 19.74 +56 52 40.3 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
ATO J037.8317+56.8856,2461191.8529,9.24,0.05,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
ATO J037.8317+56.8856 20260531.3529 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 31.3529 2461191.8529 9.24 02:31:43.43 +56:14:45.0
136.58290 -3.94473 galactic Per Second-epoch detections are separated by 2.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457382685248448384 | 02:31:43.75 +56:14:44.3 (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 02:31:43.43 +56:14:45.0: 12.37 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:43.43 +56:14:45.0: 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 31.3529* 02 31 43.43 +56 14 45.0 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 457382685248448384,2461191.8529,9.24,0.05,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 457382685248448384 20260531.3529 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 31.3529 2461191.8529 9.29 02:32:47.60 +57:14:18.6
136.34118 -2.97073 galactic Per Second-epoch detections are separated by 2.2" and 3.9 pix
The object was found in VSX24" ZTF J023246.55+571356.5
Type: RS
# Max. Min./Amp. JD0 Period
16.972 r Y 0.150 r 2458486.65480 4.402844100000
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 02:32:47.60 +57:14:18.6: 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 02:32:47.60 +57:14:18.6: 11.99 +/- 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 31.3529* 02 32 47.60 +57 14 18.6 9.3 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
ZTF J023246.55+571356.5,2461191.8529,9.29,0.05,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
ZTF J023246.55+571356.5 20260531.3529 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 31.3529 2461191.8529 9.18 02:34:34.57 +56:36:40.8
136.80766 -3.45610 galactic Per Second-epoch detections are separated by 1.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457762325995735040 | 02:34:34.87 +56:36:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2 2004AJ....128..463R G 174- 4
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:34.57 +56:36:40.8: 12.86 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:34.57 +56:36:40.8: 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 31.3529* 02 34 34.57 +56 36 40.8 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 457762325995735040,2461191.8529,9.18,0.05,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 457762325995735040 20260531.3529 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 31.3529 2461191.8529 9.29 02:30:33.43 +56:57:01.0
136.16850 -3.35228 galactic Per Second-epoch detections are separated by 2.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457978929787415936 | 02:30:33.42 +56:57:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.162+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:33.43 +56:57:01.0: 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 02:30:33.43 +56:57:01.0: 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 31.3529* 02 30 33.43 +56 57 01.0 9.3 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 457978929787415936,2461191.8529,9.29,0.05,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
Gaia DR3 457978929787415936 20260531.3529 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 31.3529 2461191.8529 9.16 02:25:42.16 +56:37:12.1
135.66922 -3.90248 galactic Per Second-epoch detections are separated by 1.1" and 4.0 pix
The object was found in VSX 2" 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 02:25:42.16 +56:37:12.1: 12.70 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:42.16 +56:37:12.1: 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 31.3529* 02 25 42.16 +56 37 12.1 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
ASASSN-V J022542.34+563711.6,2461191.8529,9.16,0.05,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
ASASSN-V J022542.34+563711.6 20260531.3529 9.16CV 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 31.3529 2461191.8529 9.22 02:30:34.92 +56:43:56.7
136.25323 -3.55309 galactic Per Second-epoch detections are separated by 2.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457589565231823360 | 02:30:35.06 +56:43:56.1 (Gaia DR3) | T | P | 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 02:30:34.92 +56:43:56.7: 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 02:30:34.92 +56:43:56.7: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 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 31.3529* 02 30 34.92 +56 43 56.7 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 457589565231823360,2461191.8529,9.22,0.05,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 457589565231823360 20260531.3529 9.22CV 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 31.3529 2461191.8529 9.25 02:21:32.88 +56:13:40.8
135.26686 -4.47046 galactic Per Second-epoch detections are separated by 2.2" and 4.2 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 J035.3809+56.2181 | 02:21:32.94 +56:13:40.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.082+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:32.88 +56:13:40.8: 10.40 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:32.88 +56:13:40.8: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 31.3529* 02 21 32.88 +56 13 40.8 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
ATO J035.3809+56.2181,2461191.8529,9.25,0.05,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
ATO J035.3809+56.2181 20260531.3529 9.25CV 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 31.3529 2461191.8529 9.28 02:33:38.50 +57:33:38.4
136.32338 -2.62937 galactic Per Second-epoch detections are separated by 6.6" and 4.4 pix
The object was found in VSX13" Gaia23cfy
Type: GCAS
# Max. Min./Amp. JD0 Period
11.620 G 12.010 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 02:33:38.50 +57:33:38.4: 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 02:33:38.50 +57:33:38.4: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 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 31.3529* 02 33 38.50 +57 33 38.4 9.3 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
Gaia23cfy,2461191.8529,9.28,0.05,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
Gaia23cfy 20260531.3529 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 31.3529 2461191.8529 9.43 02:37:15.56 +57:48:20.7
136.67309 -2.21493 galactic Cas Second-epoch detections are separated by 2.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458135743330088064 | 02:37:15.63 +57:48:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.713+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:15.56 +57:48:20.7: 11.83 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:15.56 +57:48:20.7: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 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 31.3529* 02 37 15.56 +57 48 20.7 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 458135743330088064,2461191.8529,9.43,0.05,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 458135743330088064 20260531.3529 9.43CV 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 31.3529 2461191.8529 9.34 02:33:30.70 +57:29:01.5
136.33683 -2.70709 galactic Per Second-epoch detections are separated by 4.3" and 3.6 pix
The object was found in VSX 3" Gaia23dql
Type: GCAS
# Max. Min./Amp. JD0 Period
11.590 G 11.980 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 02:33:30.70 +57:29:01.5: 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 02:33:30.70 +57:29:01.5: 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 31.3529* 02 33 30.70 +57 29 01.5 9.3 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
Gaia23dql,2461191.8529,9.34,0.05,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
Gaia23dql 20260531.3529 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 31.3529 2461191.8529 9.27 02:36:49.05 +57:24:45.7
136.77452 -2.59927 galactic Per Second-epoch detections are separated by 2.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.2264+57.4083 | 02:36:49.03 +57:24:43.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:49.05 +57:24:45.7: 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 02:36:49.05 +57:24:45.7: 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 31.3529* 02 36 49.05 +57 24 45.7 9.3 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 J039.2264+57.4083,2461191.8529,9.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.2264+57.4083 20260531.3529 9.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.30 02:32:30.78 +56:47:59.9
136.47318 -3.39072 galactic Per Second-epoch detections are separated by 1.1" and 4.0 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 J038.1231+56.8035 | 02:32:31.16 +56:48:02.0 (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 02:32:30.78 +56:47:59.9: 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 02:32:30.78 +56:47:59.9: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 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 31.3529* 02 32 30.78 +56 47 59.9 9.3 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 J038.1231+56.8035,2461191.8529,9.30,0.05,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 J038.1231+56.8035 20260531.3529 9.30CV 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 31.3529 2461191.8529 9.23 02:31:46.58 +55:52:30.0
136.73031 -4.28525 galactic Per Second-epoch detections are separated by 1.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457338876581619456 | 02:31:47.43 +55:52:29.5 (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 02:31:46.58 +55:52:30.0: 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 02:31:46.58 +55:52:30.0: 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 31.3529* 02 31 46.58 +55 52 30.0 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 457338876581619456,2461191.8529,9.23,0.05,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
Gaia DR3 457338876581619456 20260531.3529 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 31.3529 2461191.8529 9.46 02:36:54.41 +57:53:40.3
136.59480 -2.15199 galactic Cas Second-epoch detections are separated by 1.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458137225101548672 | 02:36:54.42 +57:53:41.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.270+/-0.040 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:54.41 +57:53:40.3: 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 02:36:54.41 +57:53:40.3: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 31.3529* 02 36 54.41 +57 53 40.3 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
Gaia DR3 458137225101548672,2461191.8529,9.46,0.05,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
Gaia DR3 458137225101548672 20260531.3529 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 31.3529 2461191.8529 9.26 02:21:27.45 +56:16:27.4
135.23915 -4.43127 galactic Per Second-epoch detections are separated by 3.1" and 4.3 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 458256693914103936 | 02:21:27.40 +56:16:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.681+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:27.45 +56:16:27.4: 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 02:21:27.45 +56:16:27.4: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 31.3529* 02 21 27.45 +56 16 27.4 9.3 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 458256693914103936,2461191.8529,9.26,0.05,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 458256693914103936 20260531.3529 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 31.3529 2461191.8529 9.19 02:35:12.35 +56:50:10.1
136.79980 -3.21540 galactic Per Second-epoch detections are separated by 1.9" and 4.2 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 J038.8034+56.8391 | 02:35:12.85 +56:50:10.3 (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 02:35:12.35 +56:50:10.1: 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 02:35:12.35 +56:50:10.1: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 31.3529* 02 35 12.35 +56 50 10.1 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
ATO J038.8034+56.8391,2461191.8529,9.19,0.05,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
ATO J038.8034+56.8391 20260531.3529 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 31.3529 2461191.8529 9.21 02:32:01.35 +56:51:17.4
136.39014 -3.36545 galactic Per Second-epoch detections are separated by 3.0" and 4.0 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 J038.0170+56.8475 | 02:32:01.27 +56:51:18.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:01.35 +56:51:17.4: 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 02:32:01.35 +56:51:17.4: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 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 31.3529* 02 32 01.35 +56 51 17.4 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
ATO J038.0170+56.8475,2461191.8529,9.21,0.05,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
ATO J038.0170+56.8475 20260531.3529 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 31.3529 2461191.8529 9.32 02:29:43.00 +56:05:10.4
136.38312 -4.19737 galactic Per Second-epoch detections are separated by 1.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457358770869699584 | 02:29:43.62 +56:05:12.5 (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 02:29:43.00 +56:05:10.4: 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 02:29:43.00 +56:05:10.4: 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 31.3529* 02 29 43.00 +56 05 10.4 9.3 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 457358770869699584,2461191.8529,9.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457358770869699584 20260531.3529 9.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.27 02:39:58.30 +58:20:59.8
136.78309 -1.57258 galactic Cas Second-epoch detections are separated by 1.6" and 3.6 pix
The object was found in VSX 6" ZTF J023959.02+582100.9
Type: BY
# Max. Min./Amp. JD0 Period
13.524 r Y 0.027 r 2458456.70030 12.161594600000
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 02:39:58.30 +58:20:59.8: 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 02:39:58.30 +58:20:59.8: 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 31.3529* 02 39 58.30 +58 20 59.8 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
ZTF J023959.02+582100.9,2461191.8529,9.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023959.02+582100.9 20260531.3529 9.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.29 02:33:30.84 +56:43:01.0
136.63197 -3.41499 galactic Per Second-epoch detections are separated by 1.2" and 4.0 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 J038.3826+56.7191 | 02:33:31.00 +56:43:01.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.239+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:30.84 +56:43:01.0: 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 02:33:30.84 +56:43:01.0: 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 31.3529* 02 33 30.84 +56 43 01.0 9.3 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 J038.3826+56.7191,2461191.8529,9.29,0.05,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
ATO J038.3826+56.7191 20260531.3529 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 31.3529 2461191.8529 9.21 02:35:15.88 +56:26:19.4
136.96257 -3.57817 galactic Per Second-epoch detections are separated by 2.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457710477150655104 | 02:35:16.32 +56:26:21.4 (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 02:35:15.88 +56:26:19.4: 11.20 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:15.88 +56:26:19.4: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 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 31.3529* 02 35 15.88 +56 26 19.4 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 457710477150655104,2461191.8529,9.21,0.05,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
Gaia DR3 457710477150655104 20260531.3529 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 31.3529 2461191.8529 9.21 02:27:22.97 +56:19:27.7
135.99283 -4.09490 galactic Per Second-epoch detections are separated by 1.1" and 3.8 pix
The object was found in VSX 2" 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 +56:19:27.7: 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 02:27:22.97 +56:19:27.7: 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 31.3529* 02 27 22.97 +56 19 27.7 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 457562214879587968,2461191.8529,9.21,0.05,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
Gaia DR3 457562214879587968 20260531.3529 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 31.3529 2461191.8529 9.49 02:30:05.86 +57:18:33.7
135.97649 -3.04233 galactic Per Second-epoch detections are separated by 0.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.5330+57.3072 | 02:30:05.94 +57:18:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: em 1950ApJ...112...72M AS 61 J-Ks=0.547+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:05.86 +57:18:33.7: 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 02:30:05.86 +57:18:33.7: 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 31.3529* 02 30 05.86 +57 18 33.7 9.5 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 J037.5330+57.3072,2461191.8529,9.49,0.05,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 J037.5330+57.3072 20260531.3529 9.49CV 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 31.3529 2461191.8529 9.37 02:37:01.21 +57:51:23.9
136.62365 -2.18082 galactic Cas Second-epoch detections are separated by 0.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458136847144779648 | 02:37:01.18 +57:51:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.154+/-0.037 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:01.21 +57:51:23.9: 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 02:37:01.21 +57:51:23.9: 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 31.3529* 02 37 01.21 +57 51 23.9 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 458136847144779648,2461191.8529,9.37,0.05,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 458136847144779648 20260531.3529 9.37CV 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 31.3529 2461191.8529 9.28 02:34:37.56 +56:32:35.4
136.84049 -3.51626 galactic Per Second-epoch detections are separated by 3.9" and 4.0 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 J038.6528+56.5460 | 02:34:37.95 +56:32:37.5 (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 02:34:37.56 +56:32:35.4: 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 02:34:37.56 +56:32:35.4: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 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 31.3529* 02 34 37.56 +56 32 35.4 9.3 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 J038.6528+56.5460,2461191.8529,9.28,0.05,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
ATO J038.6528+56.5460 20260531.3529 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 31.3529 2461191.8529 9.29 02:34:22.33 +56:20:27.4
136.88664 -3.71627 galactic Per Second-epoch detections are separated by 2.5" and 4.0 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 J038.5944+56.3413 | 02:34:22.68 +56:20:28.8 (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 02:34:22.33 +56:20:27.4: 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 02:34:22.33 +56:20:27.4: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 31.3529* 02 34 22.33 +56 20 27.4 9.3 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 J038.5944+56.3413,2461191.8529,9.29,0.05,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
ATO J038.5944+56.3413 20260531.3529 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 31.3529 2461191.8529 9.42 02:28:01.24 +56:23:31.7
136.05060 -3.99963 galactic Per Second-epoch detections are separated by 2.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.9932+56.3960 | 02:28:00.52 +56:23:27.6 (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 02:28:01.24 +56:23:31.7: 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 02:28:01.24 +56:23:31.7: 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 31.3529* 02 28 01.24 +56 23 31.7 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
ATO J036.9932+56.3960,2461191.8529,9.42,0.05,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 J036.9932+56.3960 20260531.3529 9.42CV 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 31.3529 2461191.8529 9.24 02:36:42.69 +57:08:11.5
136.87062 -2.85862 galactic Per Second-epoch detections are separated by 0.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457800942037764352 | 02:36:42.74 +57:08:10.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.148+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:42.69 +57:08:11.5: 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 02:36:42.69 +57:08:11.5: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 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 31.3529* 02 36 42.69 +57 08 11.5 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 457800942037764352,2461191.8529,9.24,0.05,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 457800942037764352 20260531.3529 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 31.3529 2461191.8529 9.22 02:33:57.90 +56:36:42.0
136.72985 -3.48831 galactic Per Second-epoch detections are separated by 2.1" and 4.0 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 457757412554149760 | 02:33:58.20 +56:36:41.8 (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 02:33:57.90 +56:36:42.0: 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 02:33:57.90 +56:36:42.0: 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 31.3529* 02 33 57.90 +56 36 42.0 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 457757412554149760,2461191.8529,9.22,0.05,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 457757412554149760 20260531.3529 9.22CV 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 31.3529 2461191.8529 9.33 02:20:11.66 +56:22:21.1
135.04050 -4.39828 galactic Per Second-epoch detections are separated by 1.2" and 3.7 pix
The object was found in VSX11" ZTF J022010.56+562228.1
Type: EW
# Max. Min./Amp. JD0 Period
17.880 r Y 0.223 r 2458303.96760 0.419228000000
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 02:20:11.66 +56:22:21.1: 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 02:20:11.66 +56:22:21.1: 11.99 +/- 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 31.3529* 02 20 11.66 +56 22 21.1 9.3 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
ZTF J022010.56+562228.1,2461191.8529,9.33,0.05,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
ZTF J022010.56+562228.1 20260531.3529 9.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.34 02:33:11.61 +57:36:40.3
136.24846 -2.60573 galactic Per Second-epoch detections are separated by 1.5" and 4.0 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 458028029853733248 | 02:33:11.43 +57:36:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.505+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:11.61 +57:36:40.3: 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 02:33:11.61 +57:36:40.3: 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 31.3529* 02 33 11.61 +57 36 40.3 9.3 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 458028029853733248,2461191.8529,9.34,0.05,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
Gaia DR3 458028029853733248 20260531.3529 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 31.3529 2461191.8529 9.38 02:21:23.02 +56:39:00.5
135.10084 -4.08148 galactic Per Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458297582003381120 | 02:21:23.03 +56:39:00.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:23.02 +56:39:00.5: 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 02:21:23.02 +56:39:00.5: 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 31.3529* 02 21 23.02 +56 39 00.5 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
Gaia DR3 458297582003381120,2461191.8529,9.38,0.05,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
Gaia DR3 458297582003381120 20260531.3529 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 31.3529 2461191.8529 9.29 02:35:22.14 +56:48:52.6
136.82879 -3.22651 galactic Per Second-epoch detections are separated by 3.5" and 4.3 pix
The object was found in VSX23" Gaia DR3 457788782994109440
Type: RS
# Max. Min./Amp. JD0 Period
15.830 G 15.960 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 02:35:22.14 +56:48:52.6: 12.29 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:22.14 +56:48:52.6: 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 31.3529* 02 35 22.14 +56 48 52.6 9.3 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 457788782994109440,2461191.8529,9.29,0.05,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
Gaia DR3 457788782994109440 20260531.3529 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 31.3529 2461191.8529 9.42 02:24:12.37 +56:49:24.7
135.40460 -3.78481 galactic Per Second-epoch detections are separated by 1.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.0445+56.8257 | 02:24:12.46 +56:49:26.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.242+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:12.37 +56:49:24.7: 12.65 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:12.37 +56:49:24.7: 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 31.3529* 02 24 12.37 +56 49 24.7 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
ATO J036.0445+56.8257,2461191.8529,9.42,0.05,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 J036.0445+56.8257 20260531.3529 9.42CV 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 31.3529 2461191.8529 9.49 02:32:55.55 +57:08:54.8
136.39217 -3.04702 galactic Per Second-epoch detections are separated by 0.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457999648710144000 | 02:32:55.50 +57:08:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.889+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:55.55 +57:08:54.8: 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 02:32:55.55 +57:08:54.8: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 31.3529* 02 32 55.55 +57 08 54.8 9.5 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 457999648710144000,2461191.8529,9.49,0.05,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 457999648710144000 20260531.3529 9.49CV 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 31.3529 2461191.8529 9.28 02:27:53.50 +57:06:30.2
135.77243 -3.33912 galactic Per Second-epoch detections are separated by 2.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457670276258952448 | 02:27:53.69 +57:06:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965LS....C05....0H LS V +56 47 J-Ks=0.125+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:53.50 +57:06:30.2: 12.58 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:53.50 +57:06:30.2: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 31.3529* 02 27 53.50 +57 06 30.2 9.3 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 457670276258952448,2461191.8529,9.28,0.05,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
Gaia DR3 457670276258952448 20260531.3529 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 31.3529 2461191.8529 9.33 02:37:38.82 +57:43:26.3
136.75309 -2.26942 galactic Cas Second-epoch detections are separated by 2.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.4038+57.7234 | 02:37:38.88 +57:43:27.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.269+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:38.82 +57:43:26.3: 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 02:37:38.82 +57:43:26.3: 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 31.3529* 02 37 38.82 +57 43 26.3 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
ATO J039.4038+57.7234,2461191.8529,9.33,0.05,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
ATO J039.4038+57.7234 20260531.3529 9.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.33 02:34:43.58 +56:51:49.8
136.72852 -3.21539 galactic Per Second-epoch detections are separated by 3.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457801736615450240 | 02:34:44.20 +56:51:49.0 (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 02:34:43.58 +56:51:49.8: 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 02:34:43.58 +56:51:49.8: 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 31.3529* 02 34 43.58 +56 51 49.8 9.3 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 457801736615450240,2461191.8529,9.33,0.05,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 457801736615450240 20260531.3529 9.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.36 02:36:55.85 +57:38:50.5
136.69560 -2.37773 galactic Cas Second-epoch detections are separated by 0.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.2323+57.6467 | 02:36:55.77 +57:38:48.4 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.185+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:55.85 +57:38:50.5: 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 02:36:55.85 +57:38:50.5: 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 31.3529* 02 36 55.85 +57 38 50.5 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
ATO J039.2323+57.6467,2461191.8529,9.36,0.05,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
ATO J039.2323+57.6467 20260531.3529 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 31.3529 2461191.8529 9.19 02:33:06.29 +56:00:32.4
136.85162 -4.09053 galactic Per Second-epoch detections are separated by 2.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457363993551045760 | 02:33:06.84 +56:00:37.2 (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 02:33:06.29 +56:00:32.4: 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 02:33:06.29 +56:00:32.4: 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 31.3529* 02 33 06.29 +56 00 32.4 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 457363993551045760,2461191.8529,9.19,0.05,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
Gaia DR3 457363993551045760 20260531.3529 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 31.3529 2461191.8529 9.39 02:33:08.16 +57:28:10.9
136.29553 -2.73942 galactic Per Second-epoch detections are separated by 0.5" and 3.8 pix
The object was found in VSX 0" V0975 Per
Type: EB
# Max. Min./Amp. JD0 Period
11.890 V 11.990 V 2454774.38420 0.471920000000
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 02:33:08.16 +57:28:10.9: 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 02:33:08.16 +57:28:10.9: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 31.3529* 02 33 08.16 +57 28 10.9 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
V0975 Per,2461191.8529,9.39,0.05,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
V0975 Per 20260531.3529 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 31.3529 2461191.8529 9.32 02:33:23.59 +57:33:31.5
136.29332 -2.64393 galactic Per Second-epoch detections are separated by 4.3" and 4.3 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 458023253850132608 | 02:33:23.51 +57:33:31.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.120+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:23.59 +57:33:31.5: 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 02:33:23.59 +57:33:31.5: 11.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 31.3529* 02 33 23.59 +57 33 31.5 9.3 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 458023253850132608,2461191.8529,9.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458023253850132608 20260531.3529 9.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.38 02:27:27.08 +56:31:12.3
135.93050 -3.90908 galactic Per Second-epoch detections are separated by 4.5" and 4.6 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 457617327901248128 | 02:27:27.12 +56:31:09.0 (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 02:27:27.08 +56:31:12.3: 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 02:27:27.08 +56:31:12.3: 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 31.3529* 02 27 27.08 +56 31 12.3 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
Gaia DR3 457617327901248128,2461191.8529,9.38,0.05,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
Gaia DR3 457617327901248128 20260531.3529 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 31.3529 2461191.8529 9.37 02:25:52.68 +56:47:30.2
135.63033 -3.73350 galactic Per Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457636397555905024 | 02:25:52.85 +56:47:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.107+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:52.68 +56:47:30.2: 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 02:25:52.68 +56:47:30.2: 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 31.3529* 02 25 52.68 +56 47 30.2 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
Gaia DR3 457636397555905024,2461191.8529,9.37,0.05,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 457636397555905024 20260531.3529 9.37CV 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 31.3529 2461191.8529 9.36 02:25:40.02 +56:29:21.1
135.71138 -4.02646 galactic Per Second-epoch detections are separated by 0.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457614098080789120 | 02:25:39.98 +56:29:20.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.784+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:40.02 +56:29:21.1: 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 02:25:40.02 +56:29:21.1: 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 31.3529* 02 25 40.02 +56 29 21.1 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
Large-amplitude variable Gaia DR2 457614098080789120,2461191.8529,9.36,0.05,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
Large-amplitude variable Gaia DR2 457614098080789120 20260531.3529 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 31.3529 2461191.8529 9.41 02:22:21.44 +56:34:17.9
135.25399 -4.10927 galactic Per Second-epoch detections are separated by 0.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.6108+56.5718 | 02:22:21.39 +56:34:19.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.149+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:21.44 +56:34:17.9: 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 02:22:21.44 +56:34:17.9: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 31.3529* 02 22 21.44 +56 34 17.9 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
ATO J035.6108+56.5718,2461191.8529,9.41,0.05,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
ATO J035.6108+56.5718 20260531.3529 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 31.3529 2461191.8529 9.42 02:24:46.71 +56:38:57.2
135.53976 -3.92029 galactic Per Second-epoch detections are separated by 3.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457630895694121216 | 02:24:46.83 +56:38:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.327+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:46.71 +56:38:57.2: 11.48 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:46.71 +56:38:57.2: 12.12 +/- 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 31.3529* 02 24 46.71 +56 38 57.2 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
Gaia DR3 457630895694121216,2461191.8529,9.42,0.05,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 457630895694121216 20260531.3529 9.42CV 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 31.3529 2461191.8529 9.46 02:21:16.35 +56:23:42.9
135.17357 -4.32631 galactic Per Second-epoch detections are separated by 3.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458258411900977280 | 02:21:16.26 +56:23:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.037+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:16.35 +56:23:42.9: 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 02:21:16.35 +56:23:42.9: 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 31.3529* 02 21 16.35 +56 23 42.9 9.5 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 458258411900977280,2461191.8529,9.46,0.05,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
Gaia DR3 458258411900977280 20260531.3529 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 31.3529 2461191.8529 9.28 02:24:53.85 +56:08:46.7
135.73354 -4.38488 galactic Per Second-epoch detections are separated by 2.5" and 4.2 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 J036.2276+56.1492 | 02:24:53.87 +56:08:46.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.132+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:53.85 +56:08:46.7: 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 02:24:53.85 +56:08:46.7: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 31.3529* 02 24 53.85 +56 08 46.7 9.3 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 J036.2276+56.1492,2461191.8529,9.28,0.05,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
ATO J036.2276+56.1492 20260531.3529 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 31.3529 2461191.8529 9.32 02:28:10.62 +56:06:42.3
136.17355 -4.25271 galactic Per Second-epoch detections are separated by 5.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457543798059942784 | 02:28:10.98 +56:06:41.9 (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 02:28:10.62 +56:06:42.3: 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 02:28:10.62 +56:06:42.3: 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 31.3529* 02 28 10.62 +56 06 42.3 9.3 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 457543798059942784,2461191.8529,9.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457543798059942784 20260531.3529 9.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.40 02:35:35.04 +57:33:01.8
136.56771 -2.53775 galactic Cas Second-epoch detections are separated by 1.8" and 4.0 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 J038.8988+57.5514 | 02:35:35.71 +57:33:05.1 (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 02:35:35.04 +57:33:01.8: 11.80 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:35.04 +57:33:01.8: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 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 31.3529* 02 35 35.04 +57 33 01.8 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
ATO J038.8988+57.5514,2461191.8529,9.40,0.05,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
ATO J038.8988+57.5514 20260531.3529 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 31.3529 2461191.8529 9.40 02:29:33.78 +56:09:10.9
136.33834 -4.14326 galactic Per Second-epoch detections are separated by 1.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457547199673991168 | 02:29:34.17 +56:09:08.1 (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 02:29:33.78 +56:09:10.9: 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 02:29:33.78 +56:09:10.9: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 31.3529* 02 29 33.78 +56 09 10.9 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
Gaia DR3 457547199673991168,2461191.8529,9.40,0.05,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
Gaia DR3 457547199673991168 20260531.3529 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 31.3529 2461191.8529 9.43 02:34:04.23 +57:32:43.7
136.38238 -2.62124 galactic Per Second-epoch detections are separated by 3.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5396+57.5452 | 02:34:04.33 +57:32:39.5 (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 02:34:04.23 +57:32:43.7: 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 02:34:04.23 +57:32:43.7: 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 31.3529* 02 34 04.23 +57 32 43.7 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
ATO J038.5396+57.5452,2461191.8529,9.43,0.05,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 J038.5396+57.5452 20260531.3529 9.43CV 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 31.3529 2461191.8529 9.36 02:30:51.32 +57:16:48.9
136.08245 -3.03113 galactic Per Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.7170+57.2833 | 02:30:51.33 +57:16:48.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.235+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:51.32 +57:16:48.9: 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 02:30:51.32 +57:16:48.9: 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 31.3529* 02 30 51.32 +57 16 48.9 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
ATO J037.7170+57.2833,2461191.8529,9.36,0.05,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
ATO J037.7170+57.2833 20260531.3529 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 31.3529 2461191.8529 9.42 02:21:13.42 +56:28:43.4
135.13867 -4.25014 galactic Per Second-epoch detections are separated by 1.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458294146029662208 | 02:21:13.36 +56:28:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.313+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:13.42 +56:28:43.4: 12.93 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:13.42 +56:28:43.4: 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 31.3529* 02 21 13.42 +56 28 43.4 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
Gaia DR3 458294146029662208,2461191.8529,9.42,0.05,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 458294146029662208 20260531.3529 9.42CV 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 31.3529 2461191.8529 9.34 02:29:38.91 +56:20:56.3
136.27660 -3.95687 galactic Per Second-epoch detections are separated by 4.0" and 4.4 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 J037.4149+56.3474 | 02:29:39.41 +56:21:00.7 (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 02:29:38.91 +56:20:56.3: 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 02:29:38.91 +56:20:56.3: 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 31.3529* 02 29 38.91 +56 20 56.3 9.3 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 J037.4149+56.3474,2461191.8529,9.34,0.05,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
ATO J037.4149+56.3474 20260531.3529 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 31.3529 2461191.8529 9.34 02:32:49.88 +56:14:34.7
136.72663 -3.88892 galactic Per Second-epoch detections are separated by 0.4" and 3.9 pix
The object was found in VSX10" Gaia DR3 457375366624349696
Type: ROT
# Max. Min./Amp. JD0 Period
16.490 G 16.530 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 02:32:49.88 +56:14:34.7: 13.05 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:49.88 +56:14:34.7: 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 31.3529* 02 32 49.88 +56 14 34.7 9.3 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 457375366624349696,2461191.8529,9.34,0.05,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
Gaia DR3 457375366624349696 20260531.3529 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 31.3529 2461191.8529 9.71 01:25:31.68 +57:37:40.0
127.50001 -4.94130 galactic Cas Second-epoch detections are separated by 0.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.3669+57.6328 | 01:25:32.01 +57:37:37.8 (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 01:25:31.68 +57:37:40.0: 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 01:25:31.68 +57:37:40.0: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 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 31.3529* 01 25 31.68 +57 37 40.0 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
ATO J021.3669+57.6328,2461191.8529,9.71,0.05,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
ATO J021.3669+57.6328 20260531.3529 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 31.3529 2461191.8529 9.62 02:35:41.88 +57:31:41.5
136.59054 -2.55229 galactic Per Second-epoch detections are separated by 3.1" and 3.2 pix
The object was found in VSX 1" Gaia DR3 458102998499428480
Type: VAR
# Max. Min./Amp. JD0 Period
12.230 G 12.260 G 0.062549500000 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 02:35:41.88 +57:31:41.5: 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 02:35:41.88 +57:31:41.5: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.3529* 02 35 41.88 +57 31 41.5 9.6 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 458102998499428480,2461191.8529,9.62,0.05,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 458102998499428480 20260531.3529 9.62CV 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 31.3529 2461191.8529 9.55 02:30:42.09 +57:22:37.0
136.02693 -2.94924 galactic Per Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458042289146154112 | 02:30:42.04 +57:22:35.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.410+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:42.09 +57:22:37.0: 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 02:30:42.09 +57:22:37.0: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 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 31.3529* 02 30 42.09 +57 22 37.0 9.6 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 458042289146154112,2461191.8529,9.55,0.05,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 458042289146154112 20260531.3529 9.55CV 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 31.3529 2461191.8529 9.50 02:31:45.76 +57:14:33.8
136.21041 -3.01975 galactic Per Second-epoch detections are separated by 5.1" and 3.3 pix
The object was found in VSX 4" ASASSN-V J023146.20+571431.6
Type: L
# Max. Min./Amp. JD0 Period
13.250 V 13.610 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 02:31:45.76 +57:14:33.8: 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 02:31:45.76 +57:14:33.8: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 31.3529* 02 31 45.76 +57 14 33.8 9.5 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
ASASSN-V J023146.20+571431.6,2461191.8529,9.50,0.05,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
ASASSN-V J023146.20+571431.6 20260531.3529 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 31.3529 2461191.8529 9.37 02:34:19.68 +57:08:34.6
136.57013 -2.97911 galactic Per Second-epoch detections are separated by 2.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457809635051571200 | 02:34:20.02 +57:08:33.6 (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 02:34:19.68 +57:08:34.6: 12.02 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:19.68 +57:08:34.6: 12.26 +/- 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 31.3529* 02 34 19.68 +57 08 34.6 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
Gaia DR3 457809635051571200,2461191.8529,9.37,0.05,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 457809635051571200 20260531.3529 9.37CV 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 31.3529 2461191.8529 9.54 02:37:47.00 +58:07:12.4
136.61180 -1.89886 galactic Cas Second-epoch detections are separated by 1.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.4455+58.1200 | 02:37:46.94 +58:07:12.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:47.00 +58:07:12.4: 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 02:37:47.00 +58:07:12.4: 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 31.3529* 02 37 47.00 +58 07 12.4 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
ATO J039.4455+58.1200,2461191.8529,9.54,0.05,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 J039.4455+58.1200 20260531.3529 9.54CV 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 31.3529 2461191.8529 9.46 02:29:29.31 +57:10:38.0
135.94893 -3.19560 galactic Per Second-epoch detections are separated by 5.6" and 4.5 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 J037.3768+57.1759 | 02:29:29.15 +57:10:37.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.226+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:29.31 +57:10:38.0: 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 02:29:29.31 +57:10:38.0: 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 31.3529* 02 29 29.31 +57 10 38.0 9.5 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 J037.3768+57.1759,2461191.8529,9.46,0.05,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
ATO J037.3768+57.1759 20260531.3529 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 31.3529 2461191.8529 9.49 02:33:27.53 +57:14:42.7
136.42190 -2.93011 galactic Per Second-epoch detections are separated by 3.1" and 4.0 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 458001847733355264 | 02:33:27.56 +57:14:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:27.53 +57:14:42.7: 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 02:33:27.53 +57:14:42.7: 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 31.3529* 02 33 27.53 +57 14 42.7 9.5 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 458001847733355264,2461191.8529,9.49,0.05,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 458001847733355264 20260531.3529 9.49CV 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 31.3529 2461191.8529 9.47 02:39:23.81 +58:09:08.6
136.79398 -1.78383 galactic Cas Second-epoch detections are separated by 2.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.8494+58.1525 | 02:39:23.88 +58:09:09.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 78 J-Ks=0.217+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:39:23.81 +58:09:08.6: 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 02:39:23.81 +58:09:08.6: 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 31.3529* 02 39 23.81 +58 09 08.6 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 J039.8494+58.1525,2461191.8529,9.47,0.05,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
ATO J039.8494+58.1525 20260531.3529 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 31.3529 2461191.8529 9.51 02:25:53.36 +56:14:37.1
135.82811 -4.24484 galactic Per Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.4750+56.2475 | 02:25:53.37 +56:14:35.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.146+/-0.044 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:53.36 +56:14:37.1: 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 02:25:53.36 +56:14:37.1: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 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 31.3529* 02 25 53.36 +56 14 37.1 9.5 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 J036.4750+56.2475,2461191.8529,9.51,0.05,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
ATO J036.4750+56.2475 20260531.3529 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 31.3529 2461191.8529 9.41 02:31:12.55 +56:27:35.9
136.43579 -3.77328 galactic Per Second-epoch detections are separated by 3.6" and 3.3 pix
The object was found in VSX18" Gaia DR3 457393920882782336
Type: ROT
# Max. Min./Amp. JD0 Period
15.310 G 15.340 G 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 02:31:12.55 +56:27:35.9: 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 02:31:12.55 +56:27:35.9: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 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 31.3529* 02 31 12.55 +56 27 35.9 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
Gaia DR3 457393920882782336,2461191.8529,9.41,0.05,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
Gaia DR3 457393920882782336 20260531.3529 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 31.3529 2461191.8529 9.46 02:27:22.07 +56:31:21.0
135.91886 -3.91100 galactic Per Second-epoch detections are separated by 1.0" and 3.7 pix
The object was found in VSX22" ZTF J022719.47+563119.0
Type: HADS
# Max. Min./Amp. JD0 Period
18.002 r Y 0.199 r 2458428.78930 0.077707800000
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 02:27:22.07 +56:31:21.0: 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 02:27:22.07 +56:31:21.0: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 31.3529* 02 27 22.07 +56 31 21.0 9.5 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
ZTF J022719.47+563119.0,2461191.8529,9.46,0.05,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
ZTF J022719.47+563119.0 20260531.3529 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 31.3529 2461191.8529 9.51 02:25:52.25 +57:02:03.7
135.54258 -3.50721 galactic Per Second-epoch detections are separated by 1.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457666634126204032 | 02:25:52.40 +57:02:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.758+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:52.25 +57:02:03.7: 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 02:25:52.25 +57:02:03.7: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 31.3529* 02 25 52.25 +57 02 03.7 9.5 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 457666634126204032,2461191.8529,9.51,0.05,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
Gaia DR3 457666634126204032 20260531.3529 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 31.3529 2461191.8529 9.48 02:29:04.86 +57:22:34.6
135.82410 -3.03092 galactic Per Second-epoch detections are separated by 1.8" and 4.0 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 458050569843119360 | 02:29:04.83 +57:22:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.228+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:04.86 +57:22:34.6: 11.94 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:04.86 +57:22:34.6: 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 31.3529* 02 29 04.86 +57 22 34.6 9.5 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 458050569843119360,2461191.8529,9.48,0.05,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
Gaia DR3 458050569843119360 20260531.3529 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 31.3529 2461191.8529 9.59 02:34:06.59 +56:06:19.6
136.94424 -3.94754 galactic Per Second-epoch detections are separated by 4.8" and 4.7 pix
The object was found in ASASSN-V 4" ASASSN-V J023406.97+560618.0
Type: EA
MeanMag 12.45 m Amp. 1.03 m Period 0.2057389 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 02:34:06.59 +56:06:19.6: 11.28 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:06.59 +56:06:19.6: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 31.3529* 02 34 06.59 +56 06 19.6 9.6 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
