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_052435_TTUQ1b1x1_1136561_iesUTh2n
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 31.4332 2461191.9332 9.86 02:21:40.73 +60:54:42.6
133.68142 -0.06250 galactic Cas Second-epoch detections are separated by 0.3" and 2.1 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 02:21:40.73 +60:54:42.6: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.73 +60:54:42.6: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 02 21 40.73 +60 54 42.6 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
DE Cas,2461191.9332,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DE Cas 20260531.4332 9.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.49 01:30:59.69 +63:14:35.6
127.36679 0.71259 galactic Cas Second-epoch detections are separated by 1.2" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:30:59.69 +63:14:35.6 (user input) | T | P | (position from user input) J-Ks=0.876+/-0.036 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:59.69 +63:14:35.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:59.69 +63:14:35.6: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 30 59.69 +63 14 35.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.49,0.05,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
target 20260531.4332 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.44 01:33:01.77 +59:16:33.3
128.23077 -3.16726 galactic Cas Second-epoch detections are separated by 3.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J013303.78+591550.3 | 01:33:03.78 +59:15:50.3 (Gaia DR3) | SRS (local) | 16.088000000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.396+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:01.77 +59:16:33.3: 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 01:33:01.77 +59:16:33.3: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 33 01.77 +59 16 33.3 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013303.78+591550.3,2461191.9332,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013303.78+591550.3 20260531.4332 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.23 01:10:07.77 +57:43:55.5
125.43442 -5.04882 galactic Cas Second-epoch detections are separated by 2.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:10:07.77 +57:43:55.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.731+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:07.77 +57:43:55.5: 11.93 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:07.77 +57:43:55.5: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 31.4332* 01 10 07.77 +57 43 55.5 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.23,0.05,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
target 20260531.4332 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.23 00:44:53.02 +61:53:14.0
122.15978 -0.97470 galactic Cas Second-epoch detections are separated by 3.2" and 2.0 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 | 00:44:53.02 +61:53:14.0 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:44:53.02 +61:53:14.0: 11.90 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:53.02 +61:53:14.0: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 44 53.02 +61 53 14.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.23,0.05,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
target 20260531.4332 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.20 01:00:39.98 +59:11:28.2
124.11574 -3.65937 galactic Cas Second-epoch detections are separated by 1.6" and 2.3 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 J015.1698+59.1953 | 01:00:39.98 +59:11:28.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:00:39.98 +59:11:28.2: 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 01:00:39.98 +59:11:28.2: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 00 39.98 +59 11 28.2 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J015.1698+59.1953,2461191.9332,11.20,0.05,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 J015.1698+59.1953 20260531.4332 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.21 01:35:49.43 +58:50:38.6
128.65746 -3.53339 galactic Cas Second-epoch detections are separated by 2.4" 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 | target | 01:35:49.43 +58:50:38.6 (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 01:35:49.43 +58:50:38.6: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:49.43 +58:50:38.6: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 35 49.43 +58 50 38.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.21,0.05,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
target 20260531.4332 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.03 01:06:12.88 +59:33:45.3
124.80544 -3.25540 galactic Cas Second-epoch detections are separated by 1.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:12.88 +59:33:45.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:12.88 +59:33:45.3: 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 01:06:12.88 +59:33:45.3: 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 31.4332* 01 06 12.88 +59 33 45.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.03,0.05,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 20260531.4332 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.08 01:08:25.50 +59:48:04.1
125.06952 -3.00009 galactic Cas Second-epoch detections are separated by 1.1" 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 | 01:08:25.50 +59:48:04.1 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.50 +59:48:04.1: 12.34 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.50 +59:48:04.1: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 31.4332* 01 08 25.50 +59 48 04.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.08,0.05,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
target 20260531.4332 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.02 01:16:59.09 +59:52:02.2
126.13707 -2.84539 galactic Cas Second-epoch detections are separated by 0.3" and 2.5 pix
The object was found in VSX 1" Gaia DR3 414255063203488000
Type: ROT
# Max. Min./Amp. JD0 Period
13.530 G 13.560 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 01:16:59.09 +59:52:02.2: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:59.09 +59:52:02.2: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 31.4332* 01 16 59.09 +59 52 02.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414255063203488000,2461191.9332,11.02,0.05,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 414255063203488000 20260531.4332 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.96 01:26:38.88 +59:41:40.0
127.36631 -2.87381 galactic Cas Second-epoch detections are separated by 2.1" and 2.7 pix