VARIABLE_NAME,2461191.8529,9.59,0.05,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
VARIABLE_NAME 20260531.3529 9.59CV 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 31.3529 2461191.8529 9.43 02:25:56.52 +56:32:32.5
135.72787 -3.96325 galactic Per Second-epoch detections are separated by 1.6" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457615850432513152 | 02:25:56.55 +56:32:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:56.52 +56:32:32.5: 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 02:25:56.52 +56:32:32.5: 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 31.3529* 02 25 56.52 +56 32 32.5 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
Gaia DR3 457615850432513152,2461191.8529,9.43,0.05,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 457615850432513152 20260531.3529 9.43CV 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 31.3529 2461191.8529 9.46 02:21:19.11 +56:38:13.7
135.09684 -4.09676 galactic Per Second-epoch detections are separated by 0.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.3292+56.6370 | 02:21:19.02 +56:38:13.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.798+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:19.11 +56:38:13.7: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:19.11 +56:38:13.7: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 31.3529* 02 21 19.11 +56 38 13.7 9.5 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 J035.3292+56.6370,2461191.8529,9.46,0.05,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
ATO J035.3292+56.6370 20260531.3529 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 31.3529 2461191.8529 9.38 02:39:21.43 +58:07:09.6
136.80255 -1.81619 galactic Cas Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 463964220109550080 | 02:39:21.53 +58:07:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.935+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:39:21.43 +58:07:09.6: 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 02:39:21.43 +58:07:09.6: 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 31.3529* 02 39 21.43 +58 07 09.6 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
Gaia DR3 463964220109550080,2461191.8529,9.38,0.05,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
Gaia DR3 463964220109550080 20260531.3529 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 31.3529 2461191.8529 9.64 02:28:31.02 +56:40:25.2
136.01122 -3.71258 galactic Per Second-epoch detections are separated by 2.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457596505898864384 | 02:28:31.29 +56:40:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M7 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:31.02 +56:40:25.2: 13.22 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:31.02 +56:40:25.2: 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 31.3529* 02 28 31.02 +56 40 25.2 9.6 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 457596505898864384,2461191.8529,9.64,0.05,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 457596505898864384 20260531.3529 9.64CV 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 31.3529 2461191.8529 9.51 02:23:08.48 +56:55:24.7
135.23298 -3.74193 galactic Per Second-epoch detections are separated by 1.7" and 3.7 pix
The object was found in VSX 0" Gaia DR3 458400313313975808
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.940 G 11.970 G 0.081444700000 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 02:23:08.48 +56:55:24.7: 12.37 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:08.48 +56:55:24.7: 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 31.3529* 02 23 08.48 +56 55 24.7 9.5 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 458400313313975808,2461191.8529,9.51,0.05,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
Gaia DR3 458400313313975808 20260531.3529 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 31.3529 2461191.8529 9.56 02:38:14.36 +57:58:52.1
136.72267 -2.00218 galactic Cas Second-epoch detections are separated by 1.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457956870833294720 | 02:38:14.37 +57:58:51.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.258+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:14.36 +57:58:52.1: 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 02:38:14.36 +57:58:52.1: 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 31.3529* 02 38 14.36 +57 58 52.1 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
Gaia DR3 457956870833294720,2461191.8529,9.56,0.05,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 457956870833294720 20260531.3529 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 31.3529 2461191.8529 9.49 02:31:54.47 +55:50:24.1
136.76071 -4.31063 galactic Per Second-epoch detections are separated by 1.3" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457338567344058624 | 02:31:54.97 +55:50:23.7 (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 02:31:54.47 +55:50:24.1: 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 02:31:54.47 +55:50:24.1: 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 31.3529* 02 31 54.47 +55 50 24.1 9.5 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 457338567344058624,2461191.8529,9.49,0.05,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 457338567344058624 20260531.3529 9.49CV 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 31.3529 2461191.8529 9.43 02:34:32.89 +57:07:24.9
136.60522 -2.98540 galactic Per Second-epoch detections are separated by 1.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457809398836927872 | 02:34:33.29 +57:07:22.6 (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 02:34:32.89 +57:07:24.9: 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 02:34:32.89 +57:07:24.9: 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 31.3529* 02 34 32.89 +57 07 24.9 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
Gaia DR3 457809398836927872,2461191.8529,9.43,0.05,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 457809398836927872 20260531.3529 9.43CV 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 31.3529 2461191.8529 9.52 02:21:52.35 +56:32:44.4
135.20006 -4.15663 galactic Per Second-epoch detections are separated by 2.5" and 4.2 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 458284555357304704 | 02:21:52.39 +56:32:45.0 (Gaia DR3) | T | P | 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 02:21:52.35 +56:32:44.4: 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 02:21:52.35 +56:32:44.4: 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 31.3529* 02 21 52.35 +56 32 44.4 9.5 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 458284555357304704,2461191.8529,9.52,0.05,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 458284555357304704 20260531.3529 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 31.3529 2461191.8529 9.38 02:26:14.36 +56:12:10.7
135.88826 -4.26539 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457467004044691712 | 02:26:14.28 +56:12:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.140+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:14.36 +56:12:10.7: 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 02:26:14.36 +56:12:10.7: 12.03 +/- 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 31.3529* 02 26 14.36 +56 12 10.7 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
Gaia DR3 457467004044691712,2461191.8529,9.38,0.05,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
Gaia DR3 457467004044691712 20260531.3529 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 31.3529 2461191.8529 9.49 02:34:18.24 +57:49:31.9
136.30295 -2.35086 galactic Per Second-epoch detections are separated by 1.1" and 3.8 pix
The object was found in VSX22" Gaia DR3 458124885654116224
Type: ROT
# Max. Min./Amp. JD0 Period
18.880 G 19.000 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 02:34:18.24 +57:49:31.9: 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 02:34:18.24 +57:49:31.9: 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 31.3529* 02 34 18.24 +57 49 31.9 9.5 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 458124885654116224,2461191.8529,9.49,0.05,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 458124885654116224 20260531.3529 9.49CV 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 31.3529 2461191.8529 9.52 02:29:41.72 +56:37:30.4
136.18002 -3.69801 galactic Per Second-epoch detections are separated by 1.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457593379162918784 | 02:29:41.70 +56:37:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.191+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:41.72 +56:37:30.4: 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 02:29:41.72 +56:37:30.4: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 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 31.3529* 02 29 41.72 +56 37 30.4 9.5 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 457593379162918784,2461191.8529,9.52,0.05,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 457593379162918784 20260531.3529 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 31.3529 2461191.8529 9.60 02:30:58.42 +57:16:18.4
136.10048 -3.03299 galactic Per Second-epoch detections are separated by 0.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457992639322524672 | 02:30:58.40 +57:16:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.205+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:58.42 +57:16:18.4: 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 02:30:58.42 +57:16:18.4: 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 31.3529* 02 30 58.42 +57 16 18.4 9.6 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 457992639322524672,2461191.8529,9.60,0.05,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
Gaia DR3 457992639322524672 20260531.3529 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 31.3529 2461191.8529 9.59 02:36:12.12 +57:41:55.7
136.58568 -2.36888 galactic Cas Second-epoch detections are separated by 2.4" and 3.3 pix
The object was found in VSX 2" Gaia DR3 458111038678203904
Type: ROT
# Max. Min./Amp. JD0 Period
12.370 G 12.390 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 02:36:12.12 +57:41:55.7: 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 02:36:12.12 +57:41:55.7: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 31.3529* 02 36 12.12 +57 41 55.7 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 458111038678203904,2461191.8529,9.59,0.05,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 458111038678203904 20260531.3529 9.59CV 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 31.3529 2461191.8529 9.55 02:26:01.05 +56:28:14.9
135.76328 -4.02635 galactic Per Second-epoch detections are separated by 6.4" and 4.1 pix
The object was found in VSX 3" Gaia DR3 457613342171654272
Type: VAR
# Max. Min./Amp. JD0 Period
12.120 G 12.140 G 0.249219000000 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 02:26:01.05 +56:28:14.9: 12.66 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:01.05 +56:28:14.9: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 31.3529* 02 26 01.05 +56 28 14.9 9.6 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 457613342171654272,2461191.8529,9.55,0.05,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 457613342171654272 20260531.3529 9.55CV 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 31.3529 2461191.8529 9.70 02:22:37.96 +56:37:19.4
135.27219 -4.04887 galactic Per Second-epoch detections are separated by 0.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458290469537534208 | 02:22:37.88 +56:37:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.731+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:37.96 +56:37:19.4: 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 02:22:37.96 +56:37:19.4: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 31.3529* 02 22 37.96 +56 37 19.4 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
Gaia DR3 458290469537534208,2461191.8529,9.70,0.05,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 458290469537534208 20260531.3529 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 31.3529 2461191.8529 9.55 02:24:27.17 +56:50:29.3
135.42992 -3.75615 galactic Per Second-epoch detections are separated by 5.0" and 4.2 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 458385130615759488 | 02:24:27.11 +56:50:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:27.17 +56:50:29.3: 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 02:24:27.17 +56:50:29.3: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 31.3529* 02 24 27.17 +56 50 29.3 9.6 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 458385130615759488,2461191.8529,9.55,0.05,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 458385130615759488 20260531.3529 9.55CV 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 31.3529 2461191.8529 9.57 02:36:52.73 +57:40:54.2
136.67561 -2.34892 galactic Cas Second-epoch detections are separated by 1.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.2360+57.6825 | 02:36:52.65 +57:40:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.172+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:52.73 +57:40:54.2: 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 02:36:52.73 +57:40:54.2: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 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 31.3529* 02 36 52.73 +57 40 54.2 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
ATO J039.2360+57.6825,2461191.8529,9.57,0.05,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
ATO J039.2360+57.6825 20260531.3529 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 31.3529 2461191.8529 9.93 00:58:55.95 +58:04:06.6
123.92624 -4.78878 galactic Cas Second-epoch detections are separated by 4.2" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:58:55.95 +58:04:06.6 (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 00:58:55.95 +58:04:06.6: 12.05 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:55.95 +58:04:06.6: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 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 31.3529* 00 58 55.95 +58 04 06.6 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
target,2461191.8529,9.93,0.05,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
target 20260531.3529 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 31.3529 2461191.8529 9.60 02:34:27.71 +56:43:27.0
136.74935 -3.35817 galactic Per Second-epoch detections are separated by 4.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6167+56.7240 | 02:34:27.71 +56:43:27.0 (user input) | dubious (ATLAS) | (ATLAS) | (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 02:34:27.71 +56:43:27.0: 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 02:34:27.71 +56:43:27.0: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 31.3529* 02 34 27.71 +56 43 27.0 9.6 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 J038.6167+56.7240,2461191.8529,9.60,0.05,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
ATO J038.6167+56.7240 20260531.3529 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 31.3529 2461191.8529 9.48 02:30:09.40 +57:23:13.6
135.95492 -2.96720 galactic Per Second-epoch detections are separated by 4.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.5396+57.3872 | 02:30:09.52 +57:23:14.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:09.40 +57:23:13.6: 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 02:30:09.40 +57:23:13.6: 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 31.3529* 02 30 09.40 +57 23 13.6 9.5 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 J037.5396+57.3872,2461191.8529,9.48,0.05,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
ATO J037.5396+57.3872 20260531.3529 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 31.3529 2461191.8529 9.54 02:29:02.18 +56:24:16.8
136.17704 -3.93644 galactic Per Second-epoch detections are separated by 1.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457554964966327808 | 02:29:02.21 +56:24:18.1 (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=0.167+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:02.18 +56:24:16.8: 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 02:29:02.18 +56:24:16.8: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 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 31.3529* 02 29 02.18 +56 24 16.8 9.5 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
Large-amplitude variable Gaia DR2 457554964966327808,2461191.8529,9.54,0.05,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
Large-amplitude variable Gaia DR2 457554964966327808 20260531.3529 9.54CV 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 31.3529 2461191.8529 9.57 02:30:26.89 +56:10:14.6
136.44642 -4.08099 galactic Per Second-epoch detections are separated by 3.3" and 4.2 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 457361107331848064 | 02:30:27.25 +56:10:14.2 (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 02:30:26.89 +56:10:14.6: 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 02:30:26.89 +56:10:14.6: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 31.3529* 02 30 26.89 +56 10 14.6 9.6 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 457361107331848064,2461191.8529,9.57,0.05,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
Gaia DR3 457361107331848064 20260531.3529 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 31.3529 2461191.8529 9.69 02:32:42.22 +57:14:26.4
136.32913 -2.97335 galactic Per Second-epoch detections are separated by 3.8" and 3.6 pix
The object was found in VSX20" ZTF J023242.66+571406.7
Type: BY
# Max. Min./Amp. JD0 Period
17.081 r Y 0.077 r 2458429.77470 3.429514200000
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 02:32:42.22 +57:14:26.4: 12.71 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:42.22 +57:14:26.4: 12.30 +/- 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 31.3529* 02 32 42.22 +57 14 26.4 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
ZTF J023242.66+571406.7,2461191.8529,9.69,0.05,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
ZTF J023242.66+571406.7 20260531.3529 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 31.3529 2461191.8529 9.42 02:36:28.05 +56:50:31.6
136.95641 -3.14225 galactic Per Second-epoch detections are separated by 3.2" and 4.3 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 J039.1180+56.8422 | 02:36:28.32 +56:50:31.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.901+/-0.048 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:28.05 +56:50:31.6: 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 02:36:28.05 +56:50:31.6: 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 31.3529* 02 36 28.05 +56 50 31.6 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
ATO J039.1180+56.8422,2461191.8529,9.42,0.05,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 J039.1180+56.8422 20260531.3529 9.42CV 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 31.3529 2461191.8529 9.46 02:33:18.04 +57:31:36.2
136.29413 -2.67827 galactic Per Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3024+57.5280 | 02:33:17.98 +57:31:36.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.149+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:18.04 +57:31:36.2: 13.15 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:18.04 +57:31:36.2: 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 31.3529* 02 33 18.04 +57 31 36.2 9.5 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 J038.3024+57.5280,2461191.8529,9.46,0.05,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
ATO J038.3024+57.5280 20260531.3529 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 31.3529 2461191.8529 9.51 02:31:18.63 +57:03:51.6
136.22090 -3.20809 galactic Per Second-epoch detections are separated by 2.3" and 3.5 pix
The object was found in VSX 4" Gaia DR3 457981403688250240
Type: ROT
# Max. Min./Amp. JD0 Period
12.410 G 12.440 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 02:31:18.63 +57:03:51.6: 13.00 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.63 +57:03:51.6: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 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 31.3529* 02 31 18.63 +57 03 51.6 9.5 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 457981403688250240,2461191.8529,9.51,0.05,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
Gaia DR3 457981403688250240 20260531.3529 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 31.3529 2461191.8529 9.51 02:36:19.82 +56:57:28.2
136.89350 -3.04327 galactic Per Second-epoch detections are separated by 0.6" and 4.0 pix
The object was found in VSX 6" ASASSN-V J023620.50+565726.0
Type: SRS
# Max. Min./Amp. JD0 Period
13.140 V 13.240 V 2457613.04700 25.122000000000
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 02:36:19.82 +56:57:28.2: 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 02:36:19.82 +56:57:28.2: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 31.3529* 02 36 19.82 +56 57 28.2 9.5 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
ASASSN-V J023620.50+565726.0,2461191.8529,9.51,0.05,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
ASASSN-V J023620.50+565726.0 20260531.3529 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 31.3529 2461191.8529 9.50 02:29:25.42 +55:58:54.2
136.38383 -4.30959 galactic Per Second-epoch detections are separated by 2.0" and 4.3 pix
The object was found in VSX 8" ASASSN-V J022926.29+555852.4
Type: SR
# Max. Min./Amp. JD0 Period
12.620 V 12.810 V 2457232.00000 79.400000000000
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 02:29:25.42 +55:58:54.2: 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 02:29:25.42 +55:58:54.2: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 31.3529* 02 29 25.42 +55 58 54.2 9.5 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
ASASSN-V J022926.29+555852.4,2461191.8529,9.50,0.05,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
ASASSN-V J022926.29+555852.4 20260531.3529 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 31.3529 2461191.8529 9.67 02:36:18.15 +56:52:17.8
136.92401 -3.12402 galactic Per Second-epoch detections are separated by 0.8" and 4.0 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 457788027079795584 | 02:36:18.77 +56:52:15.5 (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 02:36:18.15 +56:52:17.8: 11.44 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:18.15 +56:52:17.8: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 31.3529* 02 36 18.15 +56 52 17.8 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
Gaia DR3 457788027079795584,2461191.8529,9.67,0.05,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 457788027079795584 20260531.3529 9.67CV 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 31.3529 2461191.8529 9.59 02:34:42.56 +57:17:57.3
136.55714 -2.81501 galactic Per Second-epoch detections are separated by 2.7" and 4.0 pix
The object was found in VSX19" Gaia DR3 458004424713842560
Type: ROT
# Max. Min./Amp. JD0 Period
17.430 G 17.480 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 02:34:42.56 +57:17:57.3: 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 02:34:42.56 +57:17:57.3: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 31.3529* 02 34 42.56 +57 17 57.3 9.6 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 458004424713842560,2461191.8529,9.59,0.05,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 458004424713842560 20260531.3529 9.59CV 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 31.3529 2461191.8529 9.51 02:26:58.18 +56:22:09.7
135.92301 -4.07367 galactic Per Second-epoch detections are separated by 3.4" and 4.4 pix
The object was found in VSX25" Gaia DR3 457563348750748416
Type: ROT
# Max. Min./Amp. JD0 Period
16.950 G 17.010 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 02:26:58.18 +56:22:09.7: 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 02:26:58.18 +56:22:09.7: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 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 31.3529* 02 26 58.18 +56 22 09.7 9.5 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 457563348750748416,2461191.8529,9.51,0.05,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
Gaia DR3 457563348750748416 20260531.3529 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 31.3529 2461191.8529 9.48 02:34:40.76 +56:11:02.3
136.98704 -3.84442 galactic Per Second-epoch detections are separated by 2.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6605+56.1803 | 02:34:41.56 +56:11:01.9 (Gaia DR3) | IRR (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 02:34:40.76 +56:11:02.3: 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 02:34:40.76 +56:11:02.3: 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 31.3529* 02 34 40.76 +56 11 02.3 9.5 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 J038.6605+56.1803,2461191.8529,9.48,0.05,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
ATO J038.6605+56.1803 20260531.3529 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 31.3529 2461191.8529 9.53 02:33:07.75 +56:14:50.5
136.76326 -3.86904 galactic Per Second-epoch detections are separated by 2.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457375538423034496 | 02:33:08.17 +56:14:48.6 (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 02:33:07.75 +56:14:50.5: 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 02:33:07.75 +56:14:50.5: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 31.3529* 02 33 07.75 +56 14 50.5 9.5 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 457375538423034496,2461191.8529,9.53,0.05,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
Gaia DR3 457375538423034496 20260531.3529 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 31.3529 2461191.8529 9.57 02:36:19.79 +57:18:00.4
136.75849 -2.72867 galactic Per Second-epoch detections are separated by 3.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457908316220187520 | 02:36:19.92 +57:18:00.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:19.79 +57:18:00.4: 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 02:36:19.79 +57:18:00.4: 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 31.3529* 02 36 19.79 +57 18 00.4 9.6 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 457908316220187520,2461191.8529,9.57,0.05,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
Gaia DR3 457908316220187520 20260531.3529 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 31.3529 2461191.8529 9.62 02:27:40.45 +56:20:28.8
136.02436 -4.06442 galactic Per Second-epoch detections are separated by 3.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:27:40.45 +56:20:28.8 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.058 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:40.45 +56:20:28.8: 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 02:27:40.45 +56:20:28.8: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 31.3529* 02 27 40.45 +56 20 28.8 9.6 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
target,2461191.8529,9.62,0.05,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
target 20260531.3529 9.62CV 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 31.3529 2461191.8529 9.62 02:23:42.90 +56:38:37.4
135.40452 -3.97682 galactic Per Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.9286+56.6441 | 02:23:42.88 +56:38:38.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.179+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:42.90 +56:38:37.4: 12.55 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:42.90 +56:38:37.4: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 31.3529* 02 23 42.90 +56 38 37.4 9.6 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 J035.9286+56.6441,2461191.8529,9.62,0.05,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
ATO J035.9286+56.6441 20260531.3529 9.62CV 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 31.3529 2461191.8529 9.54 02:22:22.76 +56:39:59.4
135.22404 -4.01918 galactic Per Second-epoch detections are separated by 3.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458291362890696832 | 02:22:22.82 +56:40:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.912+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:22.76 +56:39:59.4: 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 02:22:22.76 +56:39:59.4: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 31.3529* 02 22 22.76 +56 39 59.4 9.5 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 458291362890696832,2461191.8529,9.54,0.05,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 458291362890696832 20260531.3529 9.54CV 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 31.3529 2461191.8529 9.54 02:30:38.78 +56:15:14.6
136.44080 -3.99340 galactic Per Second-epoch detections are separated by 5.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457384952991198080 | 02:30:39.44 +56:15:12.9 (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 02:30:38.78 +56:15:14.6: 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 02:30:38.78 +56:15:14.6: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 31.3529* 02 30 38.78 +56 15 14.6 9.5 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 457384952991198080,2461191.8529,9.54,0.05,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 457384952991198080 20260531.3529 9.54CV 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 31.3529 2461191.8529 9.58 02:33:02.03 +56:26:23.4
136.67721 -3.69628 galactic Per Second-epoch detections are separated by 4.5" and 4.5 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 J038.2606+56.4396 | 02:33:02.56 +56:26:22.8 (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 02:33:02.03 +56:26:23.4: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:02.03 +56:26:23.4: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 31.3529* 02 33 02.03 +56 26 23.4 9.6 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 J038.2606+56.4396,2461191.8529,9.58,0.05,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
ATO J038.2606+56.4396 20260531.3529 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 31.3529 2461191.8529 10.15 00:43:47.73 +61:54:01.0
122.03201 -0.95812 galactic Cas Second-epoch detections are separated by 1.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 427618218288011776 | 00:43:43.86 +61:53:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1991AJ....102..177L Cl* NGC 225 LMM 104 J-Ks=0.506+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:43:47.73 +61:54:01.0: 12.22 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:43:47.73 +61:54:01.0: 12.86 +/- 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 31.3529* 00 43 47.73 +61 54 01.0 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
Gaia DR3 427618218288011776,2461191.8529,10.15,0.05,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
Gaia DR3 427618218288011776 20260531.3529 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 31.3529 2461191.8529 9.70 02:18:56.11 +56:18:31.6
134.89701 -4.51678 galactic Per Second-epoch detections are separated by 1.3" and 4.0 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 J034.7162+56.3174 | 02:18:56.11 +56:18:31.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.608+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:56.11 +56:18:31.6: 12.57 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:56.11 +56:18:31.6: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 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 31.3529* 02 18 56.11 +56 18 31.6 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
ATO J034.7162+56.3174,2461191.8529,9.70,0.05,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
ATO J034.7162+56.3174 20260531.3529 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 31.3529 2461191.8529 9.46 02:33:25.63 +56:59:44.8
136.51377 -3.16208 galactic Per Second-epoch detections are separated by 3.7" and 4.0 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 457971400700134016 | 02:33:25.56 +56:59:42.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.198+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:25.63 +56:59:44.8: 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 02:33:25.63 +56:59:44.8: 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 31.3529* 02 33 25.63 +56 59 44.8 9.5 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 457971400700134016,2461191.8529,9.46,0.05,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
Gaia DR3 457971400700134016 20260531.3529 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 31.3529 2461191.8529 9.67 02:37:55.66 +58:18:21.1
136.55513 -1.72093 galactic Cas Second-epoch detections are separated by 2.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458153168019915904 | 02:37:55.90 +58:18:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.240+/-0.046 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:55.66 +58:18:21.1: 12.60 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:55.66 +58:18:21.1: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 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 31.3529* 02 37 55.66 +58 18 21.1 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 458153168019915904,2461191.8529,9.67,0.05,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 458153168019915904 20260531.3529 9.67CV 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 31.3529 2461191.8529 9.58 02:38:07.48 +58:00:10.7
136.70000 -1.98824 galactic Cas Second-epoch detections are separated by 0.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458144608145376896 | 02:38:07.33 +58:00:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.184+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:07.48 +58:00:10.7: 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 02:38:07.48 +58:00:10.7: 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 31.3529* 02 38 07.48 +58 00 10.7 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 458144608145376896,2461191.8529,9.58,0.05,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
Gaia DR3 458144608145376896 20260531.3529 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 31.3529 2461191.8529 9.53 02:26:55.93 +56:28:27.3
135.88018 -3.97774 galactic Per Second-epoch detections are separated by 6.7" and 5.0 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 J036.7308+56.4791 | 02:26:56.13 +56:28:21.8 (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 02:26:55.93 +56:28:27.3: 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 02:26:55.93 +56:28:27.3: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 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 31.3529* 02 26 55.93 +56 28 27.3 9.5 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 J036.7308+56.4791,2461191.8529,9.53,0.05,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
ATO J036.7308+56.4791 20260531.3529 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 31.3529 2461191.8529 9.62 02:32:05.93 +57:04:59.5
136.31311 -3.15017 galactic Per Second-epoch detections are separated by 1.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457975115856080512 | 02:32:05.87 +57:04:58.8 (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 02:32:05.93 +57:04:59.5: 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 02:32:05.93 +57:04:59.5: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 31.3529* 02 32 05.93 +57 04 59.5 9.6 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 457975115856080512,2461191.8529,9.62,0.05,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 457975115856080512 20260531.3529 9.62CV 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 31.3529 2461191.8529 10.03 01:18:14.25 +61:44:36.4
126.09862 -0.96342 galactic Cas Second-epoch detections are separated by 3.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:14.25 +61:44:36.4 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:14.25 +61:44:36.4: 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 01:18:14.25 +61:44:36.4: 12.77 +/- 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 31.3529* 01 18 14.25 +61 44 36.4 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
target,2461191.8529,10.03,0.05,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
target 20260531.3529 10.03CV 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 31.3529 2461191.8529 9.68 02:33:01.80 +57:36:06.2
136.23183 -2.62286 galactic Per Second-epoch detections are separated by 3.2" and 4.0 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 J038.2578+57.6016 | 02:33:01.89 +57:36:06.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.137+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:01.80 +57:36:06.2: 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 02:33:01.80 +57:36:06.2: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 31.3529* 02 33 01.80 +57 36 06.2 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
ATO J038.2578+57.6016,2461191.8529,9.68,0.05,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
ATO J038.2578+57.6016 20260531.3529 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 31.3529 2461191.8529 9.52 02:30:49.71 +56:26:27.4
136.39410 -3.81066 galactic Per Second-epoch detections are separated by 2.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457575821336762496 | 02:30:50.16 +56:26:30.0 (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 02:30:49.71 +56:26:27.4: 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 02:30:49.71 +56:26:27.4: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 31.3529* 02 30 49.71 +56 26 27.4 9.5 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 457575821336762496,2461191.8529,9.52,0.05,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 457575821336762496 20260531.3529 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 31.3529 2461191.8529 9.73 02:28:42.38 +55:58:14.1
136.29442 -4.35695 galactic Per Second-epoch detections are separated by 7.7" and 5.2 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 J037.1657+55.9806 | 02:28:43.20 +55:58:17.1 (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 02:28:42.38 +55:58:14.1: 12.91 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:42.38 +55:58:14.1: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 31.3529* 02 28 42.38 +55 58 14.1 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
ATO J037.1657+55.9806,2461191.8529,9.73,0.05,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
ATO J037.1657+55.9806 20260531.3529 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 31.3529 2461191.8529 9.68 02:31:52.59 +56:53:47.2
136.35587 -3.33448 galactic Per Second-epoch detections are separated by 1.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9796+56.9058 | 02:31:52.57 +56:53:48.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:52.59 +56:53:47.2: 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 02:31:52.59 +56:53:47.2: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 31.3529* 02 31 52.59 +56 53 47.2 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
ATO J037.9796+56.9058,2461191.8529,9.68,0.05,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
ATO J037.9796+56.9058 20260531.3529 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 31.3529 2461191.8529 9.73 02:37:59.24 +58:07:39.6
136.63350 -1.88118 galactic Cas Second-epoch detections are separated by 1.6" and 3.7 pix
The object was found in VSX 2" Gaia DR3 458146639669716992
Type: L
# Max. Min./Amp. JD0 Period
11.580 G 11.700 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 02:37:59.24 +58:07:39.6: 12.64 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:59.24 +58:07:39.6: 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 31.3529* 02 37 59.24 +58 07 39.6 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 458146639669716992,2461191.8529,9.73,0.05,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
Gaia DR3 458146639669716992 20260531.3529 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 31.3529 2461191.8529 9.71 02:27:44.77 +56:19:42.5
136.03837 -4.07277 galactic Per Second-epoch detections are separated by 6.3" and 4.6 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 457559496157823232 | 02:27:44.64 +56:19:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.083+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:44.77 +56:19:42.5: 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 02:27:44.77 +56:19:42.5: 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 31.3529* 02 27 44.77 +56 19 42.5 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
Gaia DR3 457559496157823232,2461191.8529,9.71,0.05,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 457559496157823232 20260531.3529 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 31.3529 2461191.8529 9.70 02:33:08.38 +57:21:21.6
136.33953 -2.84427 galactic Per Second-epoch detections are separated by 5.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2862+57.3553 | 02:33:08.69 +57:21:19.4 (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 02:33:08.38 +57:21:21.6: 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 02:33:08.38 +57:21:21.6: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 31.3529* 02 33 08.38 +57 21 21.6 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
ATO J038.2862+57.3553,2461191.8529,9.70,0.05,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
ATO J038.2862+57.3553 20260531.3529 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 31.3529 2461191.8529 9.73 02:38:19.80 +58:03:54.5
136.70003 -1.92039 galactic Cas Second-epoch detections are separated by 6.0" and 4.0 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 458145368359426176 | 02:38:19.85 +58:03:55.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.841+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:19.80 +58:03:54.5: 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 02:38:19.80 +58:03:54.5: 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 31.3529* 02 38 19.80 +58 03 54.5 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 458145368359426176,2461191.8529,9.73,0.05,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
Gaia DR3 458145368359426176 20260531.3529 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 31.3529 2461191.8529 9.78 02:35:58.83 +57:31:57.8
136.62368 -2.53327 galactic Per Second-epoch detections are separated by 5.7" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.9960+57.5329 | 02:35:59.06 +57:31:58.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.009+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:58.83 +57:31:57.8: 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 02:35:58.83 +57:31:57.8: 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 31.3529* 02 35 58.83 +57 31 57.8 9.8 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 J038.9960+57.5329,2461191.8529,9.78,0.05,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
ATO J038.9960+57.5329 20260531.3529 9.78CV 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 31.3529 2461191.8529 10.15 01:29:32.82 +61:46:26.3
127.42211 -0.76509 galactic Cas Second-epoch detections are separated by 1.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:32.82 +61:46:26.3 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:32.82 +61:46:26.3: 12.94 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:32.82 +61:46:26.3: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 31.3529* 01 29 32.82 +61 46 26.3 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
target,2461191.8529,10.15,0.05,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
target 20260531.3529 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 31.3529 2461191.8529 9.79 02:35:43.57 +57:50:30.9
136.47109 -2.26213 galactic Cas Second-epoch detections are separated by 2.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458115608524444160 | 02:35:43.49 +57:50:31.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.452+/-0.027 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:43.57 +57:50:30.9: 12.12 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:43.57 +57:50:30.9: 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 31.3529* 02 35 43.57 +57 50 30.9 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 458115608524444160,2461191.8529,9.79,0.05,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
Gaia DR3 458115608524444160 20260531.3529 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 31.3529 2461191.8529 9.78 02:29:48.85 +56:41:55.4
136.16785 -3.62359 galactic Per Second-epoch detections are separated by 3.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457599525253006080 | 02:29:48.84 +56:41:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.727+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:48.85 +56:41:55.4: 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 02:29:48.85 +56:41:55.4: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 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 31.3529* 02 29 48.85 +56 41 55.4 9.8 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 457599525253006080,2461191.8529,9.78,0.05,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 457599525253006080 20260531.3529 9.78CV 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 31.3529 2461191.8529 10.61 01:22:23.81 +61:13:50.8
126.64934 -1.41732 galactic Cas Second-epoch detections are separated by 1.4" and 3.2 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 01:22:23.81 +61:13:50.8: 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 01:22:23.81 +61:13:50.8: 15.71 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.71 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.3529* 01 22 23.81 +61 13 50.8 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0122238+611352,2461191.8529,10.61,0.05,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
NSVS J0122238+611352 20260531.3529 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.90 02:31:18.55 +56:20:48.9
136.49128 -3.87282 galactic Per Second-epoch detections are separated by 2.0" and 4.3 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 457386739697519488 | 02:31:19.13 +56:20:48.8 (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 02:31:18.55 +56:20:48.9: 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 02:31:18.55 +56:20:48.9: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 31.3529* 02 31 18.55 +56 20 48.9 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 457386739697519488,2461191.8529,8.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260531.3529 8.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.15 02:33:40.20 +57:40:02.4
136.28586 -2.52943 galactic Per Second-epoch detections are separated by 2.3" and 4.0 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 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 02:33:40.20 +57:40:02.4: 13.19 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:40.20 +57:40:02.4: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.77 +/- 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 31.3529* 02 33 40.20 +57 40 02.4 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 J038.4074+57.6734,2461191.8529,8.15,0.05,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
ATO J038.4074+57.6734 20260531.3529 8.15CV 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 31.3529 2461191.8529 9.55 02:17:19.11 +56:42:44.0
134.55248 -4.20939 galactic Per Second-epoch detections are separated by 3.9" and 4.5 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 J034.3299+56.7126 | 02:17:19.18 +56:42:45.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A9V (LAMOST DR5) J-Ks=0.066+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:17:19.11 +56:42:44.0: 11.22 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:19.11 +56:42:44.0: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 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 31.3529* 02 17 19.11 +56 42 44.0 9.6 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 J034.3299+56.7126,2461191.8529,9.55,0.05,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
ATO J034.3299+56.7126 20260531.3529 9.55CV 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 31.3529 2461191.8529 9.29 01:31:28.05 +57:20:36.4
128.33393 -5.10785 galactic Cas Second-epoch detections are separated by 0.9" and 3.8 pix
The object was found in VSX 2" 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 01:31:28.05 +57:20:36.4: 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 01:31:28.05 +57:20:36.4: 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 31.3529* 01 31 28.05 +57 20 36.4 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
GSC 03678-01834,2461191.8529,9.29,0.05,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
GSC 03678-01834 20260531.3529 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 31.3529 2461191.8529 6.84 02:21:40.76 +60:54:41.6
133.68158 -0.06274 galactic Cas Second-epoch detections are separated by 0.6" and 3.2 pix
The object was found in VSX 1" 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 02:21:40.76 +60:54:41.6: 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 02:21:40.76 +60:54:41.6: 11.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.23 +/- 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 31.3529* 02 21 40.76 +60 54 41.6 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
DE Cas,2461191.8529,6.84,0.05,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
DE Cas 20260531.3529 6.84CV 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 31.3529 2461191.8529 9.47 02:15:20.33 +62:13:49.2
132.53398 0.93298 galactic Cas Second-epoch detections are separated by 2.3" and 3.4 pix
The object was found in VSX 1" 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 02:15:20.33 +62:13:49.2: 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 02:15:20.33 +62:13:49.2: 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 31.3529* 02 15 20.33 +62 13 49.2 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
V0930 Cas,2461191.8529,9.47,0.05,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
V0930 Cas 20260531.3529 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 31.3529 2461191.8529 9.09 02:15:35.89 +56:21:36.7
134.44167 -4.61922 galactic Per Second-epoch detections are separated by 3.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:15:35.89 +56:21:36.7: 12.92 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:35.89 +56:21:36.7: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 31.3529* 02 15 35.89 +56 21 36.7 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 J033.8885+56.3660,2461191.8529,9.09,0.05,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
ATO J033.8885+56.3660 20260531.3529 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 31.3529 2461191.8529 9.10 02:05:05.69 +58:16:23.9
132.50913 -3.22220 galactic Per Second-epoch detections are separated by 1.3" and 3.6 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 02:05:05.69 +58:16:23.9: 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 02:05:05.69 +58:16:23.9: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 31.3529* 02 05 05.69 +58 16 23.9 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
V0661 Per,2461191.8529,9.10,0.05,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
V0661 Per 20260531.3529 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 31.3529 2461191.8529 9.78 02:19:03.87 +62:47:34.5
132.75748 1.60483 galactic Cas Second-epoch detections are separated by 2.3" and 3.4 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 02:19:03.87 +62:47:34.5: 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 02:19:03.87 +62:47:34.5: 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 31.3529* 02 19 03.87 +62 47 34.5 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
ASASSN-V J021904.01+624734.4,2461191.8529,9.78,0.05,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 J021904.01+624734.4 20260531.3529 9.78CV 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 31.3529 2461191.8529 9.34 02:29:57.73 +57:10:58.0
136.00657 -3.16665 galactic Per Second-epoch detections are separated by 1.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458032874577920256 | 02:30:00.30 +57:11:30.1 (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 02:29:57.73 +57:10:58.0: 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 02:29:57.73 +57:10:58.0: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 31.3529* 02 29 57.73 +57 10 58.0 9.3 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 458032874577920256,2461191.8529,9.34,0.05,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
Gaia DR3 458032874577920256 20260531.3529 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 31.3529 2461191.8529 9.69 02:38:02.15 +58:50:40.7
136.35295 -1.22130 galactic Cas Second-epoch detections are separated by 5.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.5186+58.8445 | 02:38:02.39 +58:50:41.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:02.15 +58:50:40.7: 10.22 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:02.15 +58:50:40.7: 12.49 +/- 0.02 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 31.3529* 02 38 02.15 +58 50 40.7 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
ATO J039.5186+58.8445,2461191.8529,9.69,0.05,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
ATO J039.5186+58.8445 20260531.3529 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 31.3529 2461191.8529 8.79 02:34:36.31 +58:11:22.9
136.19873 -1.99963 galactic Per Second-epoch detections are separated by 1.6" and 3.7 pix
The object was found in VSX 4" ASASSN-V J023436.74+581121.5
Type: SR
# Max. Min./Amp. JD0 Period
14.040 g Y 0.370 g 2459254.72100 32.650000000000
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 02:34:36.31 +58:11:22.9: 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 02:34:36.31 +58:11:22.9: 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 31.3529* 02 34 36.31 +58 11 22.9 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
ASASSN-V J023436.74+581121.5,2461191.8529,8.79,0.05,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 J023436.74+581121.5 20260531.3529 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 31.3529 2461191.8529 8.24 02:24:29.91 +59:24:30.8
134.53144 -1.35107 galactic Cas Second-epoch detections are separated by 1.3" and 3.6 pix
The object was found in VSX 0" 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 02:24:29.91 +59:24:30.8: 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 02:24:29.91 +59:24:30.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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 31.3529* 02 24 29.91 +59 24 30.8 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
V0672 Cas,2461191.8529,8.24,0.05,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
V0672 Cas 20260531.3529 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 31.3529 2461191.8529 9.23 01:21:54.72 +61:20:55.4
126.57748 -1.30714 galactic Cas Second-epoch detections are separated by 1.0" and 3.3 pix
The object was found in ASASSN-V 0" 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 01:21:54.72 +61:20:55.4: 13.21 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:54.72 +61:20:55.4: 14.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.3529* 01 21 54.72 +61 20 55.4 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
VARIABLE_NAME,2461191.8529,9.23,0.05,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
VARIABLE_NAME 20260531.3529 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 31.3529 2461191.8529 8.24 02:25:13.36 +56:30:31.4
135.64698 -4.03002 galactic Per Second-epoch detections are separated by 0.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:25:13.36 +56:30:31.4: 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 02:25:13.36 +56:30:31.4: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 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 31.3529* 02 25 13.36 +56 30 31.4 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 J036.2868+56.5107,2461191.8529,8.24,0.05,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 J036.2868+56.5107 20260531.3529 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 31.3529 2461191.8529 9.61 02:26:44.41 +58:15:51.9
135.20981 -2.31721 galactic Per Second-epoch detections are separated by 2.3" and 4.0 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 458910525375062528 | 02:26:44.54 +58:15:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.220+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:44.41 +58:15:51.9: 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 02:26:44.41 +58:15:51.9: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 31.3529* 02 26 44.41 +58 15 51.9 9.6 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 458910525375062528,2461191.8529,9.61,0.05,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
Gaia DR3 458910525375062528 20260531.3529 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 31.3529 2461191.8529 9.72 02:29:19.57 +57:07:07.2
135.95012 -3.25815 galactic Per Second-epoch detections are separated by 1.4" and 3.9 pix
The object was found in VSX 3" ASASSN-V J022919.80+570705.4
Type: SRS
# Max. Min./Amp. JD0 Period
14.310 g Y 0.240 g 2458654.10200 25.078000000000
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 02:29:19.57 +57:07:07.2: 12.10 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:19.57 +57:07:07.2: 12.84 +/- 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 31.3529* 02 29 19.57 +57 07 07.2 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
ASASSN-V J022919.80+570705.4,2461191.8529,9.72,0.05,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
ASASSN-V J022919.80+570705.4 20260531.3529 9.72CV 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 31.3529 2461191.8529 10.28 01:27:44.31 +62:06:39.9
127.16315 -0.46207 galactic Cas Second-epoch detections are separated by 0.6" and 3.0 pix
The object was found in VSX 1" 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 01:27:44.31 +62:06:39.9: 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 01:27:44.31 +62:06:39.9: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.3529* 01 27 44.31 +62 06 39.9 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
NSVS 1696374,2461191.8529,10.28,0.05,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
NSVS 1696374 20260531.3529 10.28CV 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 31.3529 2461191.8529 9.81 01:41:46.90 +59:03:47.3
129.37380 -3.17750 galactic Cas Second-epoch detections are separated by 1.8" and 3.7 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 01:41:46.90 +59:03:47.3: 11.41 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:46.90 +59:03:47.3: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.3529* 01 41 46.90 +59 03 47.3 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 J014146.93+590346.7,2461191.8529,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260531.3529 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.90 02:14:24.94 +56:42:49.3
134.17379 -4.33601 galactic Per Second-epoch detections are separated by 0.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457025172169888384 | 02:14:25.03 +56:42:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.091+/-0.037 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:24.94 +56:42:49.3: 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 02:14:24.94 +56:42:49.3: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 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 31.3529* 02 14 24.94 +56 42 49.3 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 457025172169888384,2461191.8529,8.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457025172169888384 20260531.3529 8.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 8.84 02:08:53.89 +58:42:29.3
132.85995 -2.66249 galactic Per Second-epoch detections are separated by 0.8" and 3.7 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 02:08:53.89 +58:42:29.3: 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 02:08:53.89 +58:42:29.3: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.3529* 02 08 53.89 +58 42 29.3 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
NSVS J0208545+584228,2461191.8529,8.84,0.05,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 J0208545+584228 20260531.3529 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 31.3529 2461191.8529 8.15 02:31:45.72 +56:26:45.7
136.51195 -3.75739 galactic Per Second-epoch detections are separated by 0.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457393336767227264 | 02:31:45.96 +56:26:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:45.72 +56:26:45.7: 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 02:31:45.72 +56:26:45.7: 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 31.3529* 02 31 45.72 +56 26 45.7 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
Gaia DR3 457393336767227264,2461191.8529,8.15,0.05,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
Gaia DR3 457393336767227264 20260531.3529 8.15CV 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 31.3529 2461191.8529 9.35 02:33:34.77 +57:08:54.4
136.47421 -3.01317 galactic Per Second-epoch detections are separated by 0.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3948+57.1482 | 02:33:34.77 +57:08:53.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.942+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.77 +57:08:54.4: 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 02:33:34.77 +57:08:54.4: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 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 31.3529* 02 33 34.77 +57 08 54.4 9.3 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 J038.3948+57.1482,2461191.8529,9.35,0.05,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
ATO J038.3948+57.1482 20260531.3529 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 31.3529 2461191.8529 10.40 01:32:51.45 +62:40:36.3
127.66449 0.18621 galactic Cas Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX 1" ASASSN-V J013251.56+624035.5
Type: SR
# Max. Min./Amp. JD0 Period
14.830 V 15.470 V 2458353.38020 131.762706400000
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 01:32:51.45 +62:40:36.3: 13.08 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:51.45 +62:40:36.3: 14.32 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.3529* 01 32 51.45 +62 40 36.3 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
ASASSN-V J013251.56+624035.5,2461191.8529,10.40,0.05,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
ASASSN-V J013251.56+624035.5 20260531.3529 10.40CV 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 31.3529 2461191.8529 9.54 02:31:42.43 +56:35:52.7
136.44739 -3.61958 galactic Per Second-epoch detections are separated by 1.8" and 4.0 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 457583930234825344 | 02:31:42.90 +56:35:54.8 (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 02:31:42.43 +56:35:52.7: 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 02:31:42.43 +56:35:52.7: 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 31.3529* 02 31 42.43 +56 35 52.7 9.5 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 457583930234825344,2461191.8529,9.54,0.05,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 457583930234825344 20260531.3529 9.54CV 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 31.3529 2461191.8529 8.77 02:19:16.63 +59:42:21.5
133.80803 -1.29801 galactic Cas Second-epoch detections are separated by 0.7" and 3.5 pix
The object was found in VSX 1" 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 02:19:16.63 +59:42:21.5: 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 02:19:16.63 +59:42:21.5: 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 31.3529* 02 19 16.63 +59 42 21.5 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 J021916.76+594221.6,2461191.8529,8.77,0.05,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
ZTF J021916.76+594221.6 20260531.3529 8.77CV 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 31.3529 2461191.8529 9.54 02:29:16.20 +56:24:33.1
136.20548 -3.92031 galactic Per Second-epoch detections are separated by 1.0" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.3315+56.4071 | 02:29:16.79 +56:24:33.2 (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 02:29:16.20 +56:24:33.1: 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 02:29:16.20 +56:24:33.1: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 31.3529* 02 29 16.20 +56 24 33.1 9.5 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 J037.3315+56.4071,2461191.8529,9.54,0.05,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 J037.3315+56.4071 20260531.3529 9.54CV 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 31.3529 2461191.8529 9.45 02:17:01.69 +56:56:08.6
134.44177 -4.01106 galactic Per Second-epoch detections are separated by 3.9" and 3.5 pix
The object was found in VSX15" Gaia DR3 458532327733907328
Type: RS
# Max. Min./Amp. JD0 Period
17.140 G 17.310 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 02:17:01.69 +56:56:08.6: 12.16 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:01.69 +56:56:08.6: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 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 31.3529* 02 17 01.69 +56 56 08.6 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
Gaia DR3 458532327733907328,2461191.8529,9.45,0.05,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
Gaia DR3 458532327733907328 20260531.3529 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 31.3529 2461191.8529 9.49 02:19:48.16 +56:25:08.9
134.97359 -4.37262 galactic Per Second-epoch detections are separated by 6.3" and 4.6 pix
The object was found in VSX24" Gaia DR3 458272499382317568
Type: S
# Max. Min./Amp. JD0 Period
17.040 G 17.360 G O
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 02:19:48.16 +56:25:08.9: 12.57 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:48.16 +56:25:08.9: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 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 31.3529* 02 19 48.16 +56 25 08.9 9.5 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 458272499382317568,2461191.8529,9.49,0.05,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 458272499382317568 20260531.3529 9.49CV 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 31.3529 2461191.8529 9.75 02:15:26.96 +62:47:45.2
132.36569 1.47308 galactic Cas Second-epoch detections are separated by 1.4" and 3.1 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 02:15:26.96 +62:47:45.2: 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 02:15:26.96 +62:47:45.2: 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 31.3529* 02 15 26.96 +62 47 45.2 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
ASASSN-V J021526.89+624746.2,2461191.8529,9.75,0.05,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 J021526.89+624746.2 20260531.3529 9.75CV 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 31.3529 2461191.8529 8.15 02:33:31.89 +57:34:08.3
136.30654 -2.62737 galactic Per Second-epoch detections are separated by 0.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO 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 02:33:31.89 +57:34:08.3: 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 02:33:31.89 +57:34:08.3: 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 31.3529* 02 33 31.89 +57 34 08.3 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 J038.3788+57.5785,2461191.8529,8.15,0.05,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
ATO J038.3788+57.5785 20260531.3529 8.15CV 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 31.3529 2461191.8529 8.51 01:16:28.98 +60:13:59.7
126.03872 -2.48733 galactic Cas Second-epoch detections are separated by 0.2" and 3.3 pix
The object was found in ASASSN-V 2" 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 01:16:28.98 +60:13:59.7: 12.37 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:28.98 +60:13:59.7: 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 31.3529* 01 16 28.98 +60 13 59.7 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
VARIABLE_NAME,2461191.8529,8.51,0.05,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
VARIABLE_NAME 20260531.3529 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 31.3529 2461191.8529 9.20 02:28:27.94 +57:25:38.4
135.72813 -3.01387 galactic Per Second-epoch detections are separated by 1.9" and 3.7 pix
The object was found in VSX 1" Gaia DR3 458051527614654848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.390 G 12.430 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 02:28:27.94 +57:25:38.4: 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 02:28:27.94 +57:25:38.4: 12.03 +/- 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 31.3529* 02 28 27.94 +57 25 38.4 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 458051527614654848,2461191.8529,9.20,0.05,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
Gaia DR3 458051527614654848 20260531.3529 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 31.3529 2461191.8529 9.03 02:13:41.76 +57:25:36.7
133.85574 -3.68985 galactic Per Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J033.4051+57.4276 | 02:13:42.22 +57:25:36.3 (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 02:13:41.76 +57:25:36.7: 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 02:13:41.76 +57:25:36.7: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 31.3529* 02 13 41.76 +57 25 36.7 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
ATO J033.4051+57.4276,2461191.8529,9.03,0.05,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 J033.4051+57.4276 20260531.3529 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 31.3529 2461191.8529 9.73 02:18:24.65 +58:37:26.1
134.06205 -2.35570 galactic Per Second-epoch detections are separated by 2.5" and 3.6 pix
The object was found in VSX 2" 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 02:18:24.65 +58:37:26.1: 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 02:18:24.65 +58:37:26.1: 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 31.3529* 02 18 24.65 +58 37 26.1 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
TSVSC1 TN-N311132011-556-86-2,2461191.8529,9.73,0.05,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
TSVSC1 TN-N311132011-556-86-2 20260531.3529 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 31.3529 2461191.8529 8.87 02:33:51.42 +56:10:59.9
136.88156 -3.88931 galactic Per Second-epoch detections are separated by 1.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4611+56.1832 | 02:33:52.13 +56:11:00.2 (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 02:33:51.42 +56:10:59.9: 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 02:33:51.42 +56:10:59.9: 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 31.3529* 02 33 51.42 +56 10 59.9 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 J038.4611+56.1832,2461191.8529,8.87,0.05,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 J038.4611+56.1832 20260531.3529 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 31.3529 2461191.8529 8.11 02:22:56.62 +57:11:45.0
135.11304 -3.49588 galactic Per Second-epoch detections are separated by 1.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7523+57.1948 | 02:22:56.77 +57:11:44.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.065+/-0.038 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:56.62 +57:11:45.0: 9.57 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:56.62 +57:11:45.0: 10.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.49 +/- 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 31.3529* 02 22 56.62 +57 11 45.0 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 J035.7523+57.1948,2461191.8529,8.11,0.05,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
ATO J035.7523+57.1948 20260531.3529 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 31.3529 2461191.8529 9.05 02:27:27.68 +56:03:05.8
136.10229 -4.34509 galactic Per Second-epoch detections are separated by 1.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J036.8516+56.0508 | 02:27:27.82 +56:03:04.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.934+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:27.68 +56:03:05.8: 11.10 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:27.68 +56:03:05.8: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 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 31.3529* 02 27 27.68 +56 03 05.8 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 J036.8516+56.0508,2461191.8529,9.05,0.05,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 J036.8516+56.0508 20260531.3529 9.05CV 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 31.3529 2461191.8529 9.69 01:30:50.27 +60:32:13.3
127.76146 -1.96474 galactic Cas Second-epoch detections are separated by 2.1" and 3.6 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 01:30:50.27 +60:32:13.3: 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 01:30:50.27 +60:32:13.3: 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 31.3529* 01 30 50.27 +60 32 13.3 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
NSVS J0130502+603215,2461191.8529,9.69,0.05,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 J0130502+603215 20260531.3529 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 31.3529 2461191.8529 9.26 02:34:12.69 +56:03:50.1
136.97345 -3.98036 galactic Per Second-epoch detections are separated by 1.1" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5561+56.0631 | 02:34:13.47 +56:03:47.4 (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 02:34:12.69 +56:03:50.1: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:12.69 +56:03:50.1: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 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 31.3529* 02 34 12.69 +56 03 50.1 9.3 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 J038.5561+56.0631,2461191.8529,9.26,0.05,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
ATO J038.5561+56.0631 20260531.3529 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 31.3529 2461191.8529 9.27 02:29:46.25 +56:03:50.4
136.39843 -4.21520 galactic Per Second-epoch detections are separated by 2.4" and 4.2 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 457358564711288576 | 02:29:46.93 +56:03:52.7 (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 02:29:46.25 +56:03:50.4: 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 02:29:46.25 +56:03:50.4: 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 31.3529* 02 29 46.25 +56 03 50.4 9.3 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 457358564711288576,2461191.8529,9.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457358564711288576 20260531.3529 9.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.3529 2461191.8529 9.37 01:24:30.58 +59:38:48.3
127.10471 -2.95679 galactic Cas Second-epoch detections are separated by 1.3" and 3.4 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 01:24:30.58 +59:38:48.3: 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 01:24:30.58 +59:38:48.3: 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 31.3529* 01 24 30.58 +59 38 48.3 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
ASASSN-V J012430.51+593847.9,2461191.8529,9.37,0.05,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 J012430.51+593847.9 20260531.3529 9.37CV 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 31.3529 2461191.8529 9.12 02:21:26.44 +57:16:58.2
134.89179 -3.48411 galactic Per Second-epoch detections are separated by 2.8" and 4.2 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 J035.3797+57.2867 | 02:21:26.45 +57:16:55.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.400+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:26.44 +57:16:58.2: 11.54 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:26.44 +57:16:58.2: 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 31.3529* 02 21 26.44 +57 16 58.2 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 J035.3797+57.2867,2461191.8529,9.12,0.05,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
ATO J035.3797+57.2867 20260531.3529 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 31.3529 2461191.8529 6.83 02:01:28.14 +58:18:14.4
132.04182 -3.32366 galactic Cas Second-epoch detections are separated by 1.1" and 3.7 pix
The object was found in VSX 0" 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 02:01:28.14 +58:18:14.4: 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 02:01:28.14 +58:18:14.4: 10.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.50 +/- 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 31.3529* 02 01 28.14 +58 18 14.4 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
V0666 Cas,2461191.8529,6.83,0.05,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
V0666 Cas 20260531.3529 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 31.3529 2461191.8529 8.84 02:29:59.54 +56:13:01.3
136.37013 -4.06166 galactic Per Second-epoch detections are separated by 1.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 02:29:59.54 +56:13:01.3: 11.58 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:59.54 +56:13:01.3: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 31.3529* 02 29 59.54 +56 13 01.3 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 457548814581644416,2461191.8529,8.84,0.05,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
Gaia DR3 457548814581644416 20260531.3529 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 31.3529 2461191.8529 7.08 02:34:05.60 +56:37:26.3
136.74141 -3.47015 galactic Per Second-epoch detections are separated by 0.4" and 3.9 pix
The object was found in VSX23" Gaia DR3 457763322428148096
Type: ROT
# Max. Min./Amp. JD0 Period
15.220 G 15.260 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 02:34:05.60 +56:37:26.3: 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 02:34:05.60 +56:37:26.3: 9.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.65 +/- 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 31.3529* 02 34 05.60 +56 37 26.3 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 457763322428148096,2461191.8529,7.08,0.05,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 457763322428148096 20260531.3529 7.08CV 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 31.3529 2461191.8529 9.07 02:38:48.25 +57:57:34.8
136.79993 -1.99181 galactic Cas Second-epoch detections are separated by 2.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.7144+57.9584 | 02:38:48.32 +57:57:33.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.120+/-0.028 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:48.25 +57:57:34.8: 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 02:38:48.25 +57:57:34.8: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 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 31.3529* 02 38 48.25 +57 57 34.8 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
ATO J039.7144+57.9584,2461191.8529,9.07,0.05,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
ATO J039.7144+57.9584 20260531.3529 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 31.3529 2461191.8529 9.84 02:27:22.20 +62:38:25.9
133.70336 1.79229 galactic Cas Second-epoch detections are separated by 2.7" and 2.7 pix
The object was found in VSX 1" 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 02:27:22.20 +62:38:25.9: 10.70 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:22.20 +62:38:25.9: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.90 +/- 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 31.3529* 02 27 22.20 +62 38 25.9 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
V0937 Cas,2461191.8529,9.84,0.05,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
V0937 Cas 20260531.3529 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 31.3529 2461191.8529 9.96 01:09:38.04 +59:05:14.4
125.27197 -3.70172 galactic Cas Second-epoch detections are separated by 1.4" and 3.5 pix
The object was found in VSX 2" 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 01:09:38.04 +59:05:14.4: 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 01:09:38.04 +59:05:14.4: 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 31.3529* 01 09 38.04 +59 05 14.4 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 1731355,2461191.8529,9.96,0.05,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
NSVS 1731355 20260531.3529 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 31.3529 2461191.8529 9.38 02:27:55.40 +56:27:24.2
136.01443 -3.94440 galactic Per Second-epoch detections are separated by 1.9" and 3.9 pix
The object was found in VSX 2" ASASSN-V J022755.53+562722.6
Type: SRS
# Max. Min./Amp. JD0 Period
13.790 g Y 0.160 g 2458428.83700 25.028000000000
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 02:27:55.40 +56:27:24.2: 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 02:27:55.40 +56:27:24.2: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 31.3529* 02 27 55.40 +56 27 24.2 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
ASASSN-V J022755.53+562722.6,2461191.8529,9.38,0.05,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 J022755.53+562722.6 20260531.3529 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 31.3529 2461191.8529 10.31 01:14:56.64 +59:42:13.1
125.89674 -3.03273 galactic Cas Second-epoch detections are separated by 3.0" and 3.9 pix
The object was found in VSX 0" 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 01:14:56.64 +59:42:13.1: 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 01:14:56.64 +59:42:13.1: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.3529* 01 14 56.64 +59 42 13.1 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
NSVS J0114566+594210,2461191.8529,10.31,0.05,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 J0114566+594210 20260531.3529 10.31CV 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 31.3529 2461191.8529 9.30 02:21:35.99 +57:03:40.3
134.98795 -3.68506 galactic Per Second-epoch detections are separated by 2.5" and 3.4 pix
The object was found in VSX24" Gaia DR3 458452578783931008
Type: RS
# Max. Min./Amp. JD0 Period
12.960 G 13.000 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 02:21:35.99 +57:03:40.3: 12.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:35.99 +57:03:40.3: 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 31.3529* 02 21 35.99 +57 03 40.3 9.3 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 458452578783931008,2461191.8529,9.30,0.05,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
Gaia DR3 458452578783931008 20260531.3529 9.30CV 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 31.3529 2461191.8529 8.73 02:19:34.14 +58:23:58.2
134.27942 -2.51716 galactic Per Second-epoch detections are separated by 1.6" and 3.6 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 02:19:34.14 +58:23:58.2: 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 02:19:34.14 +58:23:58.2: 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 31.3529* 02 19 34.14 +58 23 58.2 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
NSVS 1909158,2461191.8529,8.73,0.05,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
NSVS 1909158 20260531.3529 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 31.3529 2461191.8529 9.48 02:31:32.42 +56:47:58.9
136.34985 -3.44143 galactic Per Second-epoch detections are separated by 2.4" and 4.0 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 457964803634866560 | 02:31:32.30 +56:47:58.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.863+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:32.42 +56:47:58.9: 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 02:31:32.42 +56:47:58.9: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 31.3529* 02 31 32.42 +56 47 58.9 9.5 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 457964803634866560,2461191.8529,9.48,0.05,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
Gaia DR3 457964803634866560 20260531.3529 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 31.3529 2461191.8529 9.12 02:32:22.18 +58:28:54.4
135.81555 -1.84241 galactic Per Second-epoch detections are separated by 2.0" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1041+58.4796 | 02:32:22.34 +58:28:55.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3IV (LAMOST DR5) J-Ks=0.137+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:22.18 +58:28:54.4: 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 02:32:22.18 +58:28:54.4: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 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 31.3529* 02 32 22.18 +58 28 54.4 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 J038.1041+58.4796,2461191.8529,9.12,0.05,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
ATO J038.1041+58.4796 20260531.3529 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 31.3529 2461191.8529 7.43 02:37:50.81 +57:54:16.4
136.70550 -2.09319 galactic Cas Second-epoch detections are separated by 0.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:37:50.81 +57:54:16.4: 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 02:37:50.81 +57:54:16.4: 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 31.3529* 02 37 50.81 +57 54 16.4 7.4 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 457950376842758784,2461191.8529,7.43,0.05,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 457950376842758784 20260531.3529 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 31.3529 2461191.8529 7.89 02:00:57.08 +58:36:59.1
131.89288 -3.04069 galactic Cas Second-epoch detections are separated by 0.7" and 3.6 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 02:00:57.08 +58:36:59.1: 12.64 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:57.08 +58:36:59.1: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 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 31.3529* 02 00 57.08 +58 36 59.1 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
V0924 Cas,2461191.8529,7.89,0.05,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
V0924 Cas 20260531.3529 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 31.3529 2461191.8529 9.40 01:28:36.14 +61:12:06.5
127.39384 -1.34757 galactic Cas Second-epoch detections are separated by 0.3" and 3.2 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 01:28:36.14 +61:12:06.5: 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 01:28:36.14 +61:12:06.5: 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 31.3529* 01 28 36.14 +61 12 06.5 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
PQ Cas,2461191.8529,9.40,0.05,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
PQ Cas 20260531.3529 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 31.3529 2461191.8529 9.10 01:20:18.33 +64:28:06.2
126.03725 1.77083 galactic Cas Second-epoch detections are separated by 0.7" and 2.9 pix
The object was found in VSX 1" 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 01:20:18.33 +64:28:06.2: 10.37 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:18.33 +64:28:06.2: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.93 +/- 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 31.3529* 01 20 18.33 +64 28 06.2 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
V0898 Cas,2461191.8529,9.10,0.05,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
V0898 Cas 20260531.3529 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 31.3529 2461191.8529 8.24 02:31:45.44 +55:57:58.0
136.69328 -4.20192 galactic Per Second-epoch detections are separated by 1.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9520+55.9630 | 02:31:46.12 +55:57:58.2 (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 02:31:45.44 +55:57:58.0: 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 02:31:45.44 +55:57:58.0: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.13 +/- 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 31.3529* 02 31 45.44 +55 57 58.0 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 J037.9520+55.9630,2461191.8529,8.24,0.05,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 J037.9520+55.9630 20260531.3529 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 31.3529 2461191.8529 9.26 01:31:04.82 +57:13:13.1
128.30114 -5.23760 galactic Cas Second-epoch detections are separated by 0.8" and 3.7 pix
The object was found in VSX 1" 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 01:31:04.82 +57:13:13.1: 11.31 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:04.82 +57:13:13.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.78 +/- 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 31.3529* 01 31 04.82 +57 13 13.1 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
NSVS J0131044+571311,2461191.8529,9.26,0.05,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
NSVS J0131044+571311 20260531.3529 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 31.3529 2461191.8529 9.12 02:03:07.50 +57:18:14.2
132.52660 -4.22631 galactic Per Second-epoch detections are separated by 1.0" and 3.6 pix
The object was found in VSX 1" 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 02:03:07.50 +57:18:14.2: 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 02:03:07.50 +57:18:14.2: 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 31.3529* 02 03 07.50 +57 18 14.2 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
ASASSN-V J020307.46+571813.2,2461191.8529,9.12,0.05,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
ASASSN-V J020307.46+571813.2 20260531.3529 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 31.3529 2461191.8529 8.54 02:33:23.80 +64:24:59.6
133.66428 3.69052 galactic Cas Second-epoch detections are separated by 0.3" and 2.9 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 02:33:23.80 +64:24:59.6: 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 02:33:23.80 +64:24:59.6: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 31.3529* 02 33 23.80 +64 24 59.6 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
V0940 Cas,2461191.8529,8.54,0.05,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
V0940 Cas 20260531.3529 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 31.3529 2461191.8529 9.76 01:45:16.04 +57:55:47.0
130.04902 -4.19627 galactic Cas Second-epoch detections are separated by 2.5" and 3.3 pix
The object was found in VSX 1" 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 01:45:16.04 +57:55:47.0: 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 01:45:16.04 +57:55:47.0: 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 31.3529* 01 45 16.04 +57 55 47.0 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 J014516.03+575546.6,2461191.8529,9.76,0.05,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 J014516.03+575546.6 20260531.3529 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 31.3529 2461191.8529 9.47 02:29:48.53 +57:57:49.9
135.69725 -2.44897 galactic Per Second-epoch detections are separated by 1.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 458091698450291584 | 02:29:48.78 +57:57:49.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A7V (LAMOST DR5) J-Ks=0.767+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:48.53 +57:57:49.9: 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 02:29:48.53 +57:57:49.9: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 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 31.3529* 02 29 48.53 +57 57 49.9 9.5 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
Large-amplitude variable Gaia DR2 458091698450291584,2461191.8529,9.47,0.05,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
Large-amplitude variable Gaia DR2 458091698450291584 20260531.3529 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 31.3529 2461191.8529 9.95 02:13:47.87 +63:11:26.2
132.06292 1.78829 galactic Cas Second-epoch detections are separated by 0.9" and 3.0 pix
The object was found in VSX 1" 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 02:13:47.87 +63:11:26.2: 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 02:13:47.87 +63:11:26.2: 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 31.3529* 02 13 47.87 +63 11 26.2 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 J0213478+631127,2461191.8529,9.95,0.05,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
NSVS J0213478+631127 20260531.3529 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 31.3529 2461191.8529 9.72 01:43:45.27 +58:23:44.4
129.75763 -3.78105 galactic Cas Second-epoch detections are separated by 1.1" and 3.7 pix
The object was found in VSX 0" 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 01:43:45.27 +58:23:44.4: 13.35 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:45.27 +58:23:44.4: 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 31.3529* 01 43 45.27 +58 23 44.4 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014345.26+582344.7,2461191.8529,9.72,0.05,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
ASASSN-V J014345.26+582344.7 20260531.3529 9.72CV 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 31.3529 2461191.8529 8.54 02:41:04.47 +62:17:31.2
135.29960 2.08233 galactic Cas Second-epoch detections are separated by 0.2" and 3.2 pix
The object was found in VSX 3" NSVS 1880848
Type: SR
# Max. Min./Amp. JD0 Period
14.260 g Y 0.662 g 2458430.18500 162.974687700000
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 02:41:04.47 +62:17:31.2: 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 02:41:04.47 +62:17:31.2: 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 31.3529* 02 41 04.47 +62 17 31.2 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
NSVS 1880848,2461191.8529,8.54,0.05,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 1880848 20260531.3529 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 31.3529 2461191.8529 8.41 02:30:52.96 +56:54:19.5
136.22657 -3.37726 galactic Per Second-epoch detections are separated by 0.3" and 3.8 pix
The object was found in VSX 0" 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 02:30:52.96 +56:54:19.5: 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 02:30:52.96 +56:54:19.5: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.09 +/- 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 31.3529* 02 30 52.96 +56 54 19.5 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 457978208232758784,2461191.8529,8.41,0.05,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
Gaia DR3 457978208232758784 20260531.3529 8.41CV 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 31.3529 2461191.8529 9.12 02:27:11.38 +56:07:26.5
136.04054 -4.29135 galactic Per Second-epoch detections are separated by 1.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457556270644732800 | 02:27:11.38 +56:07:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.323+/-0.026 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:11.38 +56:07:26.5: 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 02:27:11.38 +56:07:26.5: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 31.3529* 02 27 11.38 +56 07 26.5 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
Gaia DR3 457556270644732800,2461191.8529,9.12,0.05,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 457556270644732800 20260531.3529 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 31.3529 2461191.8529 9.83 02:31:31.09 +57:22:44.7
136.12827 -2.90593 galactic Per Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458018340407727104 | 02:31:29.87 +57:22:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3.5 1985ApJS...59..197B LTT 10837
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:31.09 +57:22:44.7: 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 02:31:31.09 +57:22:44.7: 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 31.3529* 02 31 31.09 +57 22 44.7 9.8 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 458018340407727104,2461191.8529,9.83,0.05,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
Gaia DR3 458018340407727104 20260531.3529 9.83CV 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 31.3529 2461191.8529 8.46 01:37:01.32 +61:15:57.4
128.38371 -1.12236 galactic Cas Second-epoch detections are separated by 0.1" and 3.2 pix
The object was found in VSX 1" 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 01:37:01.32 +61:15:57.4: 12.06 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:01.32 +61:15:57.4: 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 31.3529* 01 37 01.32 +61 15 57.4 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
V0910 Cas,2461191.8529,8.46,0.05,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
V0910 Cas 20260531.3529 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 31.3529 2461191.8529 9.05 02:18:22.53 +58:47:08.9
134.00426 -2.20439 galactic Per Second-epoch detections are separated by 0.8" and 3.5 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 02:18:22.53 +58:47:08.9: 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 02:18:22.53 +58:47:08.9: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 31.3529* 02 18 22.53 +58 47 08.9 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
NSVS J0218236+584716,2461191.8529,9.05,0.05,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
NSVS J0218236+584716 20260531.3529 9.05CV 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 31.3529 2461191.8529 8.82 02:28:34.52 +56:03:00.1
136.24808 -4.28979 galactic Per Second-epoch detections are separated by 1.9" and 4.0 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 457539743610843648 | 02:28:35.31 +56:03:02.1 (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 02:28:34.52 +56:03:00.1: 12.26 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:34.52 +56:03:00.1: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 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 31.3529* 02 28 34.52 +56 03 00.1 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 457539743610843648,2461191.8529,8.82,0.05,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 457539743610843648 20260531.3529 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 31.3529 2461191.8529 9.23 01:35:09.79 +60:17:09.4
128.32914 -2.12680 galactic Cas Second-epoch detections are separated by 1.2" and 3.4 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 01:35:09.79 +60:17:09.4: 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 01:35:09.79 +60:17:09.4: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 31.3529* 01 35 09.79 +60 17 09.4 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
Mis V0883,2461191.8529,9.23,0.05,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
Mis V0883 20260531.3529 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
## 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: 2461191.85308622 31.05.2026 08:28:16.649 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 139
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): 29645
Objects passed selection criteria: 29474
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 20089.8
Average stars matched: 19460.8 (96.8691 %)
Memory usage VmPeak: 132908 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 Sun May 31 04:37:03 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: 2461191.85308622 31.05.2026 08:28:16.649 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 820
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: 64 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): 201510
Objects passed selection criteria: 200913
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 136527
Average stars matched: 131369 (96.2222 %)
Memory usage VmPeak: 2022856 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 Sun May 31 04:46:12 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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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: 2461191.85262890
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cas-03-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_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits'
wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.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: 01:42:48.638 +61:56:55.73 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 01:42:48.638 +61:56:55.73
Angular distance between the image centers 0.0533 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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: 01:42:51.318 +61:56:57.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:51.318 +61:56:57.74
Angular distance between the image centers 0.0569 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 01:42:48.638 +61:56:55.73
Second-epoch second image center 01:42:51.318 +61:56:57.74
Angular distance between the image centers 0.00528 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.jNfWYWPcg7
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.eHaMdmBjBd
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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits &> /tmp/tmp.rFRGAIW7Ga
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits &> /tmp/tmp.XlccOkWzIZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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 123 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
3.6 pix fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
3.6 pix fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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
13.4 mag. fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
13.4 mag. fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jNfWYWPcg7 (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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/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.eHaMdmBjBd (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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/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.rFRGAIW7Ga (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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.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_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=555, passed=8796
Got 8796 stars (including 8238 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits.cat
util/solve_plate_with_UCAC5 got 8796 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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 8541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 8537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 8537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits N_match=967 sigma_overall_arcsec=0.414 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.430 sigma_q3_arcsec=0.368 sigma_q4_arcsec=0.415 n_q1=277 n_q2=312 n_q3=224 n_q4=154 worst_quadrant_to_overall_ratio=1.038
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits -region wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.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.XlccOkWzIZ (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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=562, passed=8825
Got 8825 stars (including 8260 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits.cat
util/solve_plate_with_UCAC5 got 8825 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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 8586 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 8585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 8574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 964 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits N_match=964 sigma_overall_arcsec=0.439 sigma_q1_arcsec=0.404 sigma_q2_arcsec=0.451 sigma_q3_arcsec=0.314 sigma_q4_arcsec=0.483 n_q1=276 n_q2=316 n_q3=222 n_q4=150 worst_quadrant_to_overall_ratio=1.101
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits -region wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits sigma_overall=0.414 worst_q_ratio=1.038
new2=fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits sigma_overall=0.439 worst_q_ratio=1.101
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_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334_astrometric_residuals.png (967 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335_astrometric_residuals.png (964 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-27-37_20.00sec_-0.00C_LIGHTs_0334.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_043345_TTUQ1b1x1_1940136_fIzAcEzW/wcs_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335.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 02:31:03.61 +56:50:28.3: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:17.93 +56:19:04.5: 13.26 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:03.61 +56:50:28.3: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:31:03.61 +56:50:28.3: 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 02:33:17.93 +56:19:04.5: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:33:17.93 +56:19:04.5: 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_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:45.01 +55:56:54.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:30.45 +56:11:02.1: 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 02:32:26.17 +56:41:41.4: 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 02:38:49.54 +57:35:29.4: 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 02:30:45.01 +55:56:54.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:30:45.01 +55:56:54.0: 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 02:29:09.13 +56:37:12.5: 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 02:25:27.60 +56:46:56.3: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:26.17 +56:41:41.4: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:32:26.17 +56:41:41.4: 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 02:32:05.01 +56:39:58.7: 15.61 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:30.45 +56:11:02.1: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:21:30.45 +56:11:02.1: 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 02:29:09.99 +56:27:11.9: 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 02:27:57.94 +56:02:37.6: 14.72 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:49.54 +57:35:29.4: 9.33 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:38:49.54 +57:35:29.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:27.60 +56:46:56.3: 9.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.64 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:27.60 +56:46:56.3: ref_mag=9.64 +/- 0.00 new_mean_mag=9.4601 delta=0.18 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:09.99 +56:27:11.9: 9.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.56 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:09.99 +56:27:11.9: ref_mag=9.56 +/- 0.00 new_mean_mag=9.5877 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:05.01 +56:39:58.7: 9.28 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:51.59 +57:23:36.6: 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 02:29:09.13 +56:37:12.5: 9.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.28 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:05.01 +56:39:58.7: ref_mag=9.28 +/- 0.00 new_mean_mag=9.4021 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 9.21 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:57.94 +56:02:37.6: 9.42 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:29:09.13 +56:37:12.5: ref_mag=9.21 +/- 0.00 new_mean_mag=9.3865 delta=-0.17 (need > 0.90)