The object was found in VSX 4" Gaia DR3 510083239641442688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.660 G 13.680 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:38.88 +59:41:40.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:38.88 +59:41:40.0: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 26 38.88 +59 41 40.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510083239641442688,2461191.9332,10.96,0.05,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 510083239641442688 20260531.4332 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.83 02:47:16.64 +64:40:11.5
134.92566 4.53047 galactic Cas Second-epoch detections are separated by 1.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:47:16.64 +64:40:11.5 (user input) | T | P | (position from user input) J-Ks=1.002+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:47:16.64 +64:40:11.5: 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 02:47:16.64 +64:40:11.5: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 31.4332* 02 47 16.64 +64 40 11.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.83,0.05,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
target 20260531.4332 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.93 00:52:38.59 +58:02:49.0
123.09195 -4.82443 galactic Cas Second-epoch detections are separated by 1.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.1739+58.0472 | 00:52:38.59 +58:02:49.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.311+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:38.59 +58:02:49.0: 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 00:52:38.59 +58:02:49.0: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 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 31.4332* 00 52 38.59 +58 02 49.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J013.1739+58.0472,2461191.9332,10.93,0.05,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
ATO J013.1739+58.0472 20260531.4332 10.93CV 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 31.4332 2461191.9332 10.91 00:44:13.32 +56:48:04.1
121.93872 -6.05669 galactic Cas Second-epoch detections are separated by 0.8" and 2.7 pix
The object was found in VSX 4" Gaia DR3 424525670035286912
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.700 G 13.790 G 0.734350000000 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 00:44:13.32 +56:48:04.1: 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 00:44:13.32 +56:48:04.1: 13.50 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.66 +/- 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 31.4332* 00 44 13.32 +56 48 04.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 424525670035286912,2461191.9332,10.91,0.05,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 424525670035286912 20260531.4332 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.86 01:15:17.38 +57:44:02.4
126.12323 -4.98988 galactic Cas Second-epoch detections are separated by 6.1" 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 J018.8211+57.7311 | 01:15:17.38 +57:44:02.4 (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 01:15:17.38 +57:44:02.4: 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 01:15:17.38 +57:44:02.4: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 31.4332* 01 15 17.38 +57 44 02.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.8211+57.7311,2461191.9332,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.8211+57.7311 20260531.4332 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.92 00:44:18.27 +64:55:14.6
122.17562 2.05945 galactic Cas Second-epoch detections are separated by 1.4" 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 | 00:44:18.27 +64:55:14.6 (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 00:44:18.27 +64:55:14.6: 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 00:44:18.27 +64:55:14.6: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 31.4332* 00 44 18.27 +64 55 14.6 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.92,0.05,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
target 20260531.4332 10.92CV 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 31.4332 2461191.9332 10.83 01:05:37.92 +58:00:04.3
124.81809 -4.81856 galactic Cas Second-epoch detections are separated by 1.9" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:05:37.92 +58:00:04.3 (user input) | T | P | (position from user input) J-Ks=0.692+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:37.92 +58:00:04.3: 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 01:05:37.92 +58:00:04.3: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 31.4332* 01 05 37.92 +58 00 04.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.83,0.05,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
target 20260531.4332 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.89 00:56:49.03 +57:22:46.2
123.66016 -5.48464 galactic Cas Second-epoch detections are separated by 2.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J014.1998+57.3753 | 00:56:49.03 +57:22:46.2 (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 00:56:49.03 +57:22:46.2: 12.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:49.03 +57:22:46.2: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 31.4332* 00 56 49.03 +57 22 46.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J014.1998+57.3753,2461191.9332,10.89,0.05,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 J014.1998+57.3753 20260531.4332 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.92 01:02:12.07 +57:26:33.3
124.38604 -5.39877 galactic Cas Second-epoch detections are separated by 1.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:02:12.07 +57:26:33.3 (user input) | T | P | (position from user input) SpType: A2V (LAMOST DR5) J-Ks=0.395+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:12.07 +57:26:33.3: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:12.07 +57:26:33.3: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 02 12.07 +57 26 33.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.92,0.05,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
target 20260531.4332 10.92CV 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 31.4332 2461191.9332 10.68 02:10:56.02 +62:17:07.8
132.02951 0.82618 galactic Cas Second-epoch detections are separated by 1.2" and 2.3 pix
The object was found in VSX 2" ASASSN-V J021056.24+621707.7
Type: SR
# Max. Min./Amp. JD0 Period
13.610 V 13.700 V 2457406.80000 41.140000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:56.02 +62:17:07.8: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:56.02 +62:17:07.8: 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 31.4332* 02 10 56.02 +62 17 07.8 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