Forced photometry reference-image weighted average: 9.42 +/- 0.00
Forced photometry filter REJECTED candidate at 02:27:57.94 +56:02:37.6: ref_mag=9.42 +/- 0.00 new_mean_mag=9.5192 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.69 +55:59:07.1: 14.30 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:10.20 +55:50:00.3: 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 02:37:25.13 +56:53:03.9: 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 02:34:30.13 +55:55:53.1: 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 02:31:25.69 +55:59:07.1: 9.46 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.46 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:25.69 +55:59:07.1: ref_mag=9.46 +/- 0.00 new_mean_mag=9.5745 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:10.20 +55:50:00.3: 9.50 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:34:10.20 +55:50:00.3: 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 02:37:25.13 +56:53:03.9: 9.68 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:37:25.13 +56:53:03.9: 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 02:38:51.59 +57:23:36.6: 9.50 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:38:51.59 +57:23:36.6: 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 02:32:46.00 +56:48:25.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:34.19 +56:21:55.3: 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 02:34:30.13 +55:55:53.1: 9.73 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:34:30.13 +55:55:53.1: 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 02:38:18.12 +57:14:06.8: 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 02:35:37.80 +57:29:13.3: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:24.37 +56:23:04.0: 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 02:32:46.00 +56:48:25.8: 9.55 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.55 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:34.19 +56:21:55.3: 9.58 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:32:46.00 +56:48:25.8: ref_mag=9.55 +/- 0.00 new_mean_mag=9.6796 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 9.58 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:34.19 +56:21:55.3: ref_mag=9.58 +/- 0.00 new_mean_mag=9.7058 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:18.12 +57:14:06.8: 9.78 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:38:18.12 +57:14:06.8: 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 02:34:43.99 +56:06:06.9: 14.00 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:11.83 +56:35:43.2: 10.93 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:53.66 +56:14:28.2: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:24.37 +56:23:04.0: 9.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.59 +/- 0.00
Forced photometry filter REJECTED candidate at 02:27:24.37 +56:23:04.0: ref_mag=9.59 +/- 0.00 new_mean_mag=9.7403 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:37.80 +57:29:13.3: 9.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.60 +/- 0.00
Forced photometry filter REJECTED candidate at 02:35:37.80 +57:29:13.3: ref_mag=9.60 +/- 0.00 new_mean_mag=9.6990 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:43.99 +56:06:06.9: 9.68 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.68 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:43.99 +56:06:06.9: ref_mag=9.68 +/- 0.00 new_mean_mag=9.7841 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:08.49 +57:25:21.6: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:11.83 +56:35:43.2: 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 02:30:53.66 +56:14:28.2: 9.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.85 +/- 0.00
Forced photometry filter REJECTED candidate at 02:24:11.83 +56:35:43.2: ref_mag=9.85 +/- 0.00 new_mean_mag=9.8694 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 9.93 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:53.66 +56:14:28.2: ref_mag=9.93 +/- 0.00 new_mean_mag=9.8101 delta=0.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:26.39 +56:06:42.2: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.27 +55:54:24.5: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:20.57 +56:01:48.3: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:08.49 +57:25:21.6: 9.91 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:13.34 +56:15:03.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 9.91 +/- 0.00
Forced photometry filter REJECTED candidate at 02:37:08.49 +57:25:21.6: ref_mag=9.91 +/- 0.00 new_mean_mag=9.9353 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.68 +56:07:05.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:28.41 +57:11:45.6: 14.95 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:11.89 +56:17:58.7: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:26.39 +56:06:42.2: 10.02 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.27 +55:54:24.5: 9.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.02 +/- 0.00
Forced photometry filter REJECTED candidate at 02:23:26.39 +56:06:42.2: ref_mag=10.02 +/- 0.00 new_mean_mag=10.0170 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 9.74 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:34.27 +55:54:24.5: ref_mag=9.74 +/- 0.00 new_mean_mag=9.8289 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:20.57 +56:01:48.3: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.11 +/- 0.00
Forced photometry filter REJECTED candidate at 02:27:20.57 +56:01:48.3: ref_mag=10.11 +/- 0.00 new_mean_mag=10.0431 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 02:34:05.22 +56:25:31.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:15.38 +56:38:50.2: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:13.34 +56:15:03.9: 9.92 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:35:13.34 +56:15:03.9: 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 02:31:25.68 +56:07:05.4: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.40 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:25.68 +56:07:05.4: ref_mag=10.40 +/- 0.00 new_mean_mag=10.1064 delta=0.29 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:28.41 +57:11:45.6: 9.84 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:11.89 +56:17:58.7: 10.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.84 +/- 0.00
Forced photometry filter REJECTED candidate at 02:36:28.41 +57:11:45.6: ref_mag=9.84 +/- 0.00 new_mean_mag=9.9333 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 10.17 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:11.89 +56:17:58.7: ref_mag=10.17 +/- 0.00 new_mean_mag=10.1386 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:44.95 +56:56:12.4: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:15.38 +56:38:50.2: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:15.38 +56:38:50.2: ref_mag=10.23 +/- 0.00 new_mean_mag=10.1628 delta=0.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.22 +56:25:31.7: 10.12 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.12 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:05.22 +56:25:31.7: ref_mag=10.12 +/- 0.00 new_mean_mag=10.1504 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:35.34 +56:18:13.8: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:59.14 +56:01:57.3: 14.29 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:48.89 +55:59:11.8: 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 02:32:55.19 +56:39:40.2: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:44.95 +56:56:12.4: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.11 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:44.95 +56:56:12.4: ref_mag=10.11 +/- 0.00 new_mean_mag=10.1892 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:59.14 +56:01:57.3: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.22 +/- 0.00
Forced photometry filter REJECTED candidate at 02:26:59.14 +56:01:57.3: ref_mag=10.22 +/- 0.00 new_mean_mag=10.2311 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 02:36:26.13 +56:17:10.9: 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 02:22:35.34 +56:18:13.8: 10.30 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:48.89 +55:59:11.8: 10.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 0.00
Forced photometry filter REJECTED candidate at 02:22:35.34 +56:18:13.8: ref_mag=10.30 +/- 0.00 new_mean_mag=10.2642 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 10.15 +/- 0.00
Forced photometry filter REJECTED candidate at 02:26:48.89 +55:59:11.8: ref_mag=10.15 +/- 0.00 new_mean_mag=10.2502 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:55.19 +56:39:40.2: 10.31 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.31 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:55.19 +56:39:40.2: ref_mag=10.31 +/- 0.00 new_mean_mag=10.3055 delta=0.00 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:01.81 +57:02:07.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:43.03 +56:42:23.5: 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 02:20:54.06 +56:16:37.4: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:26.13 +56:17:10.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 02:36:26.13 +56:17:10.9: 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 02:31:06.50 +56:30:41.6: 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 02:36:53.29 +56:34:44.5: 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 02:33:01.81 +57:02:07.5: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:01.81 +57:02:07.5: ref_mag=10.81 +/- 0.00 new_mean_mag=10.3415 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 02:36:43.03 +56:42:23.5: 10.34 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:36:43.03 +56:42:23.5: 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 02:37:55.04 +57:39:03.7: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:54.06 +56:16:37.4: 10.59 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:53.29 +56:34:44.5: 10.38 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:36:53.29 +56:34:44.5: 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: 10.59 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:06.86 +56:07:53.5: 15.75 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 02:20:54.06 +56:16:37.4: ref_mag=10.59 +/- 0.00 new_mean_mag=10.3259 delta=0.26 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:06.50 +56:30:41.6: 10.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:06.50 +56:30:41.6: ref_mag=10.38 +/- 0.00 new_mean_mag=10.3590 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:04.87 +56:49:24.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:55.04 +57:39:03.7: 10.47 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.47 +/- 0.00
Forced photometry filter REJECTED candidate at 02:37:55.04 +57:39:03.7: ref_mag=10.47 +/- 0.00 new_mean_mag=10.4144 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:06.86 +56:07:53.5: 10.48 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:03.56 +56:30:43.8: 15.66 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.48 +/- 0.00
Forced photometry filter REJECTED candidate at 02:22:06.86 +56:07:53.5: ref_mag=10.48 +/- 0.00 new_mean_mag=10.4238 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:28.00 +56:42:41.4: 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 02:30:12.40 +56:11:25.2: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:04.87 +56:49:24.8: 10.34 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:30.17 +55:56:58.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 10.34 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:04.87 +56:49:24.8: ref_mag=10.34 +/- 0.00 new_mean_mag=10.4817 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:03.56 +56:30:43.8: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:03.56 +56:30:43.8: ref_mag=10.30 +/- 0.00 new_mean_mag=10.4075 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:50.80 +56:20:49.0: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:28.00 +56:42:41.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 02:37:28.00 +56:42:41.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:48.50 +57:01:46.3: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:12.40 +56:11:25.2: 10.48 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.48 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:12.40 +56:11:25.2: ref_mag=10.48 +/- 0.00 new_mean_mag=10.4575 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:30.17 +55:56:58.7: 10.46 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:35:30.17 +55:56:58.7: 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 02:25:28.13 +56:11:20.6: 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 02:38:43.00 +57:29:15.9: 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 02:28:50.80 +56:20:49.0: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.58 +/- 0.00
Forced photometry filter REJECTED candidate at 02:28:50.80 +56:20:49.0: ref_mag=10.58 +/- 0.00 new_mean_mag=10.4707 delta=0.11 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:48.50 +57:01:46.3: 10.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:48.50 +57:01:46.3: ref_mag=10.43 +/- 0.00 new_mean_mag=10.4860 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:20.33 +56:12:13.9: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:28.13 +56:11:20.6: 10.37 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:43.00 +57:29:15.9: 10.56 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:38:43.00 +57:29:15.9: 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: 10.37 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:28.13 +56:11:20.6: ref_mag=10.37 +/- 0.00 new_mean_mag=10.4941 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:37.56 +56:33:36.2: 14.76 +/- 0.15 detection
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 +57:08:08.1: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:33.88 +57:09:19.3: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:19.75 +57:15:27.7: 15.72 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:32.11 +56:10:01.1: 15.55 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:37.56 +56:33:36.2: 10.72 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.72 +/- 0.00
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 +57:08:08.1: 10.52 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:31:37.56 +56:33:36.2: ref_mag=10.72 +/- 0.00 new_mean_mag=10.6385 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 10.52 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:45.29 +57:08:08.1: ref_mag=10.52 +/- 0.00 new_mean_mag=10.6034 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:20.33 +56:12:13.9: 10.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.44 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:20.33 +56:12:13.9: ref_mag=10.44 +/- 0.00 new_mean_mag=10.5270 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:42.79 +56:07:10.9: 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 02:35:33.88 +57:09:19.3: 10.86 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:51.94 +57:04:10.6: 15.74 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.86 +/- 0.00
Forced photometry filter REJECTED candidate at 02:35:33.88 +57:09:19.3: ref_mag=10.86 +/- 0.00 new_mean_mag=10.6621 delta=0.20 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:32.11 +56:10:01.1: 10.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.60 +/- 0.00
Forced photometry filter REJECTED candidate at 02:20:32.11 +56:10:01.1: ref_mag=10.60 +/- 0.00 new_mean_mag=10.6586 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:19.75 +57:15:27.7: 10.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.56 +/- 0.00
Forced photometry filter REJECTED candidate at 02:36:19.75 +57:15:27.7: ref_mag=10.56 +/- 0.00 new_mean_mag=10.6517 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:07.77 +56:33:53.8: 15.25 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:33.83 +56:34:21.9: 13.99 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:42.79 +56:07:10.9: 10.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.60 +/- 0.00
Forced photometry filter REJECTED candidate at 02:23:42.79 +56:07:10.9: ref_mag=10.60 +/- 0.00 new_mean_mag=10.6749 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:51.94 +57:04:10.6: 10.55 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.55 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:51.94 +57:04:10.6: ref_mag=10.55 +/- 0.00 new_mean_mag=10.6505 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:23.00 +56:25:37.2: 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 02:27:07.77 +56:33:53.8: 10.69 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:33.83 +56:34:21.9: 10.59 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:09.74 +56:34:02.8: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:38.41 +57:13:47.9: 12.02 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:18.32 +55:53:51.1: 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 02:37:31.61 +57:28:17.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:23.00 +56:25:37.2: 10.67 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:34.99 +57:36:36.4: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:33.22 +56:13:10.5: 13.50 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 02:36:23.00 +56:25:37.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 10.60 +/- 0.00
Forced photometry filter REJECTED candidate at 02:25:33.83 +56:34:21.9: ref_mag=10.60 +/- 0.00 new_mean_mag=10.6954 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 10.69 +/- 0.00
Forced photometry filter REJECTED candidate at 02:27:07.77 +56:33:53.8: ref_mag=10.69 +/- 0.00 new_mean_mag=10.6764 delta=0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:09.74 +56:34:02.8: 10.57 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:31.61 +57:28:17.6: 10.63 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:34.99 +57:36:36.4: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.32 +55:53:51.1: 10.81 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:38.41 +57:13:47.9: 10.65 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:24:09.74 +56:34:02.8: ref_mag=10.57 +/- 0.00 new_mean_mag=10.7062 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:33.22 +56:13:10.5: 10.62 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.67 +/- 0.00
Forced photometry filter REJECTED candidate at 02:37:31.61 +57:28:17.6: ref_mag=10.67 +/- 0.00 new_mean_mag=10.7467 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Forced photometry filter REJECTED candidate at 02:36:34.99 +57:36:36.4: ref_mag=10.70 +/- 0.00 new_mean_mag=10.8164 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 10.63 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:38.41 +57:13:47.9: ref_mag=10.77 +/- 0.00 new_mean_mag=10.6995 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:31:18.32 +55:53:51.1: ref_mag=10.81 +/- 0.00 new_mean_mag=10.7133 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:27:33.22 +56:13:10.5: ref_mag=10.63 +/- 0.00 new_mean_mag=10.7242 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:45.03 +56:57:37.7: 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 02:31:58.58 +56:42:23.1: 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 02:24:06.51 +56:29:60.0: 15.36 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:56.54 +57:06:44.8: 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 02:37:45.03 +56:57:37.7: 10.80 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:37:45.03 +56:57:37.7: 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 02:31:58.58 +56:42:23.1: 10.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.65 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:58.58 +56:42:23.1: ref_mag=10.65 +/- 0.00 new_mean_mag=10.7532 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:33.07 +56:53:09.5: 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 02:38:58.40 +57:47:39.9: 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 02:24:06.51 +56:29:60.0: 10.87 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:07.39 +56:25:11.6: 13.79 +/- 0.06 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Forced photometry filter REJECTED candidate at 02:24:06.51 +56:29:60.0: ref_mag=10.87 +/- 0.00 new_mean_mag=10.8117 delta=0.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:56.54 +57:06:44.8: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:18.20 +56:21:26.6: 15.66 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 02:36:56.54 +57:06:44.8: ref_mag=10.83 +/- 0.00 new_mean_mag=10.7807 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:32.66 +55:57:16.2: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:33.07 +56:53:09.5: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:33.07 +56:53:09.5: ref_mag=10.78 +/- 0.00 new_mean_mag=10.8838 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:07.39 +56:25:11.6: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:58.40 +57:47:39.9: 10.92 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:26:07.39 +56:25:11.6: ref_mag=10.83 +/- 0.00 new_mean_mag=10.8871 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:38:58.40 +57:47:39.9: 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 02:31:45.72 +56:26:45.8: 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 02:31:05.85 +56:37:18.3: 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 02:32:18.20 +56:21:26.6: 10.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.84 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:18.20 +56:21:26.6: ref_mag=10.84 +/- 0.00 new_mean_mag=10.8330 delta=0.00 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:18.81 +57:22:52.0: 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 02:29:32.66 +55:57:16.2: 10.94 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.94 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:32.66 +55:57:16.2: ref_mag=10.94 +/- 0.00 new_mean_mag=10.8694 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 02:37:48.04 +56:52:54.7: 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 02:31:45.47 +55:57:58.3: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:40.57 +56:18:39.3: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:45.72 +56:26:45.8: 10.77 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:18.81 +57:22:52.0: 10.88 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:38:18.81 +57:22:52.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:05.85 +56:37:18.3: 10.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:45.72 +56:26:45.8: ref_mag=10.77 +/- 0.00 new_mean_mag=10.8551 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 10.89 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:05.85 +56:37:18.3: ref_mag=10.89 +/- 0.00 new_mean_mag=10.9267 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:45.47 +55:57:58.3: 10.98 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:48.04 +56:52:54.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 10.98 +/- 0.01
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:40.57 +56:18:39.3: 10.85 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:37:48.04 +56:52:54.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry filter REJECTED candidate at 02:31:45.47 +55:57:58.3: ref_mag=10.98 +/- 0.01 new_mean_mag=10.9605 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 10.85 +/- 0.00
Forced photometry filter REJECTED candidate at 02:29:40.57 +56:18:39.3: ref_mag=10.85 +/- 0.00 new_mean_mag=10.9428 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.85 +57:54:16.6: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.10 +59:15:33.5: 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 02:37:50.85 +57:54:16.6: 9.93 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:56.63 +57:11:45.2: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.93 +/- 0.00
Forced photometry filter REJECTED candidate at 02:37:50.85 +57:54:16.6: ref_mag=9.93 +/- 0.00 new_mean_mag=10.0154 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:05.62 +56:37:26.3: 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 01:43:36.46 +58:48:08.4: 14.72 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.10 +59:15:33.5: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.10 +59:15:33.5: ref_mag=9.75 +/- 0.00 new_mean_mag=8.6822 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.62 +56:37:26.3: 9.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.61 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:56.63 +57:11:45.2: 10.65 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 02:34:05.62 +56:37:26.3: ref_mag=9.61 +/- 0.00 new_mean_mag=9.7460 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 11.01 +/- 0.01
Forced photometry filter REJECTED candidate at 02:22:56.63 +57:11:45.2: ref_mag=11.01 +/- 0.01 new_mean_mag=10.6966 delta=0.31 (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 +58:48:08.4: 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 +58:48:08.4: ref_mag=10.22 +/- 0.00 new_mean_mag=9.2915 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22210.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52187_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52187_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:30:04.73 +56:40:23.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52192_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52192_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:25:57.99 +56:06:10.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52193_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52193_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:22:56.82 +56:21:07.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52196_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52196_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:55.52 +56:35:49.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52197_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52197_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52198_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52198_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52200_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52200_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:24:41.64 +56:26:14.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52201_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52201_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:36:59.86 +63:08:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52205_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52205_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:21:10.33 +56:09:52.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52207_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52207_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:31:19.59 +56:53:52.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52214_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52214_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:25:59.00 +56:39:28.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52215_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52215_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:34:06.22 +57:00:24.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52219_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52219_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:23.51 +56:15:12.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52224_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52224_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:34:58.41 +55:58:55.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52225_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52225_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52226_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52226_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:33:24.12 +56:01:04.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52227_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52227_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52230_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52230_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52235_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52235_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52239_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52239_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52240_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52240_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52243_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52243_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52247_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52247_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52252_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52252_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52254_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52254_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:13.33 +56:42:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52258_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52258_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52260_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52260_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52261_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52261_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52262_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52262_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52266_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52266_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52267_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52267_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52270_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52270_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52271_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52271_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:56.86 +56:38:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52272_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52272_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52273_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52273_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52278_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52278_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52279_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52279_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52281_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52281_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:33.82 +56:48:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52286_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52286_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52289_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52289_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52290_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52290_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52292_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52292_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52296_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52296_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52299_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52299_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52302_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52302_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52308_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52308_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52310_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52310_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52314_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52314_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52315_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52315_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52319_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52319_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52320_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52320_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52323_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52323_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52326_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52326_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52328_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52328_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52335_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52335_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:32:00.01 +56:41:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52337_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52337_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52340_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52340_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:45.56 +56:46:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52344_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52344_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52345_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52345_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52351_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52351_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52352_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52352_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52353_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52353_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52355_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52355_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52356_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52356_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52358_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52358_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52360_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52360_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52366_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52366_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52368_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52368_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:54.19 +56:38:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52370_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52370_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52374_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52374_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:23.92 +56:37:52.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52379_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52379_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52383_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52383_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52384_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52384_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52385_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52385_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:23.07 +56:43:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52386_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52386_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52388_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52388_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52390_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52390_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:47.82 +56:36:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52392_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52392_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:55.27 +56:49:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52393_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52393_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52399_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52399_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52402_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52402_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52403_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52403_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52405_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52405_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52406_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52406_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52407_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52407_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52408_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52408_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52409_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52409_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52414_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52414_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52415_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52415_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52416_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52416_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52425_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52425_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52430_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52430_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52431_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52431_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52434_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52434_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52437_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52437_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52438_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52438_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52444_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52444_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52447_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52447_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52454_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52454_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52455_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52455_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52460_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52460_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52464_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52464_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:17.98 +56:48:58.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52465_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52465_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52468_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52468_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52470_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52470_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52471_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52471_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52475_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52475_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52479_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52479_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52484_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52484_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52485_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52485_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52488_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52488_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52489_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 52489_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20736_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 20736_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26424_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 26424_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:51:53.09 +57:12:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27684_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 27684_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:06:39.54 +56:51:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20109_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 20109_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51449_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 51449_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:30:27.42 +62:31:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25035_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 25035_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50065_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 50065_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23703_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 23703_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:54:53.98 +58:33:50.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22210_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 22210_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12304_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 12304_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:21:40.78 +60:54:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 08339_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:50:10.22 +63:07:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250667_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250667_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250668_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250668_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250675_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250675_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250676_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250676_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:55:14.43 +59:32:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250680_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250680_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250682_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250682_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:16:20.61 +62:42:26.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250685_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250685_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250687_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250687_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250688_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250688_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250689_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250689_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250691_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250691_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:25:15.96 +56:36:34.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250710_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250710_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:33:32.84 +57:32:16.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250711_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250711_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:22:54.20 +56:37:24.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250712_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250712_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:30:04.84 +56:40:23.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250716_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250716_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:38:37.97 +57:49:01.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250718_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250718_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:32:24.74 +57:25:44.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250719_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250719_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:25:57.97 +56:06:10.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250720_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250720_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:22:56.82 +56:21:07.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250722_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250722_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:32:52.75 +57:31:35.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250724_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250724_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:36:35.70 +57:43:13.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250725_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250725_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:30:02.52 +57:14:56.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250726_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250726_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:20:34.17 +56:19:48.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250727_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250727_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:55.51 +56:35:49.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250728_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250728_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250729_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250729_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:21.70 +57:05:22.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250731_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250731_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250732_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250732_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:24:41.64 +56:26:14.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250740_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250740_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250741_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250741_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:31:19.58 +56:53:52.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250743_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250743_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:21:10.33 +56:09:52.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250746_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250746_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:17:59.95 +56:13:54.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250747_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250747_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:16.23 +57:04:06.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250748_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250748_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:33:16.40 +57:14:04.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250752_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250752_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:34:06.21 +57:00:24.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250753_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250753_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:25:59.00 +56:39:28.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250754_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250754_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:36:13.68 +57:43:40.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250756_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250756_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:23.50 +56:15:12.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250757_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250757_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:48:46.89 +56:41:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250758_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250758_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:34:58.40 +55:58:55.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250761_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250761_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250762_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250762_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:20.62 +57:13:45.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250763_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250763_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:33:24.09 +56:01:04.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250766_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250766_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:21.93 +56:57:05.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250767_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250767_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:41.01 +57:11:21.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250768_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250768_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250769_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250769_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250776_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250776_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250779_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250779_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250782_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250782_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250785_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250785_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250786_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250786_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250792_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250792_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250794_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250794_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250795_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250795_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:13.32 +56:42:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250798_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250798_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250800_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250800_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250802_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250802_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250803_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250803_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250805_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250805_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250807_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250807_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250808_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250808_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250810_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250810_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250813_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250813_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250814_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250814_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:56.86 +56:38:22.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250816_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250816_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250819_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250819_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250820_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250820_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250823_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250823_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:33.82 +56:48:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250824_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250824_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250828_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250828_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250832_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250832_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:40.53 +57:05:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250833_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250833_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250835_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250835_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250836_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250836_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250838_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250838_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250842_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250842_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250844_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250844_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250848_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250848_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250851_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250851_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250852_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250852_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250853_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250853_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250855_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250855_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250856_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250856_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250857_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250857_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250862_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250862_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250865_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250865_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250866_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250866_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250867_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250867_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250870_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250870_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250873_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250873_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250875_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250875_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250878_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250878_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:03.03 +56:50:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250879_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250879_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250884_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250884_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250887_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250887_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250892_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250892_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250896_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250896_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250898_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250898_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:31:59.98 +56:41:12.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250899_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250899_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:45.55 +56:46:41.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250900_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250900_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250902_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250902_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:29.07 +56:54:17.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250903_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250903_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250909_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250909_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250910_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250910_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250911_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250911_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250912_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250912_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250913_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250913_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250916_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250916_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250918_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250918_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250919_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250919_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250921_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250921_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250923_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250923_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250924_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250924_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250926_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250926_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250927_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250927_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250930_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250930_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:54.18 +56:38:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250935_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250935_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250939_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250939_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250944_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250944_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250945_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250945_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250947_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250947_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250948_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250948_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250949_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250949_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:23.05 +56:43:45.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250950_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250950_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250951_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250951_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:23.92 +56:37:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250952_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250952_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250953_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250953_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250954_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250954_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250955_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250955_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:55.26 +56:49:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250957_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250957_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:47.81 +56:36:52.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250958_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250958_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250962_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250962_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250965_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250965_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250966_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250966_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250967_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250967_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250970_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250970_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250971_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250971_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250972_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250972_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250974_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250974_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250976_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250976_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250977_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 250977_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:18:49.57 +57:07:20.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250978_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250978_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250980_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250980_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250982_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250982_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250984_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250984_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250985_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250985_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250987_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250987_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250994_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250994_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250995_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250995_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250998_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 250998_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251001_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251001_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251007_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251007_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251010_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251010_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251012_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251012_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251013_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251013_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251015_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251015_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251017_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251017_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251018_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251018_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251019_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251019_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251020_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251020_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251026_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251026_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251029_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251029_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251038_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251038_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251041_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251041_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251043_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251043_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251044_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251044_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:46.34 +56:57:46.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251047_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251047_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251049_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251049_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251050_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251050_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251053_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251053_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:17.96 +56:48:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251054_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251054_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251055_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251055_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251057_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251057_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251060_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251060_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251063_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251063_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251065_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251065_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251068_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251068_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251070_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251070_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251071_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251071_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251077_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251077_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251078_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251078_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251080_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251080_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251082_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251082_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251085_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251085_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251087_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251087_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251089_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251089_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:49.05 +56:39:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251091_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251091_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251101_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251101_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251104_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251104_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251107_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251107_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251108_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251108_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251111_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251111_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251115_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251115_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251118_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251118_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251119_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251119_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:19.62 +56:49:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251122_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251122_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251125_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251125_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251126_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251126_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251132_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251132_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251133_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251133_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251134_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251134_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251135_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251135_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251138_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251138_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:26:41.02 +60:46:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251139_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251139_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251143_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251143_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251145_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251145_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251146_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251146_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251147_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251147_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251148_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251148_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251151_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251151_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:57.94 +56:42:03.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251153_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251153_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251154_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251154_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251156_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251156_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:44.66 +56:50:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251157_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251157_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251158_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251158_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251159_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251159_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251161_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251161_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251163_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251163_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251167_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251167_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251168_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251168_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251169_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251169_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251171_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251171_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251172_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251172_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251175_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251175_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251176_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251176_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:56.01 +56:44:03.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251178_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251178_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251179_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251179_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251180_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251180_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251184_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251184_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:45.88 +57:08:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251186_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251186_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251190_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251190_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251193_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251193_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251196_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251196_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251202_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251202_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251203_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251203_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:35.99 +56:56:28.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251209_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251209_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251210_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251210_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251213_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251213_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251214_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251214_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251215_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251215_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251220_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251220_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251222_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251222_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251227_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251227_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251228_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251228_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251229_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251229_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251233_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251233_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251236_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251236_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251238_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251238_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251240_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251240_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251242_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251242_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251244_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251244_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:01.15 +56:41:47.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251246_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251246_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251247_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251247_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251249_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251249_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251253_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251253_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251254_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251254_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251256_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251256_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251259_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251259_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:38.43 +57:12:51.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251260_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251260_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251261_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251261_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251262_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251262_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251269_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251269_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251274_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251274_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251280_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251280_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251285_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251285_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251287_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251287_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251290_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251290_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251292_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251292_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251293_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251293_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251299_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251299_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251300_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251300_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:04.29 +57:06:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251302_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251302_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251304_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251304_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251306_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251306_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251309_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251309_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251311_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251311_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251313_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251313_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251315_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251315_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251319_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251319_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251320_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251320_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251322_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251322_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251323_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251323_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251324_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251324_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:00.22 +56:46:14.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251325_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251325_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251328_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251328_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251333_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251333_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251334_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251334_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251337_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251337_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251338_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251338_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251339_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251339_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:43.52 +56:44:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251343_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251343_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:29.36 +56:57:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251344_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251344_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:58.97 +56:39:57.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251345_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251345_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251346_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251346_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251348_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251348_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:59.44 +56:50:11.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251349_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251349_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:30.31 +56:56:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251350_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251350_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251351_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251351_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251352_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251352_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251354_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251354_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251355_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251355_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251356_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251356_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:27.47 +56:51:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251358_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251358_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251359_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251359_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251361_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251361_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251363_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251363_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:56:38.48 +59:13:09.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251364_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251364_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251365_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251365_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251366_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251366_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:32:19.32 +56:13:29.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251368_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251368_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251378_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251378_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251379_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251379_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251381_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251381_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251384_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251384_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251386_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251386_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251387_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251387_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251393_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251393_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251394_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251394_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:56:21.78 +60:44:46.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251396_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251396_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251398_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251398_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251399_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251399_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251403_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251403_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251405_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251405_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251407_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251407_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251410_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251410_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:08:42.68 +58:16:29.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251415_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251415_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:50.14 +56:58:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251416_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251416_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251417_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251417_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251418_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251418_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:00.71 +57:00:32.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251419_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251419_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:49.77 +56:52:40.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251420_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251420_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251424_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251424_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:04.45 +56:59:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251425_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251425_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251427_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251427_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251431_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251431_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251433_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251433_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251436_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251436_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251439_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251439_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251440_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251440_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251445_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251445_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251448_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251448_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:45.23 +56:52:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251450_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251450_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251452_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251452_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251453_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251453_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251455_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251455_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251457_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251457_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251458_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251458_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251460_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251460_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251461_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251461_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251463_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251463_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:56.68 +56:52:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251465_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251465_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251468_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251468_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251469_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251469_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:56:24.86 +60:44:21.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251472_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251472_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251474_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251474_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251475_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251475_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251477_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251477_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251481_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251481_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:36.40 +56:40:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251482_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251482_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:53:16.25 +61:08:53.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251484_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251484_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251485_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251485_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251487_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251487_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251490_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251490_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251496_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251496_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251503_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251503_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251504_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251504_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:49:48.30 +65:05:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251509_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251509_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251512_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251512_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251516_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251516_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:22:06.22 +56:34:28.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251517_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251517_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:41.13 +57:07:20.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251518_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251518_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251524_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251524_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251527_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251527_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251533_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251533_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251534_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251534_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251536_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251536_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251537_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251537_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:03:46.98 +61:03:18.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251539_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251539_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:29.76 +56:55:48.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251541_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251541_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251542_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251542_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:33.46 +56:51:29.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251543_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251543_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251545_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251545_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251546_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251546_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:51:37.29 +63:46:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251550_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251550_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251552_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251552_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251553_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251553_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251557_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251557_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251558_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251558_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251559_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251559_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251560_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251560_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251561_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251561_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:38:00.52 +57:56:45.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251565_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251565_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251572_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251572_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251578_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251578_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:53:11.57 +61:05:57.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251579_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251579_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:22.53 +56:52:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251582_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251582_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251583_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251583_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251585_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251585_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251586_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251586_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251592_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251592_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251600_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251600_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251601_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251601_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:31:05.88 +56:49:41.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251604_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251604_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251606_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251606_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251614_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251614_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251615_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251615_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251617_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251617_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251627_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251627_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251631_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251631_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251632_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251632_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251633_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251633_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251638_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251638_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251640_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251640_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251642_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251642_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:19:12.08 +65:36:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251650_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251650_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251654_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251654_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251655_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251655_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251657_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251657_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251659_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251659_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251660_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251660_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251663_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251663_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251665_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251665_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251668_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251668_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:30.24 +57:10:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251672_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251672_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251673_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251673_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251677_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251677_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251678_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251678_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251682_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251682_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:06.21 +57:03:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251693_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251693_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251696_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251696_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251697_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251697_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251708_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251708_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251710_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251710_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251715_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251715_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251716_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251716_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251720_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251720_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251725_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251725_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:51:37.43 +62:56:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251726_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251726_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:42.81 +56:57:29.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251728_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251728_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251730_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251730_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251731_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251731_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251735_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251735_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251737_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251737_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251738_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251738_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:48.77 +56:43:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251739_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251739_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251740_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251740_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251745_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251745_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:06.65 +57:11:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251746_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251746_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251747_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251747_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251751_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251751_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251755_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251755_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251758_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251758_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251759_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251759_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251760_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251760_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251761_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251761_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:14.83 +56:44:21.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251763_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251763_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:17:59.25 +57:47:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251764_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251764_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251766_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251766_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251767_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251767_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251769_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251769_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251770_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251770_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251778_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251778_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251780_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251780_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251783_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251783_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251787_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251787_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251789_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251789_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251791_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251791_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251795_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251795_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251811_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251811_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251812_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251812_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251813_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251813_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251818_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251818_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251821_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251821_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251822_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251822_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251823_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251823_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251825_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251825_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251831_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251831_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251839_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251839_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251841_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251841_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251843_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251843_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251844_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251844_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251846_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251846_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251850_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251850_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:41:44.90 +65:51:11.