ASASSN-V J021056.24+621707.7,2461191.9332,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J021056.24+621707.7 20260531.4332 10.68CV 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 31.4332 2461191.9332 10.86 00:57:40.76 +56:52:14.1
123.78931 -5.99077 galactic Cas Second-epoch detections are separated by 1.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424002130705145216 | 00:57:43.20 +56:52:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.213+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:57:40.76 +56:52:14.1: 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 00:57:40.76 +56:52:14.1: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 57 40.76 +56 52 14.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 424002130705145216,2461191.9332,10.86,0.05,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 424002130705145216 20260531.4332 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.76 01:25:19.92 +59:52:22.3
127.17813 -2.71915 galactic Cas Second-epoch detections are separated by 4.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510097945609143168 | 01:25:17.72 +59:52:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:19.92 +59:52:22.3: 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 01:25:19.92 +59:52:22.3: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 25 19.92 +59 52 22.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510097945609143168,2461191.9332,10.76,0.05,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 510097945609143168 20260531.4332 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.74 01:20:45.89 +57:55:24.6
126.83108 -4.72605 galactic Cas Second-epoch detections are separated by 0.9" and 2.5 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 413797116609704704 | 01:20:41.29 +57:55:17.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.167+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:45.89 +57:55:24.6: 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 01:20:45.89 +57:55:24.6: 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 31.4332* 01 20 45.89 +57 55 24.6 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413797116609704704,2461191.9332,10.74,0.05,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 413797116609704704 20260531.4332 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.80 01:01:47.58 +57:23:13.9
124.33317 -5.45638 galactic Cas Second-epoch detections are separated by 4.0" 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 J015.4425+57.3932 | 01:01:47.58 +57:23:13.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.712+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:47.58 +57:23:13.9: 11.85 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:47.58 +57:23:13.9: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 01 47.58 +57 23 13.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J015.4425+57.3932,2461191.9332,10.80,0.05,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 J015.4425+57.3932 20260531.4332 10.80CV 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 31.4332 2461191.9332 10.82 01:11:44.61 +61:13:56.2
125.37341 -1.54318 galactic Cas Second-epoch detections are separated by 1.7" and 2.3 pix
The object was found in VSX 1" ZTF J011144.73+611356.9
Type: RS
# Max. Min./Amp. JD0 Period
13.552 r Y 0.107 r 2458423.79830 1.359407700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:44.61 +61:13:56.2: 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 01:11:44.61 +61:13:56.2: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 31.4332* 01 11 44.61 +61 13 56.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011144.73+611356.9,2461191.9332,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011144.73+611356.9 20260531.4332 10.82CV 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 31.4332 2461191.9332 10.89 00:36:45.76 +61:48:23.5
121.19923 -1.01584 galactic Cas Second-epoch detections are separated by 0.8" and 2.7 pix
The object was found in VSX10" Gaia DR3 430273848108689536
Type: S
# Max. Min./Amp. JD0 Period
16.890 G 17.860 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 00:36:45.76 +61:48:23.5: 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 00:36:45.76 +61:48:23.5: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 36 45.76 +61 48 23.5 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430273848108689536,2461191.9332,10.89,0.05,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 430273848108689536 20260531.4332 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.78 00:56:04.04 +60:39:34.5
123.49941 -2.20706 galactic Cas Second-epoch detections are separated by 1.1" and 2.7 pix
The object was found in VSX21" Gaia DR3 426535336777707520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.420 G 13.460 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 00:56:04.04 +60:39:34.5: 11.11 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:04.04 +60:39:34.5: 13.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 31.4332* 00 56 04.04 +60 39 34.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426535336777707520,2461191.9332,10.78,0.05,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 426535336777707520 20260531.4332 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.82 01:22:28.16 +61:07:36.1
126.67052 -1.51960 galactic Cas Second-epoch detections are separated by 2.3" and 2.4 pix
The object was found in VSX23" Gaia DR3 510501328936368640
Type: RS
# Max. Min./Amp. JD0 Period
13.970 G 14.040 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:28.16 +61:07:36.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:28.16 +61:07:36.1: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 22 28.16 +61 07 36.1 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510501328936368640,2461191.9332,10.82,0.05,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 510501328936368640 20260531.4332 10.82CV 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 31.4332 2461191.9332 10.69 01:32:21.98 +60:27:29.4
127.95972 -2.01342 galactic Cas Second-epoch detections are separated by 2.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:32:21.98 +60:27:29.4 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:21.98 +60:27:29.4: 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 01:32:21.98 +60:27:29.4: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 31.4332* 01 32 21.98 +60 27 29.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.69,0.05,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
target 20260531.4332 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.62 00:54:30.96 +59:23:59.6
123.32435 -3.46951 galactic Cas Second-epoch detections are separated by 1.4" and 2.8 pix
The object was found in VSX 1" V0415 Cas