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251851_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251851_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251852_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251852_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:54.16 +56:50:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251856_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251856_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251860_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251860_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251865_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251865_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251867_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251867_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251868_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251868_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251877_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251877_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:04.97 +56:40:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251878_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251878_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251880_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251880_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251883_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251883_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251889_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251889_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:21.05 +56:37:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251892_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251892_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251896_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251896_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251899_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251899_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251901_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251901_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251909_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251909_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251917_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251917_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:20.69 +56:44:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251922_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251922_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:32:45.76 +56:29:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251923_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251923_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251929_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251929_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251931_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251931_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251944_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251944_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:03:36.79 +61:03:01.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251948_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251948_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251949_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251949_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251951_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251951_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251957_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251957_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251958_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251958_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:26.72 +57:00:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251964_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251964_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:01.53 +57:00:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251971_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251971_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251972_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251972_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251976_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251976_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:16:47.39 +57:00:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251977_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251977_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251983_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251983_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251985_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 251985_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251988_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251988_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:25:08.31 +56:38:27.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251997_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 251997_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:35.90 +57:07:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252002_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252002_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252003_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252003_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252004_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252004_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252007_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252007_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252009_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252009_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252011_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252011_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252015_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252015_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252017_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252017_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:02:46.85 +64:22:58.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252019_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252019_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252041_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252041_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252042_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252042_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252046_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252046_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252052_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252052_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252054_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252054_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252055_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252055_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252063_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252063_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252064_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252064_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252066_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252066_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:12.43 +56:48:41.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252067_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252067_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252071_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252071_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252079_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252079_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252082_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252082_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252085_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252085_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252089_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252089_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252094_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252094_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:46:35.04 +59:33:37.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252097_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252097_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252098_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252098_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252102_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252102_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252105_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252105_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:38:06.27 +58:00:14.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252108_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252108_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252115_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252115_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252117_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252117_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:18:19.10 +57:42:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252119_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252119_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:05:03.84 +64:21:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252121_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252121_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252123_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252123_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:35:15.08 +63:00:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252125_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252125_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252130_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252130_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252131_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252131_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:28:30.91 +57:02:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252133_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252133_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252135_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252135_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252139_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252139_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:56:22.96 +59:10:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252142_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252142_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252149_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252149_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252151_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252151_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:04:16.45 +61:36:09.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252152_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252152_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252153_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252153_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252156_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252156_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252157_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252157_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252165_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252165_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252168_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252168_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252173_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252173_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252187_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252187_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252190_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252190_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252192_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252192_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252193_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252193_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252194_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252194_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252199_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252199_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252200_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252200_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:04:32.73 +57:59:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252202_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252202_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252203_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252203_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252205_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252205_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:57.27 +57:03:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252215_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252215_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252229_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252229_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252231_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252231_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252233_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252233_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252235_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252235_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252239_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252239_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252241_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252241_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:00:36.57 +63:32:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252246_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252246_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252252_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252252_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252253_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252253_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:31:04.21 +66:05:03.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252257_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252257_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252261_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252261_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252267_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252267_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252289_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252289_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252292_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252292_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252293_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252293_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252296_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252296_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252300_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252300_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252301_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252301_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252304_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252304_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:16:08.49 +58:49:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252305_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252305_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:40.95 +56:55:46.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252312_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252312_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252325_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252325_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252331_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252331_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252336_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252336_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:40:50.74 +64:17:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252345_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252345_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252346_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252346_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252356_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252356_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252367_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252367_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252386_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252386_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252401_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252401_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:58:01.11 +65:22:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252408_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252408_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252413_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252413_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252421_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252421_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252432_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252432_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:30:40.36 +56:40:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252435_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252435_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252437_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252437_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252447_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252447_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252453_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252453_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252460_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252460_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252473_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252473_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:02:54.90 +64:24:57.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252509_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252509_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:59:38.00 +62:54:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252521_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252521_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252525_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252525_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252534_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252534_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:41:56.00 +63:42:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252542_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252542_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:34.95 +57:15:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252597_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252597_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:16:12.70 +62:42:26.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252612_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 252612_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252617_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 252617_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221536_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 221536_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167698_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 167698_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189549_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 189549_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:31.03 +57:15:37.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219595_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 219595_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212460_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 212460_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104399_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 104399_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79932_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 79932_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208550_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 208550_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198104_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 198104_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211999_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 211999_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:51:53.08 +57:12:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64480_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 64480_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 214517_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 214517_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:06:39.51 +56:51:07.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67097_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 67097_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:36:59.86 +63:08:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190280_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 190280_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46105_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 46105_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:38:01.06 +63:01:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134840_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 134840_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154178_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 154178_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104143_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 104143_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:36:11.07 +60:22:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134816_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 134816_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 112593_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219961_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 219961_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159128_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 159128_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21138_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 21138_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:15:23.73 +65:01:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128710_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 128710_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:29:38.80 +60:38:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 72532_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:45:35.90 +63:07:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78295_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 78295_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188089_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 188089_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96282_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 96282_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165523_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 165523_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62860_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 62860_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:11:58.78 +63:39:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216016_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 216016_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162256_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 162256_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174355_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 174355_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179696_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 179696_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:57.32 +56:45:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192577_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 192577_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34359_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 34359_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:34:27.11 +64:32:52.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84648_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 84648_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177796_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 177796_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130602_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 130602_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221133_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 221133_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173124_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 173124_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213664_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 213664_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66586_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 66586_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169916_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 169916_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140285_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 140285_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236535_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 236535_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183189_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 183189_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157256_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 157256_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108178_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 108178_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:57:35.99 +61:28:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220143_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 220143_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184393_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 184393_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235853_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 235853_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131046_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 131046_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218015_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 218015_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235712_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 235712_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 70271_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:20:32.75 +62:32:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154238_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 154238_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185268_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 185268_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196494_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 196494_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173490_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 173490_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:22:51.60 +57:50:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217298_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 217298_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180134_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 180134_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155598_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 155598_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184872_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 184872_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:26:32.78 +57:05:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62555_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 62555_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168042_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 168042_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 39378_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:47:55.81 +64:32:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220590_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 220590_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213360_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 213360_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:37:01.83 +57:20:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152727_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 152727_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181535_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 181535_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201907_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 201907_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:43:36.46 +58:48:08.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162641_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 162641_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234311_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 234311_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182351_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 182351_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148907_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 148907_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157757_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 157757_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169994_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 169994_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233764_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 233764_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:29:12.48 +56:59:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115890_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 115890_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156692_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 156692_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:56:38.10 +59:15:33.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07627_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 07627_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:25:13.36 +65:50:10.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45963_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 45963_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213271_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 213271_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178813_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 178813_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:04:41.93 +57:30:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209662_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 209662_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193780_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 193780_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 00:54:53.94 +58:33:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173182_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 173182_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22840_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 22840_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63215_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 63215_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:30:27.41 +62:31:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180648_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 180648_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08809_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 08809_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:27:31.21 +65:38:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163824_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 163824_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58464_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 58464_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191949_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 191949_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60293_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 60293_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184455_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 184455_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 212570_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 212570_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195946_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 195946_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113819_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 113819_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104341_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 104341_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 02:40:39.00 +60:07:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153703_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 153703_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211642_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 211642_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92255_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
The candidate 92255_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335 did not pass the final checks
**** FOUND 01:00:48.61 +62:16:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137025_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
Preparing report for the candidate 137025_fd_Cas-03-Q1b1x1_2026-05-31_03-28-16_20.00sec_-0.00C_LIGHTs_0335
make_report_in_HTML.sh Phase 2 (HTML assembly): 33s
make_report_in_HTML.sh TOTAL: 1103s
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 ####
01:56:38.10 +59:15:33.5
01:43:36.46 +58:48:08.4
02:21:40.76 +60:54:41.6
01:21:54.72 +61:20:55.4
01:37:01.32 +61:15:57.4
01:28:36.14 +61:12:06.5
02:19:16.63 +59:42:21.5
01:30:50.27 +60:32:13.3
02:24:29.91 +59:24:30.8
02:38:02.15 +58:50:40.7
01:35:09.79 +60:17:09.4
01:16:28.98 +60:13:59.7
02:32:22.18 +58:28:54.4
01:14:56.64 +59:42:13.1
02:18:22.53 +58:47:08.9
02:34:36.31 +58:11:22.9
01:24:30.58 +59:38:48.3
02:38:48.25 +57:57:34.8
02:18:24.65 +58:37:26.1
02:37:50.81 +57:54:16.4
02:26:44.41 +58:15:51.9
02:08:53.89 +58:42:29.3
02:19:34.14 +58:23:58.2
02:29:48.53 +57:57:49.9
01:41:46.90 +59:03:47.3
02:33:40.20 +57:40:02.4
01:09:38.04 +59:05:14.4
02:33:31.89 +57:34:08.3
02:00:57.08 +58:36:59.1
02:17:01.69 +56:56:08.6
02:03:07.50 +57:18:14.2
02:31:45.72 +56:26:45.7
02:31:42.43 +56:35:52.7
02:34:05.60 +56:37:26.3
01:45:16.04 +57:55:47.0
02:21:35.99 +57:03:40.3
02:31:32.42 +56:47:58.9
02:13:41.76 +57:25:36.7
02:22:56.62 +57:11:45.0
02:30:52.96 +56:54:19.5
02:21:26.44 +57:16:58.2
02:29:19.57 +57:07:07.2
02:29:57.73 +57:10:58.0
01:43:45.27 +58:23:44.4
02:33:34.77 +57:08:54.4
02:31:31.09 +57:22:44.7
02:01:28.14 +58:18:14.4
02:05:05.69 +58:16:23.9
02:15:35.89 +56:21:36.7
01:31:04.82 +57:13:13.1
02:28:34.52 +56:03:00.1
01:31:28.05 +57:20:36.4
02:27:11.38 +56:07:26.5
02:31:45.44 +55:57:58.0
02:19:48.16 +56:25:08.9
02:14:24.94 +56:42:49.3
02:29:59.54 +56:13:01.3
02:34:12.69 +56:03:50.1
02:17:19.11 +56:42:44.0
02:25:13.36 +56:30:31.4
02:33:51.42 +56:10:59.9
02:27:55.40 +56:27:24.2
02:29:16.20 +56:24:33.1
02:31:18.55 +56:20:48.9
02:33:23.80 +64:24:59.6
02:29:46.25 +56:03:50.4
02:27:27.68 +56:03:05.8
02:28:27.94 +57:25:38.4
00:30:33.64 +66:05:36.8
01:37:22.21 +59:19:56.8
02:09:05.47 +57:29:28.7
02:25:12.14 +58:09:07.0
00:42:45.77 +63:38:26.5
02:37:27.18 +57:28:29.8
00:36:55.27 +62:40:47.8
02:19:45.14 +57:01:17.6
02:29:09.11 +56:37:12.5
02:25:27.59 +56:46:56.3
02:32:05.00 +56:39:58.8
02:32:34.50 +57:29:15.5
02:27:57.93 +56:02:37.4
02:29:09.98 +56:27:11.8
02:31:25.66 +55:59:07.0
02:22:03.80 +56:31:26.9
02:34:10.16 +55:50:00.1
02:32:46.00 +56:48:25.9
02:34:34.19 +56:21:55.6
02:35:37.81 +57:29:13.2
02:25:20.43 +56:51:13.3
02:34:43.96 +56:06:06.8
02:27:24.36 +56:23:03.8
02:30:53.64 +56:14:28.0
02:33:34.24 +55:54:24.4
02:24:11.84 +56:35:43.1
02:23:35.43 +56:34:27.3
02:37:08.47 +57:25:21.7
02:36:28.42 +57:11:45.9
02:35:52.02 +57:47:22.1
02:23:26.39 +56:06:42.0
02:36:33.26 +57:54:38.3
02:27:20.56 +56:01:48.1
02:36:36.25 +57:46:59.1
02:18:01.27 +56:15:42.4
02:32:05.68 +57:22:03.0
02:19:46.66 +56:22:25.8
02:34:05.22 +56:25:31.7
02:21:55.21 +56:25:08.8
02:29:11.88 +56:17:58.5
02:31:25.67 +56:07:05.3
02:32:15.38 +56:38:50.2
02:30:44.93 +56:56:12.3
02:21:50.35 +56:34:31.6
02:26:59.12 +56:01:57.0
02:22:35.34 +56:18:13.6
02:26:48.88 +55:59:11.6
02:32:55.20 +56:39:40.1
02:33:01.81 +57:02:07.5
02:20:54.06 +56:16:37.3
02:31:06.51 +56:30:41.5
02:24:43.69 +56:59:33.9
02:38:46.64 +57:49:57.9
02:37:36.83 +57:51:16.3
02:37:55.04 +57:39:03.5
02:22:06.87 +56:07:53.3
02:34:03.56 +56:30:43.8
02:21:20.56 +56:29:12.2
02:32:04.85 +56:49:24.8
02:30:12.39 +56:11:25.0
02:22:10.20 +56:24:23.0
02:27:48.50 +57:05:55.4
02:28:50.78 +56:20:48.8
02:33:48.46 +57:01:46.2
02:19:52.94 +56:15:40.6
02:25:28.14 +56:11:20.3
02:33:49.33 +57:35:12.0
02:19:48.61 +56:23:45.8
02:25:20.33 +56:12:13.7
02:24:41.99 +56:55:48.0
02:31:11.98 +57:09:48.2
02:19:36.43 +56:14:20.7
02:18:48.83 +56:19:01.6
02:32:45.28 +57:08:07.9
02:18:48.46 +56:17:54.5
02:35:33.89 +57:09:19.1
02:36:19.72 +57:15:27.8
02:31:37.57 +56:33:36.1
02:27:07.76 +56:33:53.6
02:30:51.92 +57:04:10.4
02:23:42.80 +56:07:10.6
02:20:32.12 +56:10:01.0
02:24:09.75 +56:34:02.5
02:25:33.83 +56:34:21.8
02:35:18.49 +57:31:39.8
02:20:55.01 +56:23:18.7
02:33:30.04 +57:42:18.6
02:31:18.30 +55:53:50.8
02:31:38.41 +57:13:47.7
02:27:33.21 +56:13:10.2
02:36:35.00 +57:36:36.2
02:22:04.44 +57:10:39.1
02:31:58.58 +56:42:23.0
02:29:17.15 +57:14:29.9
02:36:56.54 +57:06:44.6
02:24:06.51 +56:29:59.7
02:24:33.48 +56:57:19.3
02:32:18.19 +56:21:26.4
02:19:39.63 +56:20:11.7
02:30:32.08 +57:11:25.7
02:26:13.32 +56:36:46.9
02:30:33.06 +56:53:09.3
02:35:20.15 +57:29:29.6
02:26:07.39 +56:25:11.4
02:30:00.36 +57:28:19.5
02:29:32.65 +55:57:16.0
02:31:05.86 +56:37:18.2
02:24:32.58 +57:00:45.4
02:19:56.59 +56:13:25.6
02:36:08.58 +57:39:34.6
02:29:40.57 +56:18:39.2
02:30:37.28 +56:22:56.7
02:31:20.20 +57:33:46.6
02:30:49.36 +56:11:02.6
02:34:28.42 +56:22:24.6
02:24:18.90 +56:54:02.0
02:29:50.49 +56:19:09.0
02:29:40.82 +56:20:03.6
02:25:00.79 +56:51:32.4
02:32:13.87 +55:56:23.6
02:29:28.33 +56:33:05.7
02:28:09.55 +56:10:49.3
02:33:09.16 +57:00:38.4
02:21:04.80 +56:15:33.0
02:37:41.06 +57:33:22.4
02:28:48.94 +56:07:35.3
02:21:59.12 +56:30:01.8
02:30:30.77 +57:30:27.1
02:22:31.56 +56:14:11.4
02:34:25.96 +56:29:13.8
02:33:33.86 +56:11:46.9
02:35:42.45 +56:44:19.0
02:16:48.70 +56:16:11.9
02:36:22.60 +57:40:05.9
02:23:48.04 +56:47:01.7
02:26:10.78 +56:48:29.0
02:35:30.16 +57:03:30.3
02:18:23.94 +56:23:20.9
02:26:55.66 +56:30:19.4
02:25:03.10 +56:56:58.5
02:23:02.10 +56:30:28.6
02:33:05.09 +56:13:01.1
02:37:50.53 +57:45:50.6
02:35:28.70 +56:28:21.1
02:32:25.76 +56:47:11.8
02:31:09.67 +57:16:15.4
02:34:12.78 +56:12:36.7
02:26:43.12 +56:24:13.3
02:34:04.55 +56:42:30.3
02:23:17.87 +56:42:24.1
02:25:55.90 +56:58:59.9
02:27:59.47 +56:29:43.8
02:25:48.33 +56:55:12.6
02:29:58.05 +56:08:50.3
02:33:40.64 +57:26:09.7
02:35:08.68 +57:36:15.0
02:34:48.58 +57:38:04.9
02:30:03.56 +56:22:32.1
02:32:59.21 +57:28:34.1
02:28:57.12 +57:06:16.3
02:30:18.83 +55:54:55.5
02:19:36.34 +56:23:22.7
02:31:29.13 +57:11:55.8
02:30:59.05 +56:08:44.3
02:16:52.45 +56:18:44.9
02:31:00.03 +56:00:28.9
02:32:17.76 +57:17:09.4
02:26:11.61 +56:56:03.9
02:34:43.40 +56:34:06.2
02:21:34.57 +56:26:43.6
02:36:59.39 +57:56:28.2
02:35:04.69 +57:26:54.1
02:37:50.74 +57:57:57.3
02:33:03.17 +57:03:28.2
02:38:18.06 +57:37:36.9
02:36:07.69 +57:21:39.9
02:20:18.71 +56:31:49.9
02:37:26.82 +58:01:13.3
02:34:24.38 +57:28:25.9
02:28:34.73 +56:13:02.0
02:38:13.41 +57:50:16.7
02:24:01.97 +56:49:23.4
02:33:33.49 +55:49:25.7
02:27:23.30 +55:57:43.1
02:33:10.54 +57:32:53.9
02:37:30.47 +57:39:32.1
02:28:31.63 +56:00:35.4
02:24:33.99 +56:52:59.9
02:25:56.77 +56:07:50.4
02:18:05.16 +56:15:08.3
02:29:57.46 +56:36:50.9
02:35:47.68 +57:10:24.3
02:28:48.14 +56:30:08.1
02:20:07.37 +56:27:51.6
02:25:04.18 +56:13:07.6
02:31:11.42 +56:38:16.1
02:34:12.55 +56:11:53.5
02:25:45.47 +56:26:30.9
02:26:15.74 +56:04:34.8
02:31:02.85 +57:39:55.6
02:37:02.13 +57:41:38.8
02:23:55.69 +56:44:44.9
02:30:39.36 +57:13:43.1
02:31:10.50 +57:30:48.1
02:29:26.52 +56:00:56.6
02:31:29.40 +56:26:22.3
02:33:48.37 +56:47:59.7
02:33:43.66 +57:36:01.4
02:34:13.61 +56:18:42.4
02:29:38.97 +56:11:32.5
02:30:43.84 +55:58:10.7
02:26:00.85 +56:46:18.6
02:27:59.54 +56:09:19.1
02:30:51.75 +57:15:44.4
02:21:55.10 +56:20:50.0
02:31:12.59 +57:00:49.8
02:26:08.81 +56:16:07.7
02:30:41.06 +55:56:25.5
02:35:00.16 +56:43:10.4
02:24:32.07 +56:43:35.5
02:32:18.81 +56:15:24.2
02:30:17.06 +56:38:11.7
02:23:38.16 +56:39:53.3
02:24:25.95 +56:32:57.3
02:28:40.95 +56:12:03.5
02:28:21.40 +55:58:55.7
02:33:50.71 +55:59:56.9
02:31:51.47 +56:45:50.3
02:31:03.02 +55:52:01.4
02:35:12.95 +57:56:23.8
02:30:23.25 +56:23:34.2
02:37:31.30 +57:29:01.8
02:24:47.85 +56:36:57.7
02:34:03.05 +56:00:36.1
02:26:59.37 +57:14:45.3
02:33:48.54 +55:57:07.4
02:33:37.62 +57:40:24.0
02:24:38.05 +56:49:55.5
02:24:18.80 +56:19:50.2
02:37:24.10 +57:31:04.5
02:32:35.10 +57:32:19.9
02:28:56.59 +56:11:02.8
02:25:30.05 +56:16:52.2
02:26:02.34 +56:21:00.8
02:27:34.54 +56:16:51.2
02:33:57.28 +57:00:01.2
02:25:48.44 +56:32:34.9
02:32:31.36 +57:38:51.5
02:29:55.76 +56:55:49.8
02:25:32.72 +56:32:56.9
02:32:23.05 +57:38:37.3
02:27:37.42 +57:04:56.0
02:33:44.26 +56:59:33.8
02:27:52.24 +56:29:30.2
02:38:39.71 +57:47:02.7
02:25:11.61 +56:17:21.6
02:30:00.33 +57:11:29.3
02:33:42.17 +55:51:19.1
02:32:49.37 +57:34:23.1
02:30:32.60 +57:32:13.7
02:30:00.36 +56:17:43.0
02:35:26.59 +57:46:13.0
02:30:38.21 +56:11:54.0
02:36:19.07 +57:07:02.5
02:36:27.53 +56:56:51.3
02:23:11.07 +56:11:20.3
02:22:11.90 +56:20:47.6
02:29:10.75 +55:58:47.7
02:30:45.38 +57:06:30.4
02:36:19.41 +57:59:11.1
02:33:28.12 +56:18:30.6
02:27:07.63 +56:00:29.5
02:34:32.01 +57:40:32.0
02:24:52.39 +56:43:11.8
02:23:08.55 +56:20:25.7
02:30:28.93 +56:19:35.0
02:34:13.74 +56:19:38.4
02:29:11.14 +57:21:01.2
02:36:41.43 +57:37:08.6
02:22:47.61 +56:11:10.3
02:24:38.48 +56:20:47.1
02:32:04.85 +56:53:51.0
02:27:42.05 +56:12:16.6
02:30:07.04 +56:30:20.7
02:23:56.97 +56:11:52.3
02:27:15.92 +56:00:28.3
02:32:37.22 +56:00:39.6
01:40:01.01 +60:52:39.3
02:22:16.01 +56:22:42.1
02:23:07.52 +56:41:45.7
02:34:09.36 +56:41:02.1
02:31:19.74 +56:52:40.3
02:31:43.43 +56:14:45.0
02:32:47.60 +57:14:18.6
02:34:34.57 +56:36:40.8
02:30:33.43 +56:57:01.0
02:25:42.16 +56:37:12.1
02:30:34.92 +56:43:56.7
02:21:32.88 +56:13:40.8
02:33:38.50 +57:33:38.4
02:37:15.56 +57:48:20.7
02:33:30.70 +57:29:01.5
02:36:49.05 +57:24:45.7
02:32:30.78 +56:47:59.9
02:31:46.58 +55:52:30.0
02:36:54.41 +57:53:40.3
02:21:27.45 +56:16:27.4
02:35:12.35 +56:50:10.1
02:32:01.35 +56:51:17.4
02:29:43.00 +56:05:10.4
02:39:58.30 +58:20:59.8
02:33:30.84 +56:43:01.0
02:35:15.88 +56:26:19.4
02:27:22.97 +56:19:27.7
02:30:05.86 +57:18:33.7
02:37:01.21 +57:51:23.9
02:34:37.56 +56:32:35.4
02:34:22.33 +56:20:27.4
02:28:01.24 +56:23:31.7
02:36:42.69 +57:08:11.5
02:33:57.90 +56:36:42.0
02:20:11.66 +56:22:21.1
02:33:11.61 +57:36:40.3
02:21:23.02 +56:39:00.5
02:35:22.14 +56:48:52.6
02:24:12.37 +56:49:24.7
02:32:55.55 +57:08:54.8
02:27:53.50 +57:06:30.2
02:37:38.82 +57:43:26.3
02:34:43.58 +56:51:49.8
02:36:55.85 +57:38:50.5
02:33:06.29 +56:00:32.4
02:33:08.16 +57:28:10.9
02:33:23.59 +57:33:31.5
02:27:27.08 +56:31:12.3
02:25:52.68 +56:47:30.2
02:25:40.02 +56:29:21.1
02:22:21.44 +56:34:17.9
02:24:46.71 +56:38:57.2
02:21:16.35 +56:23:42.9
02:24:53.85 +56:08:46.7
02:28:10.62 +56:06:42.3
02:35:35.04 +57:33:01.8
02:29:33.78 +56:09:10.9
02:34:04.23 +57:32:43.7
02:30:51.32 +57:16:48.9
02:21:13.42 +56:28:43.4
02:29:38.91 +56:20:56.3
02:32:49.88 +56:14:34.7
01:25:31.68 +57:37:40.0
02:35:41.88 +57:31:41.5
02:30:42.09 +57:22:37.0
02:31:45.76 +57:14:33.8
02:34:19.68 +57:08:34.6
02:37:47.00 +58:07:12.4
02:29:29.31 +57:10:38.0
02:33:27.53 +57:14:42.7
02:39:23.81 +58:09:08.6
02:25:53.36 +56:14:37.1
02:31:12.55 +56:27:35.9
02:27:22.07 +56:31:21.0
02:25:52.25 +57:02:03.7
02:29:04.86 +57:22:34.6
02:34:06.59 +56:06:19.6
02:25:56.52 +56:32:32.5
02:21:19.11 +56:38:13.7
02:39:21.43 +58:07:09.6
02:28:31.02 +56:40:25.2
02:23:08.48 +56:55:24.7
02:38:14.36 +57:58:52.1
02:31:54.47 +55:50:24.1
02:34:32.89 +57:07:24.9
02:21:52.35 +56:32:44.4
02:26:14.36 +56:12:10.7
02:34:18.24 +57:49:31.9
02:29:41.72 +56:37:30.4
02:30:58.42 +57:16:18.4
02:36:12.12 +57:41:55.7
02:26:01.05 +56:28:14.9
02:22:37.96 +56:37:19.4
02:24:27.17 +56:50:29.3
02:36:52.73 +57:40:54.2
00:58:55.95 +58:04:06.6
02:34:27.71 +56:43:27.0
02:30:09.40 +57:23:13.6
02:29:02.18 +56:24:16.8
02:30:26.89 +56:10:14.6
02:32:42.22 +57:14:26.4
02:36:28.05 +56:50:31.6
02:33:18.04 +57:31:36.2
02:31:18.63 +57:03:51.6
02:36:19.82 +56:57:28.2
02:29:25.42 +55:58:54.2
02:36:18.15 +56:52:17.8
02:34:42.56 +57:17:57.3
02:26:58.18 +56:22:09.7
02:34:40.76 +56:11:02.3
02:33:07.75 +56:14:50.5
02:36:19.79 +57:18:00.4
02:27:40.45 +56:20:28.8
02:23:42.90 +56:38:37.4
02:22:22.76 +56:39:59.4
02:30:38.78 +56:15:14.6
02:33:02.03 +56:26:23.4
00:43:47.73 +61:54:01.0
02:18:56.11 +56:18:31.6
02:33:25.63 +56:59:44.8
02:37:55.66 +58:18:21.1
02:38:07.48 +58:00:10.7
02:26:55.93 +56:28:27.3
02:32:05.93 +57:04:59.5
01:18:14.25 +61:44:36.4
02:33:01.80 +57:36:06.2
02:30:49.71 +56:26:27.4
02:28:42.38 +55:58:14.1
02:31:52.59 +56:53:47.2
02:37:59.24 +58:07:39.6
02:27:44.77 +56:19:42.5
02:33:08.38 +57:21:21.6
02:38:19.80 +58:03:54.5
02:35:58.83 +57:31:57.8
01:29:32.82 +61:46:26.3
02:35:43.57 +57:50:30.9
02:29:48.85 +56:41:55.4
01:22:23.81 +61:13:50.8
01:20:18.33 +64:28:06.2
02:13:47.87 +63:11:26.2
02:41:04.47 +62:17:31.2
02:27:22.20 +62:38:25.9
02:19:03.87 +62:47:34.5
02:15:26.96 +62:47:45.2
02:15:20.33 +62:13:49.2
01:32:51.45 +62:40:36.3
01:27:44.31 +62:06:39.9
########### 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 ####
01:56:38.10 +59:15:33.5
01:43:36.46 +58:48:08.4
00:30:33.64 +66:05:36.8
01:37:22.21 +59:19:56.8
02:09:05.47 +57:29:28.7
02:25:12.14 +58:09:07.0
00:42:45.77 +63:38:26.5
02:37:27.18 +57:28:29.8
00:36:55.27 +62:40:47.8
02:19:45.14 +57:01:17.6
02:29:09.11 +56:37:12.5
02:25:27.59 +56:46:56.3
02:32:05.00 +56:39:58.8
02:32:34.50 +57:29:15.5
02:27:57.93 +56:02:37.4
02:29:09.98 +56:27:11.8
02:31:25.66 +55:59:07.0
02:22:03.80 +56:31:26.9
02:34:10.16 +55:50:00.1
02:32:46.00 +56:48:25.9
02:34:34.19 +56:21:55.6
02:35:37.81 +57:29:13.2
02:25:20.43 +56:51:13.3
02:34:43.96 +56:06:06.8
02:27:24.36 +56:23:03.8
02:30:53.64 +56:14:28.0
02:33:34.24 +55:54:24.4
02:24:11.84 +56:35:43.1
02:23:35.43 +56:34:27.3
02:37:08.47 +57:25:21.7
02:36:28.42 +57:11:45.9
02:35:52.02 +57:47:22.1
02:23:26.39 +56:06:42.0
02:36:33.26 +57:54:38.3
02:27:20.56 +56:01:48.1
02:36:36.25 +57:46:59.1
02:18:01.27 +56:15:42.4
02:32:05.68 +57:22:03.0
02:19:46.66 +56:22:25.8
02:34:05.22 +56:25:31.7
02:21:55.21 +56:25:08.8
02:29:11.88 +56:17:58.5
02:31:25.67 +56:07:05.3
02:32:15.38 +56:38:50.2
02:30:44.93 +56:56:12.3
02:21:50.35 +56:34:31.6
02:26:59.12 +56:01:57.0
02:22:35.34 +56:18:13.6
02:26:48.88 +55:59:11.6
02:32:55.20 +56:39:40.1
02:33:01.81 +57:02:07.5
02:20:54.06 +56:16:37.3
02:31:06.51 +56:30:41.5
02:24:43.69 +56:59:33.9
02:38:46.64 +57:49:57.9
02:37:36.83 +57:51:16.3
02:37:55.04 +57:39:03.5
02:22:06.87 +56:07:53.3
02:34:03.56 +56:30:43.8
02:21:20.56 +56:29:12.2
02:32:04.85 +56:49:24.8
02:30:12.39 +56:11:25.0
02:22:10.20 +56:24:23.0
02:27:48.50 +57:05:55.4
02:28:50.78 +56:20:48.8
02:33:48.46 +57:01:46.2
02:19:52.94 +56:15:40.6
02:25:28.14 +56:11:20.3
02:33:49.33 +57:35:12.0
02:19:48.61 +56:23:45.8
02:25:20.33 +56:12:13.7
02:24:41.99 +56:55:48.0
02:31:11.98 +57:09:48.2
02:19:36.43 +56:14:20.7
02:18:48.83 +56:19:01.6
02:32:45.28 +57:08:07.9
02:18:48.46 +56:17:54.5
02:35:33.89 +57:09:19.1
02:36:19.72 +57:15:27.8
02:31:37.57 +56:33:36.1
02:27:07.76 +56:33:53.6
02:30:51.92 +57:04:10.4
02:23:42.80 +56:07:10.6
02:20:32.12 +56:10:01.0
02:24:09.75 +56:34:02.5
02:25:33.83 +56:34:21.8
02:35:18.49 +57:31:39.8
02:20:55.01 +56:23:18.7
02:33:30.04 +57:42:18.6
02:31:18.30 +55:53:50.8
02:31:38.41 +57:13:47.7
02:27:33.21 +56:13:10.2
02:36:35.00 +57:36:36.2
02:22:04.44 +57:10:39.1
02:31:58.58 +56:42:23.0
02:29:17.15 +57:14:29.9
02:36:56.54 +57:06:44.6
02:24:06.51 +56:29:59.7
02:24:33.48 +56:57:19.3
02:32:18.19 +56:21:26.4
02:19:39.63 +56:20:11.7
02:30:32.08 +57:11:25.7
02:26:13.32 +56:36:46.9
02:30:33.06 +56:53:09.3
02:35:20.15 +57:29:29.6
02:26:07.39 +56:25:11.4
02:30:00.36 +57:28:19.5
02:29:32.65 +55:57:16.0
02:31:05.86 +56:37:18.2
02:24:32.58 +57:00:45.4
02:19:56.59 +56:13:25.6
02:36:08.58 +57:39:34.6
02:29:40.57 +56:18:39.2
02:30:37.28 +56:22:56.7
02:31:20.20 +57:33:46.6
02:30:49.36 +56:11:02.6
02:34:28.42 +56:22:24.6
02:24:18.90 +56:54:02.0
02:29:50.49 +56:19:09.0
02:29:40.82 +56:20:03.6
02:25:00.79 +56:51:32.4
02:32:13.87 +55:56:23.6
02:29:28.33 +56:33:05.7
02:28:09.55 +56:10:49.3
02:33:09.16 +57:00:38.4
02:21:04.80 +56:15:33.0
02:37:41.06 +57:33:22.4
02:28:48.94 +56:07:35.3
02:21:59.12 +56:30:01.8
02:30:30.77 +57:30:27.1
02:22:31.56 +56:14:11.4
02:34:25.96 +56:29:13.8
02:33:33.86 +56:11:46.9
02:35:42.45 +56:44:19.0
02:16:48.70 +56:16:11.9
02:36:22.60 +57:40:05.9
02:23:48.04 +56:47:01.7
02:26:10.78 +56:48:29.0
02:35:30.16 +57:03:30.3
02:18:23.94 +56:23:20.9
02:26:55.66 +56:30:19.4
02:25:03.10 +56:56:58.5
02:23:02.10 +56:30:28.6
02:33:05.09 +56:13:01.1
02:37:50.53 +57:45:50.6
02:35:28.70 +56:28:21.1
02:32:25.76 +56:47:11.8
02:31:09.67 +57:16:15.4
02:34:12.78 +56:12:36.7
02:26:43.12 +56:24:13.3
02:34:04.55 +56:42:30.3
02:23:17.87 +56:42:24.1
02:25:55.90 +56:58:59.9
02:27:59.47 +56:29:43.8
02:25:48.33 +56:55:12.6
02:29:58.05 +56:08:50.3
02:33:40.64 +57:26:09.7
02:35:08.68 +57:36:15.0
02:34:48.58 +57:38:04.9
02:30:03.56 +56:22:32.1
02:32:59.21 +57:28:34.1
02:28:57.12 +57:06:16.3
02:30:18.83 +55:54:55.5
02:19:36.34 +56:23:22.7
02:31:29.13 +57:11:55.8
02:30:59.05 +56:08:44.3
02:16:52.45 +56:18:44.9
02:31:00.03 +56:00:28.9
02:32:17.76 +57:17:09.4
02:26:11.61 +56:56:03.9
02:34:43.40 +56:34:06.2
02:21:34.57 +56:26:43.6
02:36:59.39 +57:56:28.2
02:35:04.69 +57:26:54.1
02:37:50.74 +57:57:57.3
02:33:03.17 +57:03:28.2
02:38:18.06 +57:37:36.9
02:36:07.69 +57:21:39.9
02:20:18.71 +56:31:49.9
02:37:26.82 +58:01:13.3
02:34:24.38 +57:28:25.9
02:28:34.73 +56:13:02.0
02:38:13.41 +57:50:16.7
02:24:01.97 +56:49:23.4
02:33:33.49 +55:49:25.7
02:27:23.30 +55:57:43.1
02:33:10.54 +57:32:53.9
02:37:30.47 +57:39:32.1
02:28:31.63 +56:00:35.4
02:24:33.99 +56:52:59.9
02:25:56.77 +56:07:50.4
02:18:05.16 +56:15:08.3
02:29:57.46 +56:36:50.9
02:35:47.68 +57:10:24.3
02:28:48.14 +56:30:08.1
02:20:07.37 +56:27:51.6
02:25:04.18 +56:13:07.6
02:31:11.42 +56:38:16.1
02:34:12.55 +56:11:53.5
02:25:45.47 +56:26:30.9
02:26:15.74 +56:04:34.8
02:31:02.85 +57:39:55.6
02:37:02.13 +57:41:38.8
02:23:55.69 +56:44:44.9
02:30:39.36 +57:13:43.1
02:31:10.50 +57:30:48.1
02:29:26.52 +56:00:56.6
02:31:29.40 +56:26:22.3
02:33:48.37 +56:47:59.7
02:33:43.66 +57:36:01.4
02:34:13.61 +56:18:42.4
02:29:38.97 +56:11:32.5
02:30:43.84 +55:58:10.7
02:26:00.85 +56:46:18.6
02:27:59.54 +56:09:19.1
02:30:51.75 +57:15:44.4
02:21:55.10 +56:20:50.0
02:31:12.59 +57:00:49.8
02:26:08.81 +56:16:07.7
02:30:41.06 +55:56:25.5
02:35:00.16 +56:43:10.4
02:24:32.07 +56:43:35.5
02:32:18.81 +56:15:24.2
02:30:17.06 +56:38:11.7
02:23:38.16 +56:39:53.3
02:24:25.95 +56:32:57.3
02:28:40.95 +56:12:03.5
02:28:21.40 +55:58:55.7
02:33:50.71 +55:59:56.9
02:31:51.47 +56:45:50.3
02:31:03.02 +55:52:01.4
02:35:12.95 +57:56:23.8
02:30:23.25 +56:23:34.2
02:37:31.30 +57:29:01.8
02:24:47.85 +56:36:57.7
02:34:03.05 +56:00:36.1
02:26:59.37 +57:14:45.3
02:33:48.54 +55:57:07.4
02:33:37.62 +57:40:24.0
02:24:38.05 +56:49:55.5
02:24:18.80 +56:19:50.2
02:37:24.10 +57:31:04.5
02:32:35.10 +57:32:19.9
02:28:56.59 +56:11:02.8
02:25:30.05 +56:16:52.2
02:26:02.34 +56:21:00.8
02:27:34.54 +56:16:51.2
02:33:57.28 +57:00:01.2
02:25:48.44 +56:32:34.9
02:32:31.36 +57:38:51.5
02:29:55.76 +56:55:49.8
02:25:32.72 +56:32:56.9
02:32:23.05 +57:38:37.3
02:27:37.42 +57:04:56.0
02:33:44.26 +56:59:33.8
02:27:52.24 +56:29:30.2
02:38:39.71 +57:47:02.7
02:25:11.61 +56:17:21.6
02:30:00.33 +57:11:29.3
02:33:42.17 +55:51:19.1
02:32:49.37 +57:34:23.1
02:30:32.60 +57:32:13.7
02:30:00.36 +56:17:43.0
02:35:26.59 +57:46:13.0
02:30:38.21 +56:11:54.0
02:36:19.07 +57:07:02.5
02:36:27.53 +56:56:51.3
02:23:11.07 +56:11:20.3
02:22:11.90 +56:20:47.6
02:29:10.75 +55:58:47.7
02:30:45.38 +57:06:30.4
02:36:19.41 +57:59:11.1
02:33:28.12 +56:18:30.6
02:27:07.63 +56:00:29.5
02:34:32.01 +57:40:32.0
02:24:52.39 +56:43:11.8
02:23:08.55 +56:20:25.7
02:30:28.93 +56:19:35.0
02:34:13.74 +56:19:38.4
02:29:11.14 +57:21:01.2
02:36:41.43 +57:37:08.6
02:22:47.61 +56:11:10.3
02:24:38.48 +56:20:47.1
02:32:04.85 +56:53:51.0
02:27:42.05 +56:12:16.6
02:30:07.04 +56:30:20.7
02:23:56.97 +56:11:52.3
02:27:15.92 +56:00:28.3
02:32:37.22 +56:00:39.6
01:40:01.01 +60:52:39.3
02:22:16.01 +56:22:42.1
02:23:07.52 +56:41:45.7
02:34:09.36 +56:41:02.1
02:31:19.74 +56:52:40.3
02:31:43.43 +56:14:45.0
02:32:47.60 +57:14:18.6
02:34:34.57 +56:36:40.8
02:30:33.43 +56:57:01.0
02:25:42.16 +56:37:12.1
02:30:34.92 +56:43:56.7
02:21:32.88 +56:13:40.8
02:33:38.50 +57:33:38.4
02:37:15.56 +57:48:20.7
02:33:30.70 +57:29:01.5
02:36:49.05 +57:24:45.7
02:32:30.78 +56:47:59.9
02:31:46.58 +55:52:30.0
02:36:54.41 +57:53:40.3
02:21:27.45 +56:16:27.4
02:35:12.35 +56:50:10.1
02:32:01.35 +56:51:17.4
02:29:43.00 +56:05:10.4
02:39:58.30 +58:20:59.8
02:33:30.84 +56:43:01.0
02:35:15.88 +56:26:19.4
02:27:22.97 +56:19:27.7
02:30:05.86 +57:18:33.7
02:37:01.21 +57:51:23.9
02:34:37.56 +56:32:35.4
02:34:22.33 +56:20:27.4
02:28:01.24 +56:23:31.7
02:36:42.69 +57:08:11.5
02:33:57.90 +56:36:42.0
02:20:11.66 +56:22:21.1
02:33:11.61 +57:36:40.3
02:21:23.02 +56:39:00.5
02:35:22.14 +56:48:52.6
02:24:12.37 +56:49:24.7
02:32:55.55 +57:08:54.8
02:27:53.50 +57:06:30.2
02:37:38.82 +57:43:26.3
02:34:43.58 +56:51:49.8
02:36:55.85 +57:38:50.5
02:33:06.29 +56:00:32.4
02:33:08.16 +57:28:10.9
02:33:23.59 +57:33:31.5
02:27:27.08 +56:31:12.3
02:25:52.68 +56:47:30.2
02:25:40.02 +56:29:21.1
02:22:21.44 +56:34:17.9
02:24:46.71 +56:38:57.2
02:21:16.35 +56:23:42.9
02:24:53.85 +56:08:46.7
02:28:10.62 +56:06:42.3
02:35:35.04 +57:33:01.8
02:29:33.78 +56:09:10.9
02:34:04.23 +57:32:43.7
02:30:51.32 +57:16:48.9
02:21:13.42 +56:28:43.4
02:29:38.91 +56:20:56.3
02:32:49.88 +56:14:34.7
01:25:31.68 +57:37:40.0
02:35:41.88 +57:31:41.5
02:30:42.09 +57:22:37.0
02:31:45.76 +57:14:33.8
02:34:19.68 +57:08:34.6
02:37:47.00 +58:07:12.4
02:29:29.31 +57:10:38.0
02:33:27.53 +57:14:42.7
02:39:23.81 +58:09:08.6
02:25:53.36 +56:14:37.1
02:31:12.55 +56:27:35.9
02:27:22.07 +56:31:21.0
02:25:52.25 +57:02:03.7
02:29:04.86 +57:22:34.6
02:34:06.59 +56:06:19.6
02:25:56.52 +56:32:32.5
02:21:19.11 +56:38:13.7
02:39:21.43 +58:07:09.6
02:28:31.02 +56:40:25.2
02:23:08.48 +56:55:24.7
02:38:14.36 +57:58:52.1
02:31:54.47 +55:50:24.1
02:34:32.89 +57:07:24.9
02:21:52.35 +56:32:44.4
02:26:14.36 +56:12:10.7
02:34:18.24 +57:49:31.9
02:29:41.72 +56:37:30.4
02:30:58.42 +57:16:18.4
02:36:12.12 +57:41:55.7
02:26:01.05 +56:28:14.9
02:22:37.96 +56:37:19.4
02:24:27.17 +56:50:29.3
02:36:52.73 +57:40:54.2
00:58:55.95 +58:04:06.6
02:34:27.71 +56:43:27.0
02:30:09.40 +57:23:13.6
02:29:02.18 +56:24:16.8
02:30:26.89 +56:10:14.6
02:32:42.22 +57:14:26.4
02:36:28.05 +56:50:31.6
02:33:18.04 +57:31:36.2
02:31:18.63 +57:03:51.6
02:36:19.82 +56:57:28.2
02:29:25.42 +55:58:54.2
02:36:18.15 +56:52:17.8
02:34:42.56 +57:17:57.3
02:26:58.18 +56:22:09.7
02:34:40.76 +56:11:02.3
02:33:07.75 +56:14:50.5
02:36:19.79 +57:18:00.4
02:27:40.45 +56:20:28.8
02:23:42.90 +56:38:37.4
02:22:22.76 +56:39:59.4
02:30:38.78 +56:15:14.6
02:33:02.03 +56:26:23.4
00:43:47.73 +61:54:01.0
02:18:56.11 +56:18:31.6
02:33:25.63 +56:59:44.8
02:37:55.66 +58:18:21.1
02:38:07.48 +58:00:10.7
02:26:55.93 +56:28:27.3
02:32:05.93 +57:04:59.5
01:18:14.25 +61:44:36.4
02:33:01.80 +57:36:06.2
02:30:49.71 +56:26:27.4
02:28:42.38 +55:58:14.1
02:31:52.59 +56:53:47.2
02:37:59.24 +58:07:39.6
02:27:44.77 +56:19:42.5
02:33:08.38 +57:21:21.6
02:38:19.80 +58:03:54.5
02:35:58.83 +57:31:57.8
01:29:32.82 +61:46:26.3
02:35:43.57 +57:50:30.9
02:29:48.85 +56:41:55.4
01:22:23.81 +61:13:50.8
02:31:18.55 +56:20:48.9
02:33:40.20 +57:40:02.4
02:17:19.11 +56:42:44.0
01:31:28.05 +57:20:36.4
02:21:40.76 +60:54:41.6
02:15:20.33 +62:13:49.2
02:15:35.89 +56:21:36.7
02:05:05.69 +58:16:23.9
02:19:03.87 +62:47:34.5
02:29:57.73 +57:10:58.0
02:38:02.15 +58:50:40.7
02:34:36.31 +58:11:22.9
02:24:29.91 +59:24:30.8
01:21:54.72 +61:20:55.4
02:25:13.36 +56:30:31.4
02:26:44.41 +58:15:51.9
02:29:19.57 +57:07:07.2
01:27:44.31 +62:06:39.9
01:41:46.90 +59:03:47.3
02:14:24.94 +56:42:49.3
02:08:53.89 +58:42:29.3
02:31:45.72 +56:26:45.7
02:33:34.77 +57:08:54.4
01:32:51.45 +62:40:36.3
02:31:42.43 +56:35:52.7
02:19:16.63 +59:42:21.5
02:29:16.20 +56:24:33.1
02:17:01.69 +56:56:08.6
02:19:48.16 +56:25:08.9
02:15:26.96 +62:47:45.2
02:33:31.89 +57:34:08.3
01:16:28.98 +60:13:59.7
02:28:27.94 +57:25:38.4
02:13:41.76 +57:25:36.7
02:18:24.65 +58:37:26.1
02:33:51.42 +56:10:59.9
02:22:56.62 +57:11:45.0
02:27:27.68 +56:03:05.8
01:30:50.27 +60:32:13.3
02:34:12.69 +56:03:50.1
02:29:46.25 +56:03:50.4
01:24:30.58 +59:38:48.3
02:21:26.44 +57:16:58.2
02:01:28.14 +58:18:14.4
02:29:59.54 +56:13:01.3
02:34:05.60 +56:37:26.3
02:38:48.25 +57:57:34.8
02:27:22.20 +62:38:25.9
01:09:38.04 +59:05:14.4
02:27:55.40 +56:27:24.2
01:14:56.64 +59:42:13.1
02:21:35.99 +57:03:40.3
02:19:34.14 +58:23:58.2
02:31:32.42 +56:47:58.9
02:32:22.18 +58:28:54.4
02:37:50.81 +57:54:16.4
02:00:57.08 +58:36:59.1
01:28:36.14 +61:12:06.5
01:20:18.33 +64:28:06.2
02:31:45.44 +55:57:58.0
01:31:04.82 +57:13:13.1
02:03:07.50 +57:18:14.2
02:33:23.80 +64:24:59.6
01:45:16.04 +57:55:47.0
02:29:48.53 +57:57:49.9
02:13:47.87 +63:11:26.2
01:43:45.27 +58:23:44.4
02:41:04.47 +62:17:31.2
02:30:52.96 +56:54:19.5
02:27:11.38 +56:07:26.5
02:31:31.09 +57:22:44.7
01:37:01.32 +61:15:57.4
02:18:22.53 +58:47:08.9
02:28:34.52 +56:03:00.1
01:35:09.79 +60:17:09.4
###################################################################################
01:56:38.10 +59:15:33.5 -- not an asteroid (will add it to exclusion list)
01:43:36.46 +58:48:08.4 -- not an asteroid (will add it to exclusion list)
00:30:33.64 +66:05:36.8 -- not an asteroid (will add it to exclusion list)
01:37:22.21 +59:19:56.8 -- not an asteroid (will add it to exclusion list)
02:09:05.47 +57:29:28.7 -- not an asteroid (will add it to exclusion list)
02:25:12.14 +58:09:07.0 -- not an asteroid (will add it to exclusion list)
00:42:45.77 +63:38:26.5 -- not an asteroid (will add it to exclusion list)
02:37:27.18 +57:28:29.8 -- not an asteroid (will add it to exclusion list)
00:36:55.27 +62:40:47.8 -- not an asteroid (will add it to exclusion list)
02:19:45.14 +57:01:17.6 -- not an asteroid (will add it to exclusion list)
02:29:09.11 +56:37:12.5 -- not an asteroid (will add it to exclusion list)
02:25:27.59 +56:46:56.3 -- not an asteroid (will add it to exclusion list)
02:32:05.00 +56:39:58.8 -- not an asteroid (will add it to exclusion list)
02:32:34.50 +57:29:15.5 -- not an asteroid (will add it to exclusion list)
02:27:57.93 +56:02:37.4 -- not an asteroid (will add it to exclusion list)
02:29:09.98 +56:27:11.8 -- not an asteroid (will add it to exclusion list)
02:31:25.66 +55:59:07.0 -- not an asteroid (will add it to exclusion list)
02:22:03.80 +56:31:26.9 -- not an asteroid (will add it to exclusion list)
02:34:10.16 +55:50:00.1 -- not an asteroid (will add it to exclusion list)
02:32:46.00 +56:48:25.9 -- not an asteroid (will add it to exclusion list)
02:34:34.19 +56:21:55.6 -- not an asteroid (will add it to exclusion list)
02:35:37.81 +57:29:13.2 -- not an asteroid (will add it to exclusion list)
02:25:20.43 +56:51:13.3 -- not an asteroid (will add it to exclusion list)
02:34:43.96 +56:06:06.8 -- not an asteroid (will add it to exclusion list)
02:27:24.36 +56:23:03.8 -- not an asteroid (will add it to exclusion list)
02:30:53.64 +56:14:28.0 -- not an asteroid (will add it to exclusion list)
02:33:34.24 +55:54:24.4 -- not an asteroid (will add it to exclusion list)
02:24:11.84 +56:35:43.1 -- not an asteroid (will add it to exclusion list)
02:23:35.43 +56:34:27.3 -- not an asteroid (will add it to exclusion list)
02:37:08.47 +57:25:21.7 -- not an asteroid (will add it to exclusion list)
02:36:28.42 +57:11:45.9 -- not an asteroid (will add it to exclusion list)
02:35:52.02 +57:47:22.1 -- not an asteroid (will add it to exclusion list)
02:23:26.39 +56:06:42.0 -- not an asteroid (will add it to exclusion list)
02:36:33.26 +57:54:38.3 -- not an asteroid (will add it to exclusion list)
02:27:20.56 +56:01:48.1 -- not an asteroid (will add it to exclusion list)
02:36:36.25 +57:46:59.1 -- not an asteroid (will add it to exclusion list)
02:18:01.27 +56:15:42.4 -- not an asteroid (will add it to exclusion list)
02:32:05.68 +57:22:03.0 -- not an asteroid (will add it to exclusion list)
02:19:46.66 +56:22:25.8 -- not an asteroid (will add it to exclusion list)
02:34:05.22 +56:25:31.7 -- not an asteroid (will add it to exclusion list)
02:21:55.21 +56:25:08.8 -- not an asteroid (will add it to exclusion list)
02:29:11.88 +56:17:58.5 -- not an asteroid (will add it to exclusion list)
02:31:25.67 +56:07:05.3 -- not an asteroid (will add it to exclusion list)
02:32:15.38 +56:38:50.2 -- not an asteroid (will add it to exclusion list)
02:30:44.93 +56:56:12.3 -- not an asteroid (will add it to exclusion list)
02:21:50.35 +56:34:31.6 -- not an asteroid (will add it to exclusion list)
02:26:59.12 +56:01:57.0 -- not an asteroid (will add it to exclusion list)
02:22:35.34 +56:18:13.6 -- not an asteroid (will add it to exclusion list)
02:26:48.88 +55:59:11.6 -- not an asteroid (will add it to exclusion list)
02:32:55.20 +56:39:40.1 -- not an asteroid (will add it to exclusion list)
02:33:01.81 +57:02:07.5 -- not an asteroid (will add it to exclusion list)
02:20:54.06 +56:16:37.3 -- not an asteroid (will add it to exclusion list)
02:31:06.51 +56:30:41.5 -- not an asteroid (will add it to exclusion list)
02:24:43.69 +56:59:33.9 -- not an asteroid (will add it to exclusion list)
02:38:46.64 +57:49:57.9 -- not an asteroid (will add it to exclusion list)
02:37:36.83 +57:51:16.3 -- not an asteroid (will add it to exclusion list)
02:37:55.04 +57:39:03.5 -- not an asteroid (will add it to exclusion list)
02:22:06.87 +56:07:53.3 -- not an asteroid (will add it to exclusion list)
02:34:03.56 +56:30:43.8 -- not an asteroid (will add it to exclusion list)
02:21:20.56 +56:29:12.2 -- not an asteroid (will add it to exclusion list)
02:32:04.85 +56:49:24.8 -- not an asteroid (will add it to exclusion list)
02:30:12.39 +56:11:25.0 -- not an asteroid (will add it to exclusion list)
02:22:10.20 +56:24:23.0 -- not an asteroid (will add it to exclusion list)
02:27:48.50 +57:05:55.4 -- not an asteroid (will add it to exclusion list)
02:28:50.78 +56:20:48.8 -- not an asteroid (will add it to exclusion list)
02:33:48.46 +57:01:46.2 -- not an asteroid (will add it to exclusion list)
02:19:52.94 +56:15:40.6 -- not an asteroid (will add it to exclusion list)
02:25:28.14 +56:11:20.3 -- not an asteroid (will add it to exclusion list)
02:33:49.33 +57:35:12.0 -- not an asteroid (will add it to exclusion list)
02:19:48.61 +56:23:45.8 -- not an asteroid (will add it to exclusion list)
02:25:20.33 +56:12:13.7 -- not an asteroid (will add it to exclusion list)
02:24:41.99 +56:55:48.0 -- not an asteroid (will add it to exclusion list)
02:31:11.98 +57:09:48.2 -- not an asteroid (will add it to exclusion list)
02:19:36.43 +56:14:20.7 -- not an asteroid (will add it to exclusion list)
02:18:48.83 +56:19:01.6 -- not an asteroid (will add it to exclusion list)
02:32:45.28 +57:08:07.9 -- not an asteroid (will add it to exclusion list)
02:18:48.46 +56:17:54.5 -- not an asteroid (will add it to exclusion list)
02:35:33.89 +57:09:19.1 -- not an asteroid (will add it to exclusion list)
02:36:19.72 +57:15:27.8 -- not an asteroid (will add it to exclusion list)
02:31:37.57 +56:33:36.1 -- not an asteroid (will add it to exclusion list)
02:27:07.76 +56:33:53.6 -- not an asteroid (will add it to exclusion list)
02:30:51.92 +57:04:10.4 -- not an asteroid (will add it to exclusion list)
02:23:42.80 +56:07:10.6 -- not an asteroid (will add it to exclusion list)
02:20:32.12 +56:10:01.0 -- 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)
02:25:33.83 +56:34:21.8 -- not an asteroid (will add it to exclusion list)
02:35:18.49 +57:31:39.8 -- not an asteroid (will add it to exclusion list)
02:20:55.01 +56:23:18.7 -- not an asteroid (will add it to exclusion list)
02:33:30.04 +57:42:18.6 -- not an asteroid (will add it to exclusion list)
02:31:18.30 +55:53:50.8 -- not an asteroid (will add it to exclusion list)
02:31:38.41 +57:13:47.7 -- not an asteroid (will add it to exclusion list)
02:27:33.21 +56:13:10.2 -- not an asteroid (will add it to exclusion list)
02:36:35.00 +57:36:36.2 -- not an asteroid (will add it to exclusion list)
02:22:04.44 +57:10:39.1 -- not an asteroid (will add it to exclusion list)
02:31:58.58 +56:42:23.0 -- not an asteroid (will add it to exclusion list)
02:29:17.15 +57:14:29.9 -- not an asteroid (will add it to exclusion list)
02:36:56.54 +57:06:44.6 -- not an asteroid (will add it to exclusion list)
02:24:06.51 +56:29:59.7 -- not an asteroid (will add it to exclusion list)
02:24:33.48 +56:57:19.3 -- not an asteroid (will add it to exclusion list)
02:32:18.19 +56:21:26.4 -- not an asteroid (will add it to exclusion list)
02:19:39.63 +56:20:11.7 -- not an asteroid (will add it to exclusion list)
02:30:32.08 +57:11:25.7 -- not an asteroid (will add it to exclusion list)
02:26:13.32 +56:36:46.9 -- not an asteroid (will add it to exclusion list)
02:30:33.06 +56:53:09.3 -- not an asteroid (will add it to exclusion list)
02:35:20.15 +57:29:29.6 -- not an asteroid (will add it to exclusion list)
02:26:07.39 +56:25:11.4 -- not an asteroid (will add it to exclusion list)
02:30:00.36 +57:28:19.5 -- not an asteroid (will add it to exclusion list)
02:29:32.65 +55:57:16.0 -- not an asteroid (will add it to exclusion list)
02:31:05.86 +56:37:18.2 -- not an asteroid (will add it to exclusion list)
02:24:32.58 +57:00:45.4 -- not an asteroid (will add it to exclusion list)
02:19:56.59 +56:13:25.6 -- not an asteroid (will add it to exclusion list)
02:36:08.58 +57:39:34.6 -- not an asteroid (will add it to exclusion list)
02:29:40.57 +56:18:39.2 -- not an asteroid (will add it to exclusion list)
02:30:37.28 +56:22:56.7 -- not an asteroid (will add it to exclusion list)
02:31:20.20 +57:33:46.6 -- not an asteroid (will add it to exclusion list)
02:30:49.36 +56:11:02.6 -- not an asteroid (will add it to exclusion list)
02:34:28.42 +56:22:24.6 -- not an asteroid (will add it to exclusion list)
02:24:18.90 +56:54:02.0 -- not an asteroid (will add it to exclusion list)
02:29:50.49 +56:19:09.0 -- not an asteroid (will add it to exclusion list)
02:29:40.82 +56:20:03.6 -- not an asteroid (will add it to exclusion list)
02:25:00.79 +56:51:32.4 -- not an asteroid (will add it to exclusion list)
02:32:13.87 +55:56:23.6 -- not an asteroid (will add it to exclusion list)
02:29:28.33 +56:33:05.7 -- not an asteroid (will add it to exclusion list)
02:28:09.55 +56:10:49.3 -- not an asteroid (will add it to exclusion list)
02:33:09.16 +57:00:38.4 -- not an asteroid (will add it to exclusion list)
02:21:04.80 +56:15:33.0 -- not an asteroid (will add it to exclusion list)
02:37:41.06 +57:33:22.4 -- not an asteroid (will add it to exclusion list)
02:28:48.94 +56:07:35.3 -- not an asteroid (will add it to exclusion list)
02:21:59.12 +56:30:01.8 -- not an asteroid (will add it to exclusion list)
02:30:30.77 +57:30:27.1 -- not an asteroid (will add it to exclusion list)
02:22:31.56 +56:14:11.4 -- not an asteroid (will add it to exclusion list)
02:34:25.96 +56:29:13.8 -- not an asteroid (will add it to exclusion list)
02:33:33.86 +56:11:46.9 -- not an asteroid (will add it to exclusion list)
02:35:42.45 +56:44:19.0 -- not an asteroid (will add it to exclusion list)
02:16:48.70 +56:16:11.9 -- not an asteroid (will add it to exclusion list)
02:36:22.60 +57:40:05.9 -- not an asteroid (will add it to exclusion list)
02:23:48.04 +56:47:01.7 -- not an asteroid (will add it to exclusion list)
02:26:10.78 +56:48:29.0 -- not an asteroid (will add it to exclusion list)
02:35:30.16 +57:03:30.3 -- not an asteroid (will add it to exclusion list)
02:18:23.94 +56:23:20.9 -- not an asteroid (will add it to exclusion list)
02:26:55.66 +56:30:19.4 -- not an asteroid (will add it to exclusion list)
02:25:03.10 +56:56:58.5 -- not an asteroid (will add it to exclusion list)
02:23:02.10 +56:30:28.6 -- not an asteroid (will add it to exclusion list)
02:33:05.09 +56:13:01.1 -- not an asteroid (will add it to exclusion list)
02:37:50.53 +57:45:50.6 -- not an asteroid (will add it to exclusion list)
02:35:28.70 +56:28:21.1 -- not an asteroid (will add it to exclusion list)
02:32:25.76 +56:47:11.8 -- not an asteroid (will add it to exclusion list)
02:31:09.67 +57:16:15.4 -- not an asteroid (will add it to exclusion list)
02:34:12.78 +56:12:36.7 -- not an asteroid (will add it to exclusion list)
02:26:43.12 +56:24:13.3 -- not an asteroid (will add it to exclusion list)
02:34:04.55 +56:42:30.3 -- not an asteroid (will add it to exclusion list)
02:23:17.87 +56:42:24.1 -- not an asteroid (will add it to exclusion list)
02:25:55.90 +56:58:59.9 -- not an asteroid (will add it to exclusion list)
02:27:59.47 +56:29:43.8 -- not an asteroid (will add it to exclusion list)
02:25:48.33 +56:55:12.6 -- not an asteroid (will add it to exclusion list)
02:29:58.05 +56:08:50.3 -- not an asteroid (will add it to exclusion list)
02:33:40.64 +57:26:09.7 -- not an asteroid (will add it to exclusion list)
02:35:08.68 +57:36:15.0 -- not an asteroid (will add it to exclusion list)
02:34:48.58 +57:38:04.9 -- not an asteroid (will add it to exclusion list)
02:30:03.56 +56:22:32.1 -- not an asteroid (will add it to exclusion list)
02:32:59.21 +57:28:34.1 -- not an asteroid (will add it to exclusion list)
02:28:57.12 +57:06:16.3 -- not an asteroid (will add it to exclusion list)
02:30:18.83 +55:54:55.5 -- not an asteroid (will add it to exclusion list)
02:19:36.34 +56:23:22.7 -- not an asteroid (will add it to exclusion list)
02:31:29.13 +57:11:55.8 -- not an asteroid (will add it to exclusion list)
02:30:59.05 +56:08:44.3 -- not an asteroid (will add it to exclusion list)
02:16:52.45 +56:18:44.9 -- not an asteroid (will add it to exclusion list)
02:31:00.03 +56:00:28.9 -- not an asteroid (will add it to exclusion list)
02:32:17.76 +57:17:09.4 -- not an asteroid (will add it to exclusion list)
02:26:11.61 +56:56:03.9 -- not an asteroid (will add it to exclusion list)
02:34:43.40 +56:34:06.2 -- not an asteroid (will add it to exclusion list)
02:21:34.57 +56:26:43.6 -- not an asteroid (will add it to exclusion list)
02:36:59.39 +57:56:28.2 -- not an asteroid (will add it to exclusion list)
02:35:04.69 +57:26:54.1 -- not an asteroid (will add it to exclusion list)
02:37:50.74 +57:57:57.3 -- not an asteroid (will add it to exclusion list)
02:33:03.17 +57:03:28.2 -- not an asteroid (will add it to exclusion list)
02:38:18.06 +57:37:36.9 -- not an asteroid (will add it to exclusion list)
02:36:07.69 +57:21:39.9 -- not an asteroid (will add it to exclusion list)
02:20:18.71 +56:31:49.9 -- not an asteroid (will add it to exclusion list)
02:37:26.82 +58:01:13.3 -- not an asteroid (will add it to exclusion list)
02:34:24.38 +57:28:25.9 -- not an asteroid (will add it to exclusion list)
02:28:34.73 +56:13:02.0 -- not an asteroid (will add it to exclusion list)
02:38:13.41 +57:50:16.7 -- not an asteroid (will add it to exclusion list)
02:24:01.97 +56:49:23.4 -- not an asteroid (will add it to exclusion list)
02:33:33.49 +55:49:25.7 -- not an asteroid (will add it to exclusion list)
02:27:23.30 +55:57:43.1 -- not an asteroid (will add it to exclusion list)
02:33:10.54 +57:32:53.9 -- not an asteroid (will add it to exclusion list)
02:37:30.47 +57:39:32.1 -- not an asteroid (will add it to exclusion list)
02:28:31.63 +56:00:35.4 -- not an asteroid (will add it to exclusion list)
02:24:33.99 +56:52:59.9 -- not an asteroid (will add it to exclusion list)
02:25:56.77 +56:07:50.4 -- not an asteroid (will add it to exclusion list)
02:18:05.16 +56:15:08.3 -- not an asteroid (will add it to exclusion list)
02:29:57.46 +56:36:50.9 -- not an asteroid (will add it to exclusion list)
02:35:47.68 +57:10:24.3 -- not an asteroid (will add it to exclusion list)
02:28:48.14 +56:30:08.1 -- not an asteroid (will add it to exclusion list)
02:20:07.37 +56:27:51.6 -- not an asteroid (will add it to exclusion list)
02:25:04.18 +56:13:07.6 -- not an asteroid (will add it to exclusion list)
02:31:11.42 +56:38:16.1 -- not an asteroid (will add it to exclusion list)
02:34:12.55 +56:11:53.5 -- not an asteroid (will add it to exclusion list)
02:25:45.47 +56:26:30.9 -- not an asteroid (will add it to exclusion list)
02:26:15.74 +56:04:34.8 -- not an asteroid (will add it to exclusion list)
02:31:02.85 +57:39:55.6 -- not an asteroid (will add it to exclusion list)
02:37:02.13 +57:41:38.8 -- not an asteroid (will add it to exclusion list)
02:23:55.69 +56:44:44.9 -- not an asteroid (will add it to exclusion list)
02:30:39.36 +57:13:43.1 -- not an asteroid (will add it to exclusion list)
02:31:10.50 +57:30:48.1 -- not an asteroid (will add it to exclusion list)
02:29:26.52 +56:00:56.6 -- not an asteroid (will add it to exclusion list)
02:31:29.40 +56:26:22.3 -- not an asteroid (will add it to exclusion list)
02:33:48.37 +56:47:59.7 -- not an asteroid (will add it to exclusion list)
02:33:43.66 +57:36:01.4 -- not an asteroid (will add it to exclusion list)
02:34:13.61 +56:18:42.4 -- not an asteroid (will add it to exclusion list)
02:29:38.97 +56:11:32.5 -- not an asteroid (will add it to exclusion list)
02:30:43.84 +55:58:10.7 -- not an asteroid (will add it to exclusion list)
02:26:00.85 +56:46:18.6 -- not an asteroid (will add it to exclusion list)
02:27:59.54 +56:09:19.1 -- not an asteroid (will add it to exclusion list)
02:30:51.75 +57:15:44.4 -- not an asteroid (will add it to exclusion list)
02:21:55.10 +56:20:50.0 -- not an asteroid (will add it to exclusion list)
02:31:12.59 +57:00:49.8 -- not an asteroid (will add it to exclusion list)
02:26:08.81 +56:16:07.7 -- not an asteroid (will add it to exclusion list)
02:30:41.06 +55:56:25.5 -- not an asteroid (will add it to exclusion list)
02:35:00.16 +56:43:10.4 -- not an asteroid (will add it to exclusion list)
02:24:32.07 +56:43:35.5 -- not an asteroid (will add it to exclusion list)
02:32:18.81 +56:15:24.2 -- not an asteroid (will add it to exclusion list)
02:30:17.06 +56:38:11.7 -- not an asteroid (will add it to exclusion list)
02:23:38.16 +56:39:53.3 -- not an asteroid (will add it to exclusion list)
02:24:25.95 +56:32:57.3 -- not an asteroid (will add it to exclusion list)
02:28:40.95 +56:12:03.5 -- not an asteroid (will add it to exclusion list)
02:28:21.40 +55:58:55.7 -- not an asteroid (will add it to exclusion list)
02:33:50.71 +55:59:56.9 -- not an asteroid (will add it to exclusion list)
02:31:51.47 +56:45:50.3 -- not an asteroid (will add it to exclusion list)
02:31:03.02 +55:52:01.4 -- not an asteroid (will add it to exclusion list)
02:35:12.95 +57:56:23.8 -- not an asteroid (will add it to exclusion list)
02:30:23.25 +56:23:34.2 -- not an asteroid (will add it to exclusion list)
02:37:31.30 +57:29:01.8 -- not an asteroid (will add it to exclusion list)
02:24:47.85 +56:36:57.7 -- not an asteroid (will add it to exclusion list)
02:34:03.05 +56:00:36.1 -- not an asteroid (will add it to exclusion list)
02:26:59.37 +57:14:45.3 -- not an asteroid (will add it to exclusion list)
02:33:48.54 +55:57:07.4 -- not an asteroid (will add it to exclusion list)
02:33:37.62 +57:40:24.0 -- not an asteroid (will add it to exclusion list)
02:24:38.05 +56:49:55.5 -- not an asteroid (will add it to exclusion list)
02:24:18.80 +56:19:50.2 -- not an asteroid (will add it to exclusion list)
02:37:24.10 +57:31:04.5 -- not an asteroid (will add it to exclusion list)
02:32:35.10 +57:32:19.9 -- not an asteroid (will add it to exclusion list)
02:28:56.59 +56:11:02.8 -- not an asteroid (will add it to exclusion list)
02:25:30.05 +56:16:52.2 -- not an asteroid (will add it to exclusion list)
02:26:02.34 +56:21:00.8 -- not an asteroid (will add it to exclusion list)
02:27:34.54 +56:16:51.2 -- not an asteroid (will add it to exclusion list)
02:33:57.28 +57:00:01.2 -- not an asteroid (will add it to exclusion list)
02:25:48.44 +56:32:34.9 -- not an asteroid (will add it to exclusion list)
02:32:31.36 +57:38:51.5 -- not an asteroid (will add it to exclusion list)
02:29:55.76 +56:55:49.8 -- not an asteroid (will add it to exclusion list)
02:25:32.72 +56:32:56.9 -- not an asteroid (will add it to exclusion list)
02:32:23.05 +57:38:37.3 -- not an asteroid (will add it to exclusion list)
02:27:37.42 +57:04:56.0 -- not an asteroid (will add it to exclusion list)
02:33:44.26 +56:59:33.8 -- not an asteroid (will add it to exclusion list)
02:27:52.24 +56:29:30.2 -- not an asteroid (will add it to exclusion list)
02:38:39.71 +57:47:02.7 -- not an asteroid (will add it to exclusion list)
02:25:11.61 +56:17:21.6 -- not an asteroid (will add it to exclusion list)
02:30:00.33 +57:11:29.3 -- not an asteroid (will add it to exclusion list)
02:33:42.17 +55:51:19.1 -- not an asteroid (will add it to exclusion list)
02:32:49.37 +57:34:23.1 -- not an asteroid (will add it to exclusion list)
02:30:32.60 +57:32:13.7 -- not an asteroid (will add it to exclusion list)
02:30:00.36 +56:17:43.0 -- not an asteroid (will add it to exclusion list)
02:35:26.59 +57:46:13.0 -- not an asteroid (will add it to exclusion list)
02:30:38.21 +56:11:54.0 -- not an asteroid (will add it to exclusion list)
02:36:19.07 +57:07:02.5 -- not an asteroid (will add it to exclusion list)
02:36:27.53 +56:56:51.3 -- not an asteroid (will add it to exclusion list)
02:23:11.07 +56:11:20.3 -- not an asteroid (will add it to exclusion list)
02:22:11.90 +56:20:47.6 -- not an asteroid (will add it to exclusion list)
02:29:10.75 +55:58:47.7 -- not an asteroid (will add it to exclusion list)
02:30:45.38 +57:06:30.4 -- not an asteroid (will add it to exclusion list)
02:36:19.41 +57:59:11.1 -- not an asteroid (will add it to exclusion list)
02:33:28.12 +56:18:30.6 -- not an asteroid (will add it to exclusion list)
02:27:07.63 +56:00:29.5 -- not an asteroid (will add it to exclusion list)
02:34:32.01 +57:40:32.0 -- not an asteroid (will add it to exclusion list)
02:24:52.39 +56:43:11.8 -- not an asteroid (will add it to exclusion list)
02:23:08.55 +56:20:25.7 -- not an asteroid (will add it to exclusion list)
02:30:28.93 +56:19:35.0 -- not an asteroid (will add it to exclusion list)
02:34:13.74 +56:19:38.4 -- not an asteroid (will add it to exclusion list)
02:29:11.14 +57:21:01.2 -- not an asteroid (will add it to exclusion list)
02:36:41.43 +57:37:08.6 -- not an asteroid (will add it to exclusion list)
02:22:47.61 +56:11:10.3 -- not an asteroid (will add it to exclusion list)
02:24:38.48 +56:20:47.1 -- not an asteroid (will add it to exclusion list)
02:32:04.85 +56:53:51.0 -- not an asteroid (will add it to exclusion list)
02:27:42.05 +56:12:16.6 -- not an asteroid (will add it to exclusion list)
02:30:07.04 +56:30:20.7 -- not an asteroid (will add it to exclusion list)
02:23:56.97 +56:11:52.3 -- not an asteroid (will add it to exclusion list)
02:27:15.92 +56:00:28.3 -- not an asteroid (will add it to exclusion list)
02:32:37.22 +56:00:39.6 -- not an asteroid (will add it to exclusion list)
01:40:01.01 +60:52:39.3 -- not an asteroid (will add it to exclusion list)
02:22:16.01 +56:22:42.1 -- not an asteroid (will add it to exclusion list)
02:23:07.52 +56:41:45.7 -- not an asteroid (will add it to exclusion list)
02:34:09.36 +56:41:02.1 -- not an asteroid (will add it to exclusion list)
02:31:19.74 +56:52:40.3 -- not an asteroid (will add it to exclusion list)
02:31:43.43 +56:14:45.0 -- not an asteroid (will add it to exclusion list)
02:32:47.60 +57:14:18.6 -- not an asteroid (will add it to exclusion list)
02:34:34.57 +56:36:40.8 -- not an asteroid (will add it to exclusion list)
02:30:33.43 +56:57:01.0 -- not an asteroid (will add it to exclusion list)
02:25:42.16 +56:37:12.1 -- not an asteroid (will add it to exclusion list)
02:30:34.92 +56:43:56.7 -- not an asteroid (will add it to exclusion list)
02:21:32.88 +56:13:40.8 -- not an asteroid (will add it to exclusion list)
02:33:38.50 +57:33:38.4 -- not an asteroid (will add it to exclusion list)
02:37:15.56 +57:48:20.7 -- not an asteroid (will add it to exclusion list)
02:33:30.70 +57:29:01.5 -- not an asteroid (will add it to exclusion list)
02:36:49.05 +57:24:45.7 -- not an asteroid (will add it to exclusion list)
02:32:30.78 +56:47:59.9 -- not an asteroid (will add it to exclusion list)
02:31:46.58 +55:52:30.0 -- not an asteroid (will add it to exclusion list)
02:36:54.41 +57:53:40.3 -- not an asteroid (will add it to exclusion list)
02:21:27.45 +56:16:27.4 -- not an asteroid (will add it to exclusion list)
02:35:12.35 +56:50:10.1 -- not an asteroid (will add it to exclusion list)
02:32:01.35 +56:51:17.4 -- not an asteroid (will add it to exclusion list)
02:29:43.00 +56:05:10.4 -- not an asteroid (will add it to exclusion list)
02:39:58.30 +58:20:59.8 -- not an asteroid (will add it to exclusion list)
02:33:30.84 +56:43:01.0 -- not an asteroid (will add it to exclusion list)
02:35:15.88 +56:26:19.4 -- not an asteroid (will add it to exclusion list)
02:27:22.97 +56:19:27.7 -- not an asteroid (will add it to exclusion list)
02:30:05.86 +57:18:33.7 -- not an asteroid (will add it to exclusion list)
02:37:01.21 +57:51:23.9 -- not an asteroid (will add it to exclusion list)
02:34:37.56 +56:32:35.4 -- not an asteroid (will add it to exclusion list)
02:34:22.33 +56:20:27.4 -- not an asteroid (will add it to exclusion list)
02:28:01.24 +56:23:31.7 -- not an asteroid (will add it to exclusion list)
02:36:42.69 +57:08:11.5 -- not an asteroid (will add it to exclusion list)
02:33:57.90 +56:36:42.0 -- not an asteroid (will add it to exclusion list)
02:20:11.66 +56:22:21.1 -- not an asteroid (will add it to exclusion list)
02:33:11.61 +57:36:40.3 -- not an asteroid (will add it to exclusion list)
02:21:23.02 +56:39:00.5 -- not an asteroid (will add it to exclusion list)
02:35:22.14 +56:48:52.6 -- not an asteroid (will add it to exclusion list)
02:24:12.37 +56:49:24.7 -- not an asteroid (will add it to exclusion list)
02:32:55.55 +57:08:54.8 -- not an asteroid (will add it to exclusion list)
02:27:53.50 +57:06:30.2 -- not an asteroid (will add it to exclusion list)
02:37:38.82 +57:43:26.3 -- not an asteroid (will add it to exclusion list)
02:34:43.58 +56:51:49.8 -- not an asteroid (will add it to exclusion list)
02:36:55.85 +57:38:50.5 -- not an asteroid (will add it to exclusion list)
02:33:06.29 +56:00:32.4 -- not an asteroid (will add it to exclusion list)
02:33:08.16 +57:28:10.9 -- not an asteroid (will add it to exclusion list)
02:33:23.59 +57:33:31.5 -- not an asteroid (will add it to exclusion list)
02:27:27.08 +56:31:12.3 -- not an asteroid (will add it to exclusion list)
02:25:52.68 +56:47:30.2 -- not an asteroid (will add it to exclusion list)
02:25:40.02 +56:29:21.1 -- not an asteroid (will add it to exclusion list)
02:22:21.44 +56:34:17.9 -- not an asteroid (will add it to exclusion list)
02:24:46.71 +56:38:57.2 -- not an asteroid (will add it to exclusion list)
02:21:16.35 +56:23:42.9 -- not an asteroid (will add it to exclusion list)
02:24:53.85 +56:08:46.7 -- not an asteroid (will add it to exclusion list)
02:28:10.62 +56:06:42.3 -- not an asteroid (will add it to exclusion list)
02:35:35.04 +57:33:01.8 -- not an asteroid (will add it to exclusion list)
02:29:33.78 +56:09:10.9 -- not an asteroid (will add it to exclusion list)
02:34:04.23 +57:32:43.7 -- not an asteroid (will add it to exclusion list)
02:30:51.32 +57:16:48.9 -- not an asteroid (will add it to exclusion list)
02:21:13.42 +56:28:43.4 -- not an asteroid (will add it to exclusion list)
02:29:38.91 +56:20:56.3 -- not an asteroid (will add it to exclusion list)
02:32:49.88 +56:14:34.7 -- not an asteroid (will add it to exclusion list)
01:25:31.68 +57:37:40.0 -- not an asteroid (will add it to exclusion list)
02:35:41.88 +57:31:41.5 -- not an asteroid (will add it to exclusion list)
02:30:42.09 +57:22:37.0 -- not an asteroid (will add it to exclusion list)
02:31:45.76 +57:14:33.8 -- not an asteroid (will add it to exclusion list)
02:34:19.68 +57:08:34.6 -- not an asteroid (will add it to exclusion list)
02:37:47.00 +58:07:12.4 -- not an asteroid (will add it to exclusion list)
02:29:29.31 +57:10:38.0 -- not an asteroid (will add it to exclusion list)
02:33:27.53 +57:14:42.7 -- not an asteroid (will add it to exclusion list)
02:39:23.81 +58:09:08.6 -- not an asteroid (will add it to exclusion list)
02:25:53.36 +56:14:37.1 -- not an asteroid (will add it to exclusion list)
02:31:12.55 +56:27:35.9 -- not an asteroid (will add it to exclusion list)
02:27:22.07 +56:31:21.0 -- not an asteroid (will add it to exclusion list)
02:25:52.25 +57:02:03.7 -- not an asteroid (will add it to exclusion list)
02:29:04.86 +57:22:34.6 -- not an asteroid (will add it to exclusion list)
02:34:06.59 +56:06:19.6 -- not an asteroid (will add it to exclusion list)
02:25:56.52 +56:32:32.5 -- not an asteroid (will add it to exclusion list)
02:21:19.11 +56:38:13.7 -- not an asteroid (will add it to exclusion list)
02:39:21.43 +58:07:09.6 -- not an asteroid (will add it to exclusion list)
02:28:31.02 +56:40:25.2 -- not an asteroid (will add it to exclusion list)
02:23:08.48 +56:55:24.7 -- not an asteroid (will add it to exclusion list)
02:38:14.36 +57:58:52.1 -- not an asteroid (will add it to exclusion list)
02:31:54.47 +55:50:24.1 -- not an asteroid (will add it to exclusion list)
02:34:32.89 +57:07:24.9 -- not an asteroid (will add it to exclusion list)
02:21:52.35 +56:32:44.4 -- not an asteroid (will add it to exclusion list)
02:26:14.36 +56:12:10.7 -- not an asteroid (will add it to exclusion list)
02:34:18.24 +57:49:31.9 -- not an asteroid (will add it to exclusion list)
02:29:41.72 +56:37:30.4 -- not an asteroid (will add it to exclusion list)
02:30:58.42 +57:16:18.4 -- not an asteroid (will add it to exclusion list)
02:36:12.12 +57:41:55.7 -- not an asteroid (will add it to exclusion list)
02:26:01.05 +56:28:14.9 -- not an asteroid (will add it to exclusion list)
02:22:37.96 +56:37:19.4 -- not an asteroid (will add it to exclusion list)
02:24:27.17 +56:50:29.3 -- not an asteroid (will add it to exclusion list)
02:36:52.73 +57:40:54.2 -- not an asteroid (will add it to exclusion list)
00:58:55.95 +58:04:06.6 -- not an asteroid (will add it to exclusion list)
02:34:27.71 +56:43:27.0 -- not an asteroid (will add it to exclusion list)
02:30:09.40 +57:23:13.6 -- not an asteroid (will add it to exclusion list)
02:29:02.18 +56:24:16.8 -- not an asteroid (will add it to exclusion list)
02:30:26.89 +56:10:14.6 -- not an asteroid (will add it to exclusion list)
02:32:42.22 +57:14:26.4 -- not an asteroid (will add it to exclusion list)
02:36:28.05 +56:50:31.6 -- not an asteroid (will add it to exclusion list)
02:33:18.04 +57:31:36.2 -- not an asteroid (will add it to exclusion list)
02:31:18.63 +57:03:51.6 -- not an asteroid (will add it to exclusion list)
02:36:19.82 +56:57:28.2 -- not an asteroid (will add it to exclusion list)
02:29:25.42 +55:58:54.2 -- not an asteroid (will add it to exclusion list)
02:36:18.15 +56:52:17.8 -- not an asteroid (will add it to exclusion list)
02:34:42.56 +57:17:57.3 -- not an asteroid (will add it to exclusion list)
02:26:58.18 +56:22:09.7 -- not an asteroid (will add it to exclusion list)
02:34:40.76 +56:11:02.3 -- not an asteroid (will add it to exclusion list)
02:33:07.75 +56:14:50.5 -- not an asteroid (will add it to exclusion list)
02:36:19.79 +57:18:00.4 -- not an asteroid (will add it to exclusion list)
02:27:40.45 +56:20:28.8 -- not an asteroid (will add it to exclusion list)
02:23:42.90 +56:38:37.4 -- not an asteroid (will add it to exclusion list)
02:22:22.76 +56:39:59.4 -- not an asteroid (will add it to exclusion list)
02:30:38.78 +56:15:14.6 -- not an asteroid (will add it to exclusion list)
02:33:02.03 +56:26:23.4 -- not an asteroid (will add it to exclusion list)
00:43:47.73 +61:54:01.0 -- not an asteroid (will add it to exclusion list)
02:18:56.11 +56:18:31.6 -- not an asteroid (will add it to exclusion list)
02:33:25.63 +56:59:44.8 -- not an asteroid (will add it to exclusion list)
02:37:55.66 +58:18:21.1 -- not an asteroid (will add it to exclusion list)
02:38:07.48 +58:00:10.7 -- not an asteroid (will add it to exclusion list)
02:26:55.93 +56:28:27.3 -- not an asteroid (will add it to exclusion list)
02:32:05.93 +57:04:59.5 -- not an asteroid (will add it to exclusion list)
01:18:14.25 +61:44:36.4 -- not an asteroid (will add it to exclusion list)
02:33:01.80 +57:36:06.2 -- not an asteroid (will add it to exclusion list)
02:30:49.71 +56:26:27.4 -- not an asteroid (will add it to exclusion list)
02:28:42.38 +55:58:14.1 -- not an asteroid (will add it to exclusion list)
02:31:52.59 +56:53:47.2 -- not an asteroid (will add it to exclusion list)
02:37:59.24 +58:07:39.6 -- not an asteroid (will add it to exclusion list)
02:27:44.77 +56:19:42.5 -- not an asteroid (will add it to exclusion list)
02:33:08.38 +57:21:21.6 -- not an asteroid (will add it to exclusion list)
02:38:19.80 +58:03:54.5 -- not an asteroid (will add it to exclusion list)
02:35:58.83 +57:31:57.8 -- not an asteroid (will add it to exclusion list)
01:29:32.82 +61:46:26.3 -- not an asteroid (will add it to exclusion list)
02:35:43.57 +57:50:30.9 -- not an asteroid (will add it to exclusion list)
02:29:48.85 +56:41:55.4 -- not an asteroid (will add it to exclusion list)
01:22:23.81 +61:13:50.8 -- not an asteroid (will add it to exclusion list)
02:31:18.55 +56:20:48.9 -- not an asteroid (will add it to exclusion list)
02:33:40.20 +57:40:02.4 -- not an asteroid (will add it to exclusion list)
02:17:19.11 +56:42:44.0 -- not an asteroid (will add it to exclusion list)
01:31:28.05 +57:20:36.4 -- not an asteroid (will add it to exclusion list)
02:21:40.76 +60:54:41.6 -- not an asteroid (will add it to exclusion list)
02:15:20.33 +62:13:49.2 -- not an asteroid (will add it to exclusion list)
02:15:35.89 +56:21:36.7 -- not an asteroid (will add it to exclusion list)
02:05:05.69 +58:16:23.9 -- not an asteroid (will add it to exclusion list)
02:19:03.87 +62:47:34.5 -- not an asteroid (will add it to exclusion list)
02:29:57.73 +57:10:58.0 -- not an asteroid (will add it to exclusion list)
02:38:02.15 +58:50:40.7 -- not an asteroid (will add it to exclusion list)
02:34:36.31 +58:11:22.9 -- not an asteroid (will add it to exclusion list)
02:24:29.91 +59:24:30.8 -- not an asteroid (will add it to exclusion list)
01:21:54.72 +61:20:55.4 -- not an asteroid (will add it to exclusion list)
02:25:13.36 +56:30:31.4 -- not an asteroid (will add it to exclusion list)
02:26:44.41 +58:15:51.9 -- not an asteroid (will add it to exclusion list)
02:29:19.57 +57:07:07.2 -- not an asteroid (will add it to exclusion list)
01:27:44.31 +62:06:39.9 -- not an asteroid (will add it to exclusion list)
01:41:46.90 +59:03:47.3 -- not an asteroid (will add it to exclusion list)
02:14:24.94 +56:42:49.3 -- not an asteroid (will add it to exclusion list)
02:08:53.89 +58:42:29.3 -- not an asteroid (will add it to exclusion list)
02:31:45.72 +56:26:45.7 -- not an asteroid (will add it to exclusion list)
02:33:34.77 +57:08:54.4 -- not an asteroid (will add it to exclusion list)
01:32:51.45 +62:40:36.3 -- not an asteroid (will add it to exclusion list)
02:31:42.43 +56:35:52.7 -- not an asteroid (will add it to exclusion list)
02:19:16.63 +59:42:21.5 -- not an asteroid (will add it to exclusion list)
02:29:16.20 +56:24:33.1 -- not an asteroid (will add it to exclusion list)
02:17:01.69 +56:56:08.6 -- not an asteroid (will add it to exclusion list)
02:19:48.16 +56:25:08.9 -- not an asteroid (will add it to exclusion list)
02:15:26.96 +62:47:45.2 -- not an asteroid (will add it to exclusion list)
02:33:31.89 +57:34:08.3 -- not an asteroid (will add it to exclusion list)
01:16:28.98 +60:13:59.7 -- not an asteroid (will add it to exclusion list)
02:28:27.94 +57:25:38.4 -- not an asteroid (will add it to exclusion list)
02:13:41.76 +57:25:36.7 -- not an asteroid (will add it to exclusion list)
02:18:24.65 +58:37:26.1 -- not an asteroid (will add it to exclusion list)
02:33:51.42 +56:10:59.9 -- not an asteroid (will add it to exclusion list)
02:22:56.62 +57:11:45.0 -- not an asteroid (will add it to exclusion list)
02:27:27.68 +56:03:05.8 -- not an asteroid (will add it to exclusion list)
01:30:50.27 +60:32:13.3 -- not an asteroid (will add it to exclusion list)
02:34:12.69 +56:03:50.1 -- not an asteroid (will add it to exclusion list)
02:29:46.25 +56:03:50.4 -- not an asteroid (will add it to exclusion list)
01:24:30.58 +59:38:48.3 -- not an asteroid (will add it to exclusion list)
02:21:26.44 +57:16:58.2 -- not an asteroid (will add it to exclusion list)
02:01:28.14 +58:18:14.4 -- not an asteroid (will add it to exclusion list)
02:29:59.54 +56:13:01.3 -- not an asteroid (will add it to exclusion list)
02:34:05.60 +56:37:26.3 -- not an asteroid (will add it to exclusion list)
02:38:48.25 +57:57:34.8 -- not an asteroid (will add it to exclusion list)
02:27:22.20 +62:38:25.9 -- not an asteroid (will add it to exclusion list)
01:09:38.04 +59:05:14.4 -- not an asteroid (will add it to exclusion list)
02:27:55.40 +56:27:24.2 -- not an asteroid (will add it to exclusion list)
01:14:56.64 +59:42:13.1 -- not an asteroid (will add it to exclusion list)
02:21:35.99 +57:03:40.3 -- not an asteroid (will add it to exclusion list)
02:19:34.14 +58:23:58.2 -- not an asteroid (will add it to exclusion list)
02:31:32.42 +56:47:58.9 -- not an asteroid (will add it to exclusion list)
02:32:22.18 +58:28:54.4 -- not an asteroid (will add it to exclusion list)
02:37:50.81 +57:54:16.4 -- not an asteroid (will add it to exclusion list)
02:00:57.08 +58:36:59.1 -- not an asteroid (will add it to exclusion list)
01:28:36.14 +61:12:06.5 -- not an asteroid (will add it to exclusion list)
01:20:18.33 +64:28:06.2 -- not an asteroid (will add it to exclusion list)
02:31:45.44 +55:57:58.0 -- not an asteroid (will add it to exclusion list)
01:31:04.82 +57:13:13.1 -- not an asteroid (will add it to exclusion list)
02:03:07.50 +57:18:14.2 -- not an asteroid (will add it to exclusion list)
02:33:23.80 +64:24:59.6 -- not an asteroid (will add it to exclusion list)
01:45:16.04 +57:55:47.0 -- not an asteroid (will add it to exclusion list)
02:29:48.53 +57:57:49.9 -- not an asteroid (will add it to exclusion list)
02:13:47.87 +63:11:26.2 -- not an asteroid (will add it to exclusion list)
01:43:45.27 +58:23:44.4 -- not an asteroid (will add it to exclusion list)
02:41:04.47 +62:17:31.2 -- not an asteroid (will add it to exclusion list)
02:30:52.96 +56:54:19.5 -- not an asteroid (will add it to exclusion list)
02:27:11.38 +56:07:26.5 -- not an asteroid (will add it to exclusion list)
02:31:31.09 +57:22:44.7 -- not an asteroid (will add it to exclusion list)
01:37:01.32 +61:15:57.4 -- not an asteroid (will add it to exclusion list)
02:18:22.53 +58:47:08.9 -- not an asteroid (will add it to exclusion list)
02:28:34.52 +56:03:00.1 -- not an asteroid (will add it to exclusion list)
01:35:09.79 +60:17:09.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:30:33.64 +66:05:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:55.27 +62:40:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:45.77 +63:38:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:47.73 +61:54:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:55.95 +58:04:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:38.04 +59:05:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:56.64 +59:42:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:28.98 +60:13:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:14.25 +61:44:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:18.33 +64:28:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:54.72 +61:20:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:23.81 +61:13:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:30.58 +59:38:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:31.68 +57:37:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:44.31 +62:06:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:36.14 +61:12:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.82 +61:46:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:50.27 +60:32:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:04.82 +57:13:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:28.05 +57:20:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:51.45 +62:40:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:09.79 +60:17:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:01.32 +61:15:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:22.21 +59:19:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:01.01 +60:52:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:46.90 +59:03:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:36.46 +58:48:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:45.27 +58:23:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:16.04 +57:55:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.10 +59:15:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:57.08 +58:36:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:28.14 +58:18:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:07.50 +57:18:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:05.69 +58:16:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:53.89 +58:42:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:05.47 +57:29:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:41.76 +57:25:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.87 +63:11:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:24.94 +56:42:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:20.33 +62:13:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:26.96 +62:47:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:35.89 +56:21:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:48.70 +56:16:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:52.45 +56:18:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:01.69 +56:56:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:19.11 +56:42:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:01.27 +56:15:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:05.16 +56:15:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:22.53 +58:47:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:23.94 +56:23:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:24.65 +58:37:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:48.46 +56:17:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:48.83 +56:19:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:56.11 +56:18:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:03.87 +62:47:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:16.63 +59:42:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:34.14 +58:23:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:36.34 +56:23:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:36.43 +56:14:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:39.63 +56:20:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:45.14 +57:01:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:46.66 +56:22:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:48.16 +56:25:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:48.61 +56:23:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:52.94 +56:15:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:56.59 +56:13:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:07.37 +56:27:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:11.66 +56:22:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:18.71 +56:31:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:32.12 +56:10:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:54.06 +56:16:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:55.01 +56:23:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:04.80 +56:15:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:13.42 +56:28:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:16.35 +56:23:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:19.11 +56:38:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:20.56 +56:29:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:23.02 +56:39:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:26.44 +57:16:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:27.45 +56:16:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:32.88 +56:13:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:34.57 +56:26:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:35.99 +57:03:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:40.76 +60:54:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:50.35 +56:34:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:52.35 +56:32:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:55.10 +56:20:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:55.21 +56:25:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:59.12 +56:30:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:03.80 +56:31:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:04.44 +57:10:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:06.87 +56:07:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:10.20 +56:24:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:11.90 +56:20:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:16.01 +56:22:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:21.44 +56:34:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:22.76 +56:39:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:31.56 +56:14:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:35.34 +56:18:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:37.96 +56:37:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:47.61 +56:11:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:56.62 +57:11:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:02.10 +56:30:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:07.52 +56:41:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:08.48 +56:55:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:08.55 +56:20:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:11.07 +56:11:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:17.87 +56:42:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:26.39 +56:06:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:35.43 +56:34:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:38.16 +56:39:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:42.80 +56:07:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:42.90 +56:38:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:48.04 +56:47:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:55.69 +56:44:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:56.97 +56:11:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:01.97 +56:49:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:06.51 +56:29:59.7 -- 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)