Type: EA/DS
# Max. Min./Amp. JD0 Period
14.000 pg 16.800 pg 2429106.58700 12.536157000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:54:30.96 +59:23:59.6: 11.77 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:30.96 +59:23:59.6: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 31.4332* 00 54 30.96 +59 23 59.6 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0415 Cas,2461191.9332,10.62,0.05,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
V0415 Cas 20260531.4332 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.51 01:46:42.34 +61:09:51.6
129.54710 -0.99556 galactic Cas Second-epoch detections are separated by 0.5" and 2.3 pix
The object was found in VSX19" V1156 Cas
Type: BCEP
# Max. Min./Amp. JD0 Period
11.720 I Y 0.030 I 0.276400000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:42.34 +61:09:51.6: 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 01:46:42.34 +61:09:51.6: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 31.4332* 01 46 42.34 +61 09 51.6 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1156 Cas,2461191.9332,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1156 Cas 20260531.4332 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.73 00:56:47.36 +60:38:48.1
123.58817 -2.21824 galactic Cas Second-epoch detections are separated by 3.1" and 2.1 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 426546125736902528 | 00:56:44.52 +60:38:23.6 (Gaia DR3) | DSCT/GDOR (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 00:56:47.36 +60:38:48.1: 10.67 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:47.36 +60:38:48.1: 13.39 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 56 47.36 +60 38 48.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426546125736902528,2461191.9332,10.73,0.05,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 426546125736902528 20260531.4332 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.55 01:02:45.62 +58:39:34.2
124.40767 -4.17980 galactic Cas Second-epoch detections are separated by 0.8" and 2.5 pix
The object was found in VSX20" Gaia DR3 425802855871731072
Type: ROT
# Max. Min./Amp. JD0 Period
12.620 G 12.680 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 01:02:45.62 +58:39:34.2: 12.40 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:45.62 +58:39:34.2: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 02 45.62 +58 39 34.2 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 425802855871731072,2461191.9332,10.55,0.05,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 425802855871731072 20260531.4332 10.55CV 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 31.4332 2461191.9332 10.44 01:15:00.94 +57:58:06.1
126.06510 -4.75988 galactic Cas Second-epoch detections are separated by 2.1" and 2.3 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 J018.7329+57.9628 | 01:15:00.94 +57:58:06.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.087+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:00.94 +57:58:06.1: 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 01:15:00.94 +57:58:06.1: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 31.4332* 01 15 00.94 +57 58 06.1 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.7329+57.9628,2461191.9332,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.7329+57.9628 20260531.4332 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.59 01:30:10.08 +59:36:18.7
127.81973 -2.89850 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 | 01:30:10.08 +59:36:18.7 (user input) | T | P | (position from user input) J-Ks=0.144+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:10.08 +59:36:18.7: 11.63 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:10.08 +59:36:18.7: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 31.4332* 01 30 10.08 +59 36 18.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.59,0.05,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
target 20260531.4332 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.47 00:54:20.36 +57:41:46.4
123.32113 -5.17333 galactic Cas Second-epoch detections are separated by 1.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:54:20.36 +57:41:46.4 (user input) | T | P | (position from user input) J-Ks=0.753+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:54:20.36 +57:41:46.4: 11.27 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:20.36 +57:41:46.4: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 31.4332* 00 54 20.36 +57 41 46.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.47,0.05,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
target 20260531.4332 10.47CV 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 31.4332 2461191.9332 10.38 00:51:09.78 +60:42:30.8
122.89827 -2.16318 galactic Cas Second-epoch detections are separated by 0.7" 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 | target | 00:51:09.78 +60:42:30.8 (user input) | T | P | (position from user input) J-Ks=0.204+/-0.040 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:09.78 +60:42:30.8: 10.29 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:09.78 +60:42:30.8: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.67 +/- 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 31.4332* 00 51 09.78 +60 42 30.8 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
target,2461191.9332,10.38,0.05,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
target 20260531.4332 10.38CV 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 31.4332 2461191.9332 10.49 01:26:05.85 +57:30:37.8
127.59169 -5.04733 galactic Cas Second-epoch detections are separated by 2.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:26:05.85 +57:30:37.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.85 +57:30:37.8: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.85 +57:30:37.8: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 31.4332* 01 26 05.85 +57 30 37.8 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.49,0.05,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
target 20260531.4332 10.49CV 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 31.4332 2461191.9332 10.56 01:17:48.19 +57:17:33.7
126.50380 -5.39609 galactic Cas Second-epoch detections are separated by 3.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:17:48.19 +57:17:33.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:48.19 +57:17:33.7: 12.56 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:48.19 +57:17:33.7: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 17 48.19 +57 17 33.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.56,0.05,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
target 20260531.4332 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.37 01:27:51.63 +56:56:50.7