02:24:11.84 +56:35:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:12.37 +56:49:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:18.80 +56:19:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:18.90 +56:54:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:25.95 +56:32:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:27.17 +56:50:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:29.91 +59:24:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:32.07 +56:43:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:32.58 +57:00:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:33.48 +56:57:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:33.99 +56:52:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:38.05 +56:49:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:38.48 +56:20:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:41.99 +56:55:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:43.69 +56:59:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:46.71 +56:38:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:47.85 +56:36:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:52.39 +56:43:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:53.85 +56:08:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:00.79 +56:51:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:03.10 +56:56:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:04.18 +56:13:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:11.61 +56:17:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:12.14 +58:09:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:13.36 +56:30:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:20.33 +56:12:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:20.43 +56:51:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:27.59 +56:46:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:28.14 +56:11:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:30.05 +56:16:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:32.72 +56:32:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:33.83 +56:34:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:40.02 +56:29:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:42.16 +56:37:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:45.47 +56:26:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:48.33 +56:55:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:48.44 +56:32:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:52.25 +57:02:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:52.68 +56:47:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:53.36 +56:14:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:55.90 +56:58:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:56.52 +56:32:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:56.77 +56:07:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:00.85 +56:46:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:01.05 +56:28:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:02.34 +56:21:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:07.39 +56:25:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:08.81 +56:16:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:10.78 +56:48:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:11.61 +56:56:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:13.32 +56:36:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:14.36 +56:12:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:15.74 +56:04:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:43.12 +56:24:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:44.41 +58:15:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:48.88 +55:59:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:55.66 +56:30:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:55.93 +56:28:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:58.18 +56:22:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:59.12 +56:01:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:59.37 +57:14:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:07.63 +56:00:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:07.76 +56:33:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:11.38 +56:07:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:15.92 +56:00:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:20.56 +56:01:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:22.07 +56:31:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:22.20 +62:38:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:22.97 +56:19:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:23.30 +55:57:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:24.36 +56:23:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:27.08 +56:31:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:27.68 +56:03:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:33.21 +56:13:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:34.54 +56:16:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:37.42 +57:04:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:40.45 +56:20:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:42.05 +56:12:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:44.77 +56:19:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:48.50 +57:05:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:52.24 +56:29:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:53.50 +57:06:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:55.40 +56:27:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:57.93 +56:02:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:59.47 +56:29:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:59.54 +56:09:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:01.24 +56:23:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:09.55 +56:10:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:10.62 +56:06:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:21.40 +55:58:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:27.94 +57:25:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:31.02 +56:40:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:31.63 +56:00:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:34.52 +56:03:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:34.73 +56:13:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:40.95 +56:12:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:42.38 +55:58:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:48.14 +56:30:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:48.94 +56:07:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:50.78 +56:20:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:56.59 +56:11:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:57.12 +57:06:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:02.18 +56:24:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:04.86 +57:22:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:09.11 +56:37:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:09.98 +56:27:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:10.75 +55:58:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:11.14 +57:21:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:11.88 +56:17:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:16.20 +56:24:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:17.15 +57:14:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:19.57 +57:07:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:25.42 +55:58:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:26.52 +56:00:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:28.33 +56:33:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:29.31 +57:10:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:32.65 +55:57:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:33.78 +56:09:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:38.91 +56:20:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:38.97 +56:11:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:40.57 +56:18:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:40.82 +56:20:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:41.72 +56:37:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:43.00 +56:05:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:46.25 +56:03:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:48.53 +57:57:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:48.85 +56:41:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:50.49 +56:19:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:55.76 +56:55:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:57.46 +56:36:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:57.73 +57:10:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:58.05 +56:08:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:59.54 +56:13:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:00.33 +57:11:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:00.36 +56:17:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:00.36 +57:28:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:03.56 +56:22:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:05.86 +57:18:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:07.04 +56:30:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:09.40 +57:23:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:12.39 +56:11:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:17.06 +56:38:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:18.83 +55:54:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:23.25 +56:23:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:26.89 +56:10:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:28.93 +56:19:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:30.77 +57:30:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:32.08 +57:11:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:32.60 +57:32:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:33.06 +56:53:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:33.43 +56:57:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:34.92 +56:43:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:37.28 +56:22:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:38.21 +56:11:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:38.78 +56:15:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:39.36 +57:13:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:41.06 +55:56:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:42.09 +57:22:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:43.84 +55:58:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:44.93 +56:56:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:45.38 +57:06:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:49.36 +56:11:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:49.71 +56:26:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:51.32 +57:16:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:51.75 +57:15:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:51.92 +57:04:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:52.96 +56:54:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:53.64 +56:14:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:58.42 +57:16:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:59.05 +56:08:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:00.03 +56:00:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:02.85 +57:39:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:03.02 +55:52:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:05.86 +56:37:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:06.51 +56:30:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:09.67 +57:16:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:10.50 +57:30:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:11.42 +56:38:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:11.98 +57:09:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:12.55 +56:27:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:12.59 +57:00:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.30 +55:53:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.55 +56:20:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.63 +57:03:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:19.74 +56:52:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:20.20 +57:33:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:25.66 +55:59:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:25.67 +56:07:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:29.13 +57:11:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:29.40 +56:26:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:31.09 +57:22:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:32.42 +56:47:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:37.57 +56:33:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:38.41 +57:13:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:42.43 +56:35:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:43.43 +56:14:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:45.44 +55:57:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:45.72 +56:26:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:45.76 +57:14:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:46.58 +55:52:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:51.47 +56:45:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:52.59 +56:53:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:54.47 +55:50:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:58.58 +56:42:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:01.35 +56:51:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:04.85 +56:49:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:04.85 +56:53:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:05.00 +56:39:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:05.68 +57:22:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:05.93 +57:04:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:13.87 +55:56:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:15.38 +56:38:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:17.76 +57:17:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:18.19 +56:21:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:18.81 +56:15:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:22.18 +58:28:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:23.05 +57:38:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:25.76 +56:47:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:30.78 +56:47:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:31.36 +57:38:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:34.50 +57:29:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:35.10 +57:32:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:37.22 +56:00:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:42.22 +57:14:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:45.28 +57:08:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:46.00 +56:48:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:47.60 +57:14:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:49.37 +57:34:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:49.88 +56:14:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:55.20 +56:39:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:55.55 +57:08:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:59.21 +57:28:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:01.80 +57:36:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:01.81 +57:02:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:02.03 +56:26:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:03.17 +57:03:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:05.09 +56:13:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:06.29 +56:00:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:07.75 +56:14:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:08.16 +57:28:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:08.38 +57:21:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:09.16 +57:00:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:10.54 +57:32:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:11.61 +57:36:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:18.04 +57:31:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:23.59 +57:33:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:23.80 +64:24:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:25.63 +56:59:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:27.53 +57:14:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:28.12 +56:18:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:30.04 +57:42:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:30.70 +57:29:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:30.84 +56:43:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:31.89 +57:34:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:33.49 +55:49:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:33.86 +56:11:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.24 +55:54:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.77 +57:08:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:37.62 +57:40:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:38.50 +57:33:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:40.20 +57:40:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:40.64 +57:26:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:42.17 +55:51:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:43.66 +57:36:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:44.26 +56:59:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:48.37 +56:47:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:48.46 +57:01:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:48.54 +55:57:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:49.33 +57:35:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:50.71 +55:59:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:51.42 +56:10:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:57.28 +57:00:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:57.90 +56:36:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:03.05 +56:00:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:03.56 +56:30:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:04.23 +57:32:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:04.55 +56:42:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:05.22 +56:25:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:05.60 +56:37:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:06.59 +56:06:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:09.36 +56:41:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:10.16 +55:50:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:12.55 +56:11:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:12.69 +56:03:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:12.78 +56:12:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.61 +56:18:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.74 +56:19:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:18.24 +57:49:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:19.68 +57:08:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:22.33 +56:20:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:24.38 +57:28:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:25.96 +56:29:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:27.71 +56:43:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:28.42 +56:22:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:32.01 +57:40:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:32.89 +57:07:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:34.19 +56:21:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:34.57 +56:36:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:36.31 +58:11:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:37.56 +56:32:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:40.76 +56:11:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:42.56 +57:17:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:43.40 +56:34:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:43.58 +56:51:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:43.96 +56:06:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:48.58 +57:38:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:00.16 +56:43:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:04.69 +57:26:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:08.68 +57:36:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:12.35 +56:50:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:12.95 +57:56:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:15.88 +56:26:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:18.49 +57:31:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:20.15 +57:29:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:22.14 +56:48:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:26.59 +57:46:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:28.70 +56:28:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:30.16 +57:03:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:33.89 +57:09:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:35.04 +57:33:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:37.81 +57:29:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:41.88 +57:31:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:42.45 +56:44:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:43.57 +57:50:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:47.68 +57:10:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:52.02 +57:47:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:58.83 +57:31:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:07.69 +57:21:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:08.58 +57:39:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:12.12 +57:41:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:18.15 +56:52:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:19.07 +57:07:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:19.41 +57:59:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:19.72 +57:15:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:19.79 +57:18:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:19.82 +56:57:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:22.60 +57:40:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:27.53 +56:56:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:28.05 +56:50:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:28.42 +57:11:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:33.26 +57:54:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:35.00 +57:36:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:36.25 +57:46:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:41.43 +57:37:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:42.69 +57:08:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:49.05 +57:24:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:52.73 +57:40:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:54.41 +57:53:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:55.85 +57:38:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:56.54 +57:06:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:59.39 +57:56:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:01.21 +57:51:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:02.13 +57:41:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:08.47 +57:25:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:15.56 +57:48:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:24.10 +57:31:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:26.82 +58:01:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:27.18 +57:28:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:30.47 +57:39:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:31.30 +57:29:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:36.83 +57:51:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:38.82 +57:43:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:41.06 +57:33:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:47.00 +58:07:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.53 +57:45:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.74 +57:57:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.81 +57:54:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:55.04 +57:39:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:55.66 +58:18:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:59.24 +58:07:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:02.15 +58:50:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:07.48 +58:00:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:13.41 +57:50:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:14.36 +57:58:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:18.06 +57:37:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:19.80 +58:03:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:39.71 +57:47:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:46.64 +57:49:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:48.25 +57:57:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:21.43 +58:07:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:23.81 +58:09:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:58.30 +58:20:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:04.47 +62:17:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:30:33.64 +66:05:36.8 -- not a known variable star
00:36:55.27 +62:40:47.8 -- not a known variable star
00:42:45.77 +63:38:26.5 -- not a known variable star
00:43:47.73 +61:54:01.0 -- not a known variable star
00:58:55.95 +58:04:06.6 -- not a known variable star
01:09:38.04 +59:05:14.4 -- a known variable star
01:14:56.64 +59:42:13.1 -- a known variable star
01:16:28.98 +60:13:59.7 -- a known variable star
01:18:14.25 +61:44:36.4 -- not a known variable star
01:20:18.33 +64:28:06.2 -- a known variable star
01:21:54.72 +61:20:55.4 -- a known variable star
01:22:23.81 +61:13:50.8 -- a known variable star
01:24:30.58 +59:38:48.3 -- a known variable star
01:25:31.68 +57:37:40.0 -- not a known variable star
01:27:44.31 +62:06:39.9 -- a known variable star
01:28:36.14 +61:12:06.5 -- a known variable star
01:29:32.82 +61:46:26.3 -- not a known variable star
01:30:50.27 +60:32:13.3 -- a known variable star
01:31:04.82 +57:13:13.1 -- a known variable star
01:31:28.05 +57:20:36.4 -- a known variable star
01:32:51.45 +62:40:36.3 -- a known variable star
01:35:09.79 +60:17:09.4 -- a known variable star
01:37:01.32 +61:15:57.4 -- a known variable star
01:37:22.21 +59:19:56.8 -- not a known variable star
01:40:01.01 +60:52:39.3 -- not a known variable star
01:41:46.90 +59:03:47.3 -- a known variable star
01:43:36.46 +58:48:08.4 -- a known variable star
01:43:45.27 +58:23:44.4 -- a known variable star
01:45:16.04 +57:55:47.0 -- a known variable star
01:56:38.10 +59:15:33.5 -- a known variable star
02:00:57.08 +58:36:59.1 -- a known variable star
02:01:28.14 +58:18:14.4 -- a known variable star
02:03:07.50 +57:18:14.2 -- a known variable star
02:05:05.69 +58:16:23.9 -- a known variable star
02:08:53.89 +58:42:29.3 -- a known variable star
02:09:05.47 +57:29:28.7 -- not a known variable star
02:13:41.76 +57:25:36.7 -- not a known variable star
02:13:47.87 +63:11:26.2 -- a known variable star
02:14:24.94 +56:42:49.3 -- not a known variable star
02:15:20.33 +62:13:49.2 -- a known variable star
02:15:26.96 +62:47:45.2 -- a known variable star
02:15:35.89 +56:21:36.7 -- not a known variable star
02:16:48.70 +56:16:11.9 -- a known variable star
02:16:52.45 +56:18:44.9 -- not a known variable star
02:17:01.69 +56:56:08.6 -- a known variable star
02:17:19.11 +56:42:44.0 -- not a known variable star
02:18:01.27 +56:15:42.4 -- not a known variable star
02:18:05.16 +56:15:08.3 -- not a known variable star
02:18:22.53 +58:47:08.9 -- a known variable star
02:18:23.94 +56:23:20.9 -- not a known variable star
02:18:24.65 +58:37:26.1 -- a known variable star
02:18:48.46 +56:17:54.5 -- a known variable star
02:18:48.83 +56:19:01.6 -- not a known variable star
02:18:56.11 +56:18:31.6 -- not a known variable star
02:19:03.87 +62:47:34.5 -- a known variable star
02:19:16.63 +59:42:21.5 -- a known variable star
02:19:34.14 +58:23:58.2 -- a known variable star
02:19:36.34 +56:23:22.7 -- a known variable star
02:19:36.43 +56:14:20.7 -- not a known variable star
02:19:39.63 +56:20:11.7 -- not a known variable star
02:19:45.14 +57:01:17.6 -- not a known variable star
02:19:46.66 +56:22:25.8 -- not a known variable star
02:19:48.16 +56:25:08.9 -- a known variable star
02:19:48.61 +56:23:45.8 -- not a known variable star
02:19:52.94 +56:15:40.6 -- not a known variable star
02:19:56.59 +56:13:25.6 -- not a known variable star
02:20:07.37 +56:27:51.6 -- not a known variable star
02:20:11.66 +56:22:21.1 -- a known variable star
02:20:18.71 +56:31:49.9 -- a known variable star
02:20:32.12 +56:10:01.0 -- not a known variable star
02:20:54.06 +56:16:37.3 -- a known variable star
02:20:55.01 +56:23:18.7 -- a known variable star
02:21:04.80 +56:15:33.0 -- a known variable star
02:21:13.42 +56:28:43.4 -- not a known variable star
02:21:16.35 +56:23:42.9 -- not a known variable star
02:21:19.11 +56:38:13.7 -- not a known variable star
02:21:20.56 +56:29:12.2 -- not a known variable star
02:21:23.02 +56:39:00.5 -- not a known variable star
02:21:26.44 +57:16:58.2 -- not a known variable star
02:21:27.45 +56:16:27.4 -- not a known variable star
02:21:32.88 +56:13:40.8 -- not a known variable star
02:21:34.57 +56:26:43.6 -- not a known variable star
02:21:35.99 +57:03:40.3 -- a known variable star
02:21:40.76 +60:54:41.6 -- a known variable star
02:21:50.35 +56:34:31.6 -- not a known variable star
02:21:52.35 +56:32:44.4 -- not a known variable star
02:21:55.10 +56:20:50.0 -- not a known variable star
02:21:55.21 +56:25:08.8 -- not a known variable star
02:21:59.12 +56:30:01.8 -- a known variable star
02:22:03.80 +56:31:26.9 -- not a known variable star
02:22:04.44 +57:10:39.1 -- a known variable star
02:22:06.87 +56:07:53.3 -- a known variable star
02:22:10.20 +56:24:23.0 -- not a known variable star
02:22:11.90 +56:20:47.6 -- not a known variable star
02:22:16.01 +56:22:42.1 -- not a known variable star
02:22:21.44 +56:34:17.9 -- not a known variable star
02:22:22.76 +56:39:59.4 -- not a known variable star
02:22:31.56 +56:14:11.4 -- a known variable star
02:22:35.34 +56:18:13.6 -- not a known variable star
02:22:37.96 +56:37:19.4 -- not a known variable star
02:22:47.61 +56:11:10.3 -- not a known variable star
02:22:56.62 +57:11:45.0 -- not a known variable star
02:23:02.10 +56:30:28.6 -- not a known variable star
02:23:07.52 +56:41:45.7 -- not a known variable star
02:23:08.48 +56:55:24.7 -- a known variable star
02:23:08.55 +56:20:25.7 -- not a known variable star
02:23:11.07 +56:11:20.3 -- not a known variable star
02:23:17.87 +56:42:24.1 -- a known variable star
02:23:26.39 +56:06:42.0 -- not a known variable star
02:23:35.43 +56:34:27.3 -- a known variable star
02:23:38.16 +56:39:53.3 -- not a known variable star
02:23:42.80 +56:07:10.6 -- not a known variable star
02:23:42.90 +56:38:37.4 -- not a known variable star
02:23:48.04 +56:47:01.7 -- not a known variable star
02:23:55.69 +56:44:44.9 -- not a known variable star
02:23:56.97 +56:11:52.3 -- not a known variable star
02:24:01.97 +56:49:23.4 -- not a known variable star
02:24:06.51 +56:29:59.7 -- not a known variable star
02:24:09.75 +56:34:02.5 -- not a known variable star
02:24:11.84 +56:35:43.1 -- not a known variable star
02:24:12.37 +56:49:24.7 -- not a known variable star
02:24:18.80 +56:19:50.2 -- not a known variable star
02:24:18.90 +56:54:02.0 -- a known variable star
02:24:25.95 +56:32:57.3 -- not a known variable star
02:24:27.17 +56:50:29.3 -- not a known variable star
02:24:29.91 +59:24:30.8 -- a known variable star
02:24:32.07 +56:43:35.5 -- not a known variable star
02:24:32.58 +57:00:45.4 -- a known variable star
02:24:33.48 +56:57:19.3 -- not a known variable star
02:24:33.99 +56:52:59.9 -- not a known variable star
02:24:38.05 +56:49:55.5 -- not a known variable star
02:24:38.48 +56:20:47.1 -- not a known variable star
02:24:41.99 +56:55:48.0 -- not a known variable star
02:24:43.69 +56:59:33.9 -- not a known variable star
02:24:46.71 +56:38:57.2 -- not a known variable star
02:24:47.85 +56:36:57.7 -- a known variable star
02:24:52.39 +56:43:11.8 -- not a known variable star
02:24:53.85 +56:08:46.7 -- not a known variable star
02:25:00.79 +56:51:32.4 -- not a known variable star
02:25:03.10 +56:56:58.5 -- not a known variable star
02:25:04.18 +56:13:07.6 -- not a known variable star
02:25:11.61 +56:17:21.6 -- not a known variable star
02:25:12.14 +58:09:07.0 -- not a known variable star
02:25:13.36 +56:30:31.4 -- not a known variable star
02:25:20.33 +56:12:13.7 -- not a known variable star
02:25:20.43 +56:51:13.3 -- not a known variable star
02:25:27.59 +56:46:56.3 -- not a known variable star
02:25:28.14 +56:11:20.3 -- not a known variable star
02:25:30.05 +56:16:52.2 -- a known variable star
02:25:32.72 +56:32:56.9 -- not a known variable star
02:25:33.83 +56:34:21.8 -- not a known variable star
02:25:40.02 +56:29:21.1 -- not a known variable star
02:25:42.16 +56:37:12.1 -- a known variable star
02:25:45.47 +56:26:30.9 -- not a known variable star
02:25:48.33 +56:55:12.6 -- not a known variable star
02:25:48.44 +56:32:34.9 -- a known variable star
02:25:52.25 +57:02:03.7 -- not a known variable star
02:25:52.68 +56:47:30.2 -- not a known variable star
02:25:53.36 +56:14:37.1 -- not a known variable star
02:25:55.90 +56:58:59.9 -- not a known variable star
02:25:56.52 +56:32:32.5 -- not a known variable star
02:25:56.77 +56:07:50.4 -- not a known variable star
02:26:00.85 +56:46:18.6 -- not a known variable star
02:26:01.05 +56:28:14.9 -- a known variable star
02:26:02.34 +56:21:00.8 -- not a known variable star
02:26:07.39 +56:25:11.4 -- not a known variable star
02:26:08.81 +56:16:07.7 -- a known variable star
02:26:10.78 +56:48:29.0 -- not a known variable star
02:26:11.61 +56:56:03.9 -- not a known variable star
02:26:13.32 +56:36:46.9 -- not a known variable star
02:26:14.36 +56:12:10.7 -- not a known variable star
02:26:15.74 +56:04:34.8 -- not a known variable star
02:26:43.12 +56:24:13.3 -- not a known variable star
02:26:44.41 +58:15:51.9 -- not a known variable star
02:26:48.88 +55:59:11.6 -- not a known variable star
02:26:55.66 +56:30:19.4 -- not a known variable star
02:26:55.93 +56:28:27.3 -- not a known variable star
02:26:58.18 +56:22:09.7 -- a known variable star
02:26:59.12 +56:01:57.0 -- not a known variable star
02:26:59.37 +57:14:45.3 -- a known variable star
02:27:07.63 +56:00:29.5 -- not a known variable star
02:27:07.76 +56:33:53.6 -- not a known variable star
02:27:11.38 +56:07:26.5 -- not a known variable star
02:27:15.92 +56:00:28.3 -- not a known variable star
02:27:20.56 +56:01:48.1 -- not a known variable star
02:27:22.07 +56:31:21.0 -- a known variable star
02:27:22.20 +62:38:25.9 -- a known variable star
02:27:22.97 +56:19:27.7 -- a known variable star
02:27:23.30 +55:57:43.1 -- a known variable star
02:27:24.36 +56:23:03.8 -- a known variable star
02:27:27.08 +56:31:12.3 -- not a known variable star
02:27:27.68 +56:03:05.8 -- not a known variable star
02:27:33.21 +56:13:10.2 -- not a known variable star
02:27:34.54 +56:16:51.2 -- not a known variable star
02:27:37.42 +57:04:56.0 -- a known variable star
02:27:40.45 +56:20:28.8 -- not a known variable star
02:27:42.05 +56:12:16.6 -- not a known variable star
02:27:44.77 +56:19:42.5 -- not a known variable star
02:27:48.50 +57:05:55.4 -- a known variable star
02:27:52.24 +56:29:30.2 -- not a known variable star
02:27:53.50 +57:06:30.2 -- not a known variable star
02:27:55.40 +56:27:24.2 -- a known variable star
02:27:57.93 +56:02:37.4 -- not a known variable star
02:27:59.47 +56:29:43.8 -- not a known variable star
02:27:59.54 +56:09:19.1 -- not a known variable star
02:28:01.24 +56:23:31.7 -- not a known variable star
02:28:09.55 +56:10:49.3 -- not a known variable star
02:28:10.62 +56:06:42.3 -- not a known variable star
02:28:21.40 +55:58:55.7 -- not a known variable star
02:28:27.94 +57:25:38.4 -- a known variable star
02:28:31.02 +56:40:25.2 -- not a known variable star
02:28:31.63 +56:00:35.4 -- not a known variable star
02:28:34.52 +56:03:00.1 -- not a known variable star
02:28:34.73 +56:13:02.0 -- not a known variable star
02:28:40.95 +56:12:03.5 -- a known variable star
02:28:42.38 +55:58:14.1 -- not a known variable star
02:28:48.14 +56:30:08.1 -- not a known variable star
02:28:48.94 +56:07:35.3 -- a known variable star
02:28:50.78 +56:20:48.8 -- not a known variable star
02:28:56.59 +56:11:02.8 -- a known variable star
02:28:57.12 +57:06:16.3 -- not a known variable star
02:29:02.18 +56:24:16.8 -- not a known variable star
02:29:04.86 +57:22:34.6 -- not a known variable star
02:29:09.11 +56:37:12.5 -- not a known variable star
02:29:09.98 +56:27:11.8 -- not a known variable star
02:29:10.75 +55:58:47.7 -- not a known variable star
02:29:11.14 +57:21:01.2 -- not a known variable star
02:29:11.88 +56:17:58.5 -- not a known variable star
02:29:16.20 +56:24:33.1 -- not a known variable star
02:29:17.15 +57:14:29.9 -- not a known variable star
02:29:19.57 +57:07:07.2 -- a known variable star
02:29:25.42 +55:58:54.2 -- a known variable star
02:29:26.52 +56:00:56.6 -- not a known variable star
02:29:28.33 +56:33:05.7 -- a known variable star
02:29:29.31 +57:10:38.0 -- not a known variable star
02:29:32.65 +55:57:16.0 -- not a known variable star
02:29:33.78 +56:09:10.9 -- not a known variable star
02:29:38.91 +56:20:56.3 -- not a known variable star
02:29:38.97 +56:11:32.5 -- a known variable star
02:29:40.57 +56:18:39.2 -- not a known variable star
02:29:40.82 +56:20:03.6 -- not a known variable star
02:29:41.72 +56:37:30.4 -- not a known variable star
02:29:43.00 +56:05:10.4 -- not a known variable star
02:29:46.25 +56:03:50.4 -- not a known variable star
02:29:48.53 +57:57:49.9 -- not a known variable star
02:29:48.85 +56:41:55.4 -- not a known variable star
02:29:50.49 +56:19:09.0 -- not a known variable star
02:29:55.76 +56:55:49.8 -- not a known variable star
02:29:57.46 +56:36:50.9 -- not a known variable star
02:29:57.73 +57:10:58.0 -- not a known variable star
02:29:58.05 +56:08:50.3 -- not a known variable star
02:29:59.54 +56:13:01.3 -- not a known variable star
02:30:00.33 +57:11:29.3 -- not a known variable star
02:30:00.36 +56:17:43.0 -- not a known variable star
02:30:00.36 +57:28:19.5 -- not a known variable star
02:30:03.56 +56:22:32.1 -- not a known variable star
02:30:05.86 +57:18:33.7 -- not a known variable star
02:30:07.04 +56:30:20.7 -- a known variable star
02:30:09.40 +57:23:13.6 -- not a known variable star
02:30:12.39 +56:11:25.0 -- a known variable star
02:30:17.06 +56:38:11.7 -- not a known variable star
02:30:18.83 +55:54:55.5 -- not a known variable star
02:30:23.25 +56:23:34.2 -- not a known variable star
02:30:26.89 +56:10:14.6 -- not a known variable star
02:30:28.93 +56:19:35.0 -- not a known variable star
02:30:30.77 +57:30:27.1 -- not a known variable star
02:30:32.08 +57:11:25.7 -- not a known variable star
02:30:32.60 +57:32:13.7 -- not a known variable star
02:30:33.06 +56:53:09.3 -- not a known variable star
02:30:33.43 +56:57:01.0 -- not a known variable star
02:30:34.92 +56:43:56.7 -- not a known variable star
02:30:37.28 +56:22:56.7 -- a known variable star
02:30:38.21 +56:11:54.0 -- not a known variable star
02:30:38.78 +56:15:14.6 -- not a known variable star
02:30:39.36 +57:13:43.1 -- not a known variable star
02:30:41.06 +55:56:25.5 -- a known variable star
02:30:42.09 +57:22:37.0 -- not a known variable star
02:30:43.84 +55:58:10.7 -- not a known variable star
02:30:44.93 +56:56:12.3 -- not a known variable star
02:30:45.38 +57:06:30.4 -- not a known variable star
02:30:49.36 +56:11:02.6 -- not a known variable star
02:30:49.71 +56:26:27.4 -- not a known variable star
02:30:51.32 +57:16:48.9 -- not a known variable star
02:30:51.75 +57:15:44.4 -- not a known variable star
02:30:51.92 +57:04:10.4 -- not a known variable star
02:30:52.96 +56:54:19.5 -- a known variable star
02:30:53.64 +56:14:28.0 -- not a known variable star
02:30:58.42 +57:16:18.4 -- not a known variable star
02:30:59.05 +56:08:44.3 -- not a known variable star
02:31:00.03 +56:00:28.9 -- not a known variable star
02:31:02.85 +57:39:55.6 -- not a known variable star
02:31:03.02 +55:52:01.4 -- not a known variable star
02:31:05.86 +56:37:18.2 -- not a known variable star
02:31:06.51 +56:30:41.5 -- not a known variable star
02:31:09.67 +57:16:15.4 -- not a known variable star
02:31:10.50 +57:30:48.1 -- a known variable star
02:31:11.42 +56:38:16.1 -- not a known variable star
02:31:11.98 +57:09:48.2 -- not a known variable star
02:31:12.55 +56:27:35.9 -- a known variable star
02:31:12.59 +57:00:49.8 -- not a known variable star
02:31:18.30 +55:53:50.8 -- not a known variable star
02:31:18.55 +56:20:48.9 -- not a known variable star
02:31:18.63 +57:03:51.6 -- a known variable star
02:31:19.74 +56:52:40.3 -- not a known variable star
02:31:20.20 +57:33:46.6 -- not a known variable star
02:31:25.66 +55:59:07.0 -- a known variable star
02:31:25.67 +56:07:05.3 -- not a known variable star
02:31:29.13 +57:11:55.8 -- not a known variable star
02:31:29.40 +56:26:22.3 -- not a known variable star
02:31:31.09 +57:22:44.7 -- not a known variable star
02:31:32.42 +56:47:58.9 -- not a known variable star
02:31:37.57 +56:33:36.1 -- a known variable star
02:31:38.41 +57:13:47.7 -- not a known variable star
02:31:42.43 +56:35:52.7 -- not a known variable star
02:31:43.43 +56:14:45.0 -- not a known variable star
02:31:45.44 +55:57:58.0 -- not a known variable star
02:31:45.72 +56:26:45.7 -- not a known variable star
02:31:45.76 +57:14:33.8 -- a known variable star
02:31:46.58 +55:52:30.0 -- not a known variable star
02:31:51.47 +56:45:50.3 -- a known variable star
02:31:52.59 +56:53:47.2 -- not a known variable star
02:31:54.47 +55:50:24.1 -- not a known variable star
02:31:58.58 +56:42:23.0 -- not a known variable star
02:32:01.35 +56:51:17.4 -- not a known variable star
02:32:04.85 +56:49:24.8 -- not a known variable star
02:32:04.85 +56:53:51.0 -- not a known variable star
02:32:05.00 +56:39:58.8 -- not a known variable star
02:32:05.68 +57:22:03.0 -- not a known variable star
02:32:05.93 +57:04:59.5 -- not a known variable star
02:32:13.87 +55:56:23.6 -- a known variable star
02:32:15.38 +56:38:50.2 -- not a known variable star
02:32:17.76 +57:17:09.4 -- a known variable star
02:32:18.19 +56:21:26.4 -- not a known variable star
02:32:18.81 +56:15:24.2 -- a known variable star
02:32:22.18 +58:28:54.4 -- not a known variable star
02:32:23.05 +57:38:37.3 -- not a known variable star
02:32:25.76 +56:47:11.8 -- not a known variable star
02:32:30.78 +56:47:59.9 -- not a known variable star
02:32:31.36 +57:38:51.5 -- not a known variable star
02:32:34.50 +57:29:15.5 -- not a known variable star
02:32:35.10 +57:32:19.9 -- not a known variable star
02:32:37.22 +56:00:39.6 -- not a known variable star
02:32:42.22 +57:14:26.4 -- a known variable star
02:32:45.28 +57:08:07.9 -- not a known variable star
02:32:46.00 +56:48:25.9 -- not a known variable star
02:32:47.60 +57:14:18.6 -- a known variable star
02:32:49.37 +57:34:23.1 -- not a known variable star
02:32:49.88 +56:14:34.7 -- a known variable star
02:32:55.20 +56:39:40.1 -- not a known variable star
02:32:55.55 +57:08:54.8 -- not a known variable star
02:32:59.21 +57:28:34.1 -- not a known variable star
02:33:01.80 +57:36:06.2 -- not a known variable star
02:33:01.81 +57:02:07.5 -- a known variable star
02:33:02.03 +56:26:23.4 -- not a known variable star
02:33:03.17 +57:03:28.2 -- not a known variable star
02:33:05.09 +56:13:01.1 -- not a known variable star
02:33:06.29 +56:00:32.4 -- not a known variable star
02:33:07.75 +56:14:50.5 -- not a known variable star
02:33:08.16 +57:28:10.9 -- a known variable star
02:33:08.38 +57:21:21.6 -- not a known variable star
02:33:09.16 +57:00:38.4 -- not a known variable star
02:33:10.54 +57:32:53.9 -- a known variable star
02:33:11.61 +57:36:40.3 -- not a known variable star
02:33:18.04 +57:31:36.2 -- not a known variable star
02:33:23.59 +57:33:31.5 -- not a known variable star
02:33:23.80 +64:24:59.6 -- a known variable star
02:33:25.63 +56:59:44.8 -- not a known variable star
02:33:27.53 +57:14:42.7 -- not a known variable star
02:33:28.12 +56:18:30.6 -- not a known variable star
02:33:30.04 +57:42:18.6 -- a known variable star
02:33:30.70 +57:29:01.5 -- a known variable star
02:33:30.84 +56:43:01.0 -- not a known variable star
02:33:31.89 +57:34:08.3 -- not a known variable star
02:33:33.49 +55:49:25.7 -- not a known variable star
02:33:33.86 +56:11:46.9 -- a known variable star
02:33:34.24 +55:54:24.4 -- not a known variable star
02:33:34.77 +57:08:54.4 -- not a known variable star
02:33:37.62 +57:40:24.0 -- not a known variable star
02:33:38.50 +57:33:38.4 -- a known variable star
02:33:40.20 +57:40:02.4 -- not a known variable star
02:33:40.64 +57:26:09.7 -- not a known variable star
02:33:42.17 +55:51:19.1 -- not a known variable star
02:33:43.66 +57:36:01.4 -- not a known variable star
02:33:44.26 +56:59:33.8 -- not a known variable star
02:33:48.37 +56:47:59.7 -- not a known variable star
02:33:48.46 +57:01:46.2 -- not a known variable star
02:33:48.54 +55:57:07.4 -- not a known variable star
02:33:49.33 +57:35:12.0 -- a known variable star
02:33:50.71 +55:59:56.9 -- not a known variable star
02:33:51.42 +56:10:59.9 -- not a known variable star
02:33:57.28 +57:00:01.2 -- not a known variable star
02:33:57.90 +56:36:42.0 -- not a known variable star
02:34:03.05 +56:00:36.1 -- not a known variable star
02:34:03.56 +56:30:43.8 -- not a known variable star
02:34:04.23 +57:32:43.7 -- not a known variable star
02:34:04.55 +56:42:30.3 -- a known variable star
02:34:05.22 +56:25:31.7 -- not a known variable star
02:34:05.60 +56:37:26.3 -- a known variable star
02:34:06.59 +56:06:19.6 -- a known variable star
02:34:09.36 +56:41:02.1 -- a known variable star
02:34:10.16 +55:50:00.1 -- a known variable star
02:34:12.55 +56:11:53.5 -- not a known variable star
02:34:12.69 +56:03:50.1 -- not a known variable star
02:34:12.78 +56:12:36.7 -- a known variable star
02:34:13.61 +56:18:42.4 -- not a known variable star
02:34:13.74 +56:19:38.4 -- not a known variable star
02:34:18.24 +57:49:31.9 -- a known variable star
02:34:19.68 +57:08:34.6 -- not a known variable star
02:34:22.33 +56:20:27.4 -- not a known variable star
02:34:24.38 +57:28:25.9 -- not a known variable star
02:34:25.96 +56:29:13.8 -- not a known variable star
02:34:27.71 +56:43:27.0 -- not a known variable star
02:34:28.42 +56:22:24.6 -- not a known variable star
02:34:32.01 +57:40:32.0 -- not a known variable star
02:34:32.89 +57:07:24.9 -- not a known variable star
02:34:34.19 +56:21:55.6 -- not a known variable star
02:34:34.57 +56:36:40.8 -- not a known variable star
02:34:36.31 +58:11:22.9 -- a known variable star
02:34:37.56 +56:32:35.4 -- not a known variable star
02:34:40.76 +56:11:02.3 -- not a known variable star
02:34:42.56 +57:17:57.3 -- a known variable star
02:34:43.40 +56:34:06.2 -- a known variable star
02:34:43.58 +56:51:49.8 -- not a known variable star
02:34:43.96 +56:06:06.8 -- not a known variable star
02:34:48.58 +57:38:04.9 -- not a known variable star
02:35:00.16 +56:43:10.4 -- not a known variable star
02:35:04.69 +57:26:54.1 -- not a known variable star
02:35:08.68 +57:36:15.0 -- not a known variable star
02:35:12.35 +56:50:10.1 -- not a known variable star
02:35:12.95 +57:56:23.8 -- not a known variable star
02:35:15.88 +56:26:19.4 -- not a known variable star
02:35:18.49 +57:31:39.8 -- not a known variable star
02:35:20.15 +57:29:29.6 -- not a known variable star
02:35:22.14 +56:48:52.6 -- a known variable star
02:35:26.59 +57:46:13.0 -- not a known variable star
02:35:28.70 +56:28:21.1 -- a known variable star
02:35:30.16 +57:03:30.3 -- not a known variable star
02:35:33.89 +57:09:19.1 -- not a known variable star
02:35:35.04 +57:33:01.8 -- not a known variable star
02:35:37.81 +57:29:13.2 -- not a known variable star
02:35:41.88 +57:31:41.5 -- a known variable star
02:35:42.45 +56:44:19.0 -- a known variable star
02:35:43.57 +57:50:30.9 -- not a known variable star
02:35:47.68 +57:10:24.3 -- not a known variable star
02:35:52.02 +57:47:22.1 -- not a known variable star
02:35:58.83 +57:31:57.8 -- not a known variable star
02:36:07.69 +57:21:39.9 -- not a known variable star
02:36:08.58 +57:39:34.6 -- not a known variable star
02:36:12.12 +57:41:55.7 -- a known variable star
02:36:18.15 +56:52:17.8 -- not a known variable star
02:36:19.07 +57:07:02.5 -- not a known variable star
02:36:19.41 +57:59:11.1 -- a known variable star
02:36:19.72 +57:15:27.8 -- not a known variable star
02:36:19.79 +57:18:00.4 -- not a known variable star
02:36:19.82 +56:57:28.2 -- a known variable star
02:36:22.60 +57:40:05.9 -- not a known variable star
02:36:27.53 +56:56:51.3 -- not a known variable star
02:36:28.05 +56:50:31.6 -- not a known variable star
02:36:28.42 +57:11:45.9 -- not a known variable star
02:36:33.26 +57:54:38.3 -- not a known variable star
02:36:35.00 +57:36:36.2 -- not a known variable star
02:36:36.25 +57:46:59.1 -- not a known variable star
02:36:41.43 +57:37:08.6 -- not a known variable star
02:36:42.69 +57:08:11.5 -- not a known variable star
02:36:49.05 +57:24:45.7 -- not a known variable star
02:36:52.73 +57:40:54.2 -- not a known variable star
02:36:54.41 +57:53:40.3 -- not a known variable star
02:36:55.85 +57:38:50.5 -- not a known variable star
02:36:56.54 +57:06:44.6 -- not a known variable star
02:36:59.39 +57:56:28.2 -- a known variable star
02:37:01.21 +57:51:23.9 -- not a known variable star
02:37:02.13 +57:41:38.8 -- not a known variable star
02:37:08.47 +57:25:21.7 -- not a known variable star
02:37:15.56 +57:48:20.7 -- not a known variable star
02:37:24.10 +57:31:04.5 -- not a known variable star
02:37:26.82 +58:01:13.3 -- not a known variable star
02:37:27.18 +57:28:29.8 -- not a known variable star
02:37:30.47 +57:39:32.1 -- not a known variable star
02:37:31.30 +57:29:01.8 -- not a known variable star
02:37:36.83 +57:51:16.3 -- not a known variable star
02:37:38.82 +57:43:26.3 -- not a known variable star
02:37:41.06 +57:33:22.4 -- not a known variable star
02:37:47.00 +58:07:12.4 -- not a known variable star
02:37:50.53 +57:45:50.6 -- not a known variable star
02:37:50.74 +57:57:57.3 -- not a known variable star
02:37:50.81 +57:54:16.4 -- not a known variable star
02:37:55.04 +57:39:03.5 -- not a known variable star
02:37:55.66 +58:18:21.1 -- not a known variable star
02:37:59.24 +58:07:39.6 -- a known variable star
02:38:02.15 +58:50:40.7 -- not a known variable star
02:38:07.48 +58:00:10.7 -- not a known variable star
02:38:13.41 +57:50:16.7 -- not a known variable star
02:38:14.36 +57:58:52.1 -- not a known variable star
02:38:18.06 +57:37:36.9 -- not a known variable star
02:38:19.80 +58:03:54.5 -- not a known variable star
02:38:39.71 +57:47:02.7 -- not a known variable star
02:38:46.64 +57:49:57.9 -- not a known variable star
02:38:48.25 +57:57:34.8 -- not a known variable star
02:39:21.43 +58:07:09.6 -- not a known variable star
02:39:23.81 +58:09:08.6 -- not a known variable star
02:39:58.30 +58:20:59.8 -- a known variable star
02:41:04.47 +62:17:31.2 -- a known variable star
Found 375 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
502 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 502 (excluding asteroids and hot pixels, 375 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461191.85262890 -observatory V36
05:49:37.40 +25:33:13.5 Mercury (-0.6mag)
07:02:49.31 +24:34:24.5 Venus (-3.9mag)
02:26:55.59 +13:51:56.4 Mars (1.3mag)
07:42:02.72 +21:47:01.3 Jupiter (-1.9mag)
00:47:00.32 +02:35:32.9 Saturn (0.9mag)
03:58:19.47 +20:20:00.1 Uranus (5.8mag)
00:15:37.65 +00:13:52.9 Neptune (7.8mag)
20:33:44.46 -23:01:45.0 Pluto (14.5mag)
16:26:11.47 -27:30:38.6 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 363 May 31 04:37 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461191.85262890:
07:42:00.75 +21:47:05.4 Io (6.0mag)
07:41:53.12 +21:47:29.7 Europa (6.1mag)
07:41:50.10 +21:47:33.9 Ganymede (5.5mag)
07:41:52.69 +21:47:36.2 Callisto (6.8mag)
07:42:48.78 +21:23:07.3 Himalia (15.6mag)
07:42:01.35 +21:47:05.4 Thebe (16.5mag)
07:43:00.44 +21:42:05.0 Elara (17.5mag)
07:43:48.15 +22:02:58.9 Pasiphae (17.7mag)
07:48:57.64 +21:48:10.8 Carme (18.8mag)
00:47:10.62 +02:35:43.6 Titan (8.7mag)
00:46:58.19 +02:35:30.6 Rhea (10.0mag)
00:47:30.48 +02:36:35.8 Iapetus (11.4mag)
00:46:58.38 +02:36:03.5 Hyperion (14.7mag)
00:47:51.96 +02:38:36.5 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 31 04:37 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461191.85262890:
17:21:05.33 -34:18:59.3 JWST
15:03:26.85 +54:31:07.0 Chandra
20:43:18.97 +37:06:20.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 31 04:37 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461191.85262890 -observatory V36
18:48:23.44 -32:03:44.0 13.7mag P/2010 H2 (Vales)
05:45:49.77 -68:10:15.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:46:12.03 +31:52:10.0 17.5mag C/2017 K2 (PANSTARRS)
17:17:51.36 +14:54:11.9 17.8mag C/2021 G2 (ATLAS)
20:08:06.87 -51:31:21.0 17.6mag P/2021 N1 (ZTF)
23:14:00.55 +31:16:25.9 17.2mag C/2022 E2 (ATLAS)
05:24:23.67 +26:54:51.4 16.4mag C/2022 N2 (PANSTARRS)
09:24:18.12 +31:20:26.1 16.6mag C/2022 QE78 (ATLAS)
08:46:30.23 +03:31:23.5 17.6mag C/2022 R6 (PANSTARRS)
18:33:13.09 +21:23:49.4 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:22:20.79 -11:00:55.1 17.5mag P/2023 B1 (PANSTARRS)
22:16:04.76 +66:01:14.4 17.7mag C/2023 H5 (Lemmon)
18:05:18.17 -05:57:52.3 13.7mag C/2023 R1 (PANSTARRS)
13:26:36.38 +84:43:33.6 17.9mag C/2023 X2 (Lemmon)
06:59:55.46 +64:03:57.7 17.6mag C/2024 A1 (ATLAS)
06:35:08.32 +27:03:55.1 13.3mag C/2024 E1 (Wierzchos)
15:43:35.79 +12:46:25.9 17.4mag C/2024 G6 (ATLAS)
20:17:32.59 +28:45:48.0 14.1mag C/2024 J3 (ATLAS)
04:10:09.63 -16:40:49.3 16.1mag C/2024 T5 (ATLAS)
05:58:32.99 +35:52:34.8 17.9mag C/2025 J1 (Borisov)
11:40:15.34 +53:08:55.0 17.1mag C/2025 L1 (ATLAS)
06:34:03.92 -10:29:50.6 13.3mag C/2025 R3 (PANSTARRS)
09:18:08.57 +23:24:33.9 18.0mag C/2025 V2 (Rankin)
12:40:14.29 +04:40:25.8 17.2mag C/2025 Y1 (ATLAS)
01:46:23.48 +42:49:08.3 15.9mag C/2026 B2 (Sun-Gao)
11:10:20.64 -06:44:19.6 16.3mag A/2026 E1
20:09:15.36 -08:11:56.5 9.2mag 10P/Tempel
11:00:26.73 -00:53:12.1 15.9mag 29P/Schwassmann-Wachmann
10:54:54.86 -02:37:03.4 17.9mag 43P/Wolf-Harrington
02:59:32.09 +24:34:15.1 17.6mag 47P/Ashbrook-Jackson
08:43:15.25 +25:57:55.9 16.9mag 63P/Wild
00:19:51.89 -06:54:58.8 15.7mag 65P/Gunn
06:18:08.40 +32:28:49.2 16.7mag 76P/West-Kohoutek-Ikemura
02:50:18.67 +16:09:12.6 13.9mag 78P/Gehrels
01:03:13.68 +03:04:07.8 15.4mag 88P/Howell
04:29:22.61 +29:34:23.0 15.2mag 93P/Lovas
02:21:14.40 +26:17:50.0 17.8mag 114P/Wiseman-Skiff
06:32:00.94 +33:15:11.8 15.7mag 123P/West-Hartley
09:36:41.22 +18:01:03.2 16.5mag 124P/Mrkos
03:46:06.42 +18:41:32.3 16.4mag 128P/Shoemaker-Holt
04:17:55.25 +18:40:24.3 17.7mag 131P/Mueller
05:23:15.32 +19:23:22.3 13.6mag 141P/Machholz
05:25:44.54 +17:02:42.9 13.6mag 141P-A/Machholz
04:13:46.65 +14:50:58.1 10.9mag 141P-D/Machholz
02:52:01.72 -25:50:34.3 17.1mag 161P/Hartley-IRAS
03:16:11.50 +20:31:41.2 14.9mag 162P/SidingSpring
19:36:06.93 -00:25:47.3 17.3mag 169P/NEAT
23:57:03.66 +00:52:44.4 18.0mag 220P/McNaught
16:58:18.80 -08:57:08.0 16.3mag 235P/LINEAR
07:16:50.72 +35:45:24.5 17.4mag 240P/NEAT
00:11:54.52 -05:43:08.6 16.6mag 260P/McNaught
03:43:20.24 +30:58:56.0 17.6mag 295P/LINEAR
22:53:31.66 -20:28:39.6 17.6mag 320P/McNaught
15:19:01.22 +08:18:03.3 17.4mag 391P/Kowalski
08:01:03.10 +20:55:59.7 17.9mag 450P/LONEOS
06:47:10.82 +42:14:27.5 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K May 31 04:37 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.43 -16:06:06.50 ASASSN-26cz 2026-04-22.06 16.26
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
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
19:32:43.68 -22:39:32.70 ASASSN-26cm 2026-04-4.27 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
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
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
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
-rw-r--r-- 1 apache apache 5.6K May 31 04:37 asassn_transients_list.txt
############################################################
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 31 04:37 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:57:07.722 +64:54:01.31 AT 2026neg 2026-05-16.39 20.4372
17:23:00.229 +49:54:27.70 AT 2026nef 2026-05-12.36 21.147
19:15:09.705 +71:42:45.58 AT 2026nee 2026-05-08.41 19.4072
18:15:07.464 +60:42:25.02 AT 2026ned 2026-05-12.37 20.8746
12:24:19.245 +58:53:27.37 AT 2026nec 2026-05-16.28 20.6431
17:56:12.972 +18:10:24.42 AT 2026neb 2026-05-20.06 19.38
14:52:56.305 +52:50:14.00 AT 2026nea 2026-05-16.30 21.2345
14:25:02.106 +32:09:59.37 AT 2026ndz 2026-05-14.38 21.0821
14:52:59.767 +27:53:45.66 AT 2026ndy 2026-05-15.31 20.6613
14:37:16.214 +14:42:45.23 SN 2026ndx 2026-05-16.25 20.6354
14:13:31.790 +04:45:16.38 SN 2026ndw 2026-05-19.26 18.5483
09:55:44.174 +02:45:45.31 AT 2026ndv 2026-05-12.00 22.84
14:43:44.315 +49:43:35.97 AT 2026ndu 2026-05-03.46 20.86
14:45:24.035 +50:25:35.75 AT 2026ndt 2026-05-18.36 20.02
18:04:37.380 -51:12:10.70 AT 2026nds 2026-05-19.19 19.364
17:37:10.989 -81:26:31.03 AT 2026ndr 2026-05-19.25 19.303
10:15:01.129 -45:58:21.05 AT 2026ndq 2026-05-19.04 19.416
19:56:09.761 -48:38:10.36 AT 2026ndp 2026-05-19.32 18.727
00:11:56.324 -43:41:26.71 AT 2026ndo 2026-05-19.40 18.981
16:35:04.502 -82:48:31.63 AT 2026ndn 2026-05-19.22 19.089
-rw-r--r-- 1 apache apache 30K May 31 04:37 tns_transients_list.txt