127.90706 -5.57208 galactic Cas Second-epoch detections are separated by 0.7" and 2.5 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 J021.9604+56.9398 | 01:27:51.20 +56:56:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.418+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:51.63 +56:56:50.7: 13.02 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:51.63 +56:56:50.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 31.4332* 01 27 51.63 +56 56 50.7 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.9604+56.9398,2461191.9332,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.9604+56.9398 20260531.4332 10.37CV 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 31.4332 2461191.9332 10.39 01:01:25.35 +57:50:14.0
124.26547 -5.00867 galactic Cas Second-epoch detections are separated by 1.8" and 2.4 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 J015.3611+57.8296 | 01:01:25.35 +57:50:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.462+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:25.35 +57:50:14.0: 10.61 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:25.35 +57:50:14.0: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 01 25.35 +57 50 14.0 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J015.3611+57.8296,2461191.9332,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J015.3611+57.8296 20260531.4332 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.42 00:56:45.50 +58:52:46.3
123.62099 -3.98510 galactic Cas Second-epoch detections are separated by 0.4" 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 J014.1841+58.8773 | 00:56:42.26 +58:52:33.9 (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 00:56:45.50 +58:52:46.3: 11.45 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:45.50 +58:52:46.3: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 31.4332* 00 56 45.50 +58 52 46.3 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
ATO J014.1841+58.8773,2461191.9332,10.42,0.05,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 J014.1841+58.8773 20260531.4332 10.42CV 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 31.4332 2461191.9332 10.23 00:52:52.78 +58:28:52.0
123.12090 -4.39011 galactic Cas Second-epoch detections are separated by 1.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.2201+58.4812 | 00:52:52.78 +58:28:52.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.728+/-0.025 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:52.78 +58:28:52.0: 10.61 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:52.78 +58:28:52.0: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 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 31.4332* 00 52 52.78 +58 28 52.0 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
ATO J013.2201+58.4812,2461191.9332,10.23,0.05,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
ATO J013.2201+58.4812 20260531.4332 10.23CV 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 31.4332 2461191.9332 10.39 01:25:15.32 +64:40:32.7
126.53975 2.04115 galactic Cas Second-epoch detections are separated by 1.4" and 2.3 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 512840196327698304 | 01:25:16.38 +64:40:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.479+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:15.32 +64:40:32.7: 10.96 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:15.32 +64:40:32.7: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 31.4332* 01 25 15.32 +64 40 32.7 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512840196327698304,2461191.9332,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512840196327698304 20260531.4332 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.30 00:40:25.91 +61:07:15.7
121.60283 -1.72232 galactic Cas Second-epoch detections are separated by 2.2" and 2.3 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 427219056906089600 | 00:40:25.71 +61:07:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:40:25.91 +61:07:15.7: 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 00:40:25.91 +61:07:15.7: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 40 25.91 +61 07 15.7 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 427219056906089600,2461191.9332,10.30,0.05,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 427219056906089600 20260531.4332 10.30CV 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 31.4332 2461191.9332 10.21 00:40:43.95 +61:40:52.1
121.66241 -1.16422 galactic Cas Second-epoch detections are separated by 1.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:40:43.95 +61:40:52.1 (user input) | T | P | (position from user input) 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 00:40:43.95 +61:40:52.1: 12.09 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:40:43.95 +61:40:52.1: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 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 31.4332* 00 40 43.95 +61 40 52.1 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,2461191.9332,10.21,0.05,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
target 20260531.4332 10.21CV 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 31.4332 2461191.9332 10.13 01:25:38.45 +59:16:00.4
127.29701 -3.31478 galactic Cas Second-epoch detections are separated by 0.5" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510043588502369152 | 01:25:40.25 +59:16:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.017+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:38.45 +59:16:00.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:38.45 +59:16:00.4: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 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 31.4332* 01 25 38.45 +59 16 00.4 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510043588502369152,2461191.9332,10.13,0.05,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 510043588502369152 20260531.4332 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.14 01:12:40.83 +61:20:37.3
125.47664 -1.42305 galactic Cas Second-epoch detections are separated by 0.4" and 2.3 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 522563173351220736 | 01:12:36.96 +61:20:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.300+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:40.83 +61:20:37.3: 12.31 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:40.83 +61:20:37.3: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 12 40.83 +61 20 37.3 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522563173351220736,2461191.9332,10.14,0.05,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 522563173351220736 20260531.4332 10.14CV 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 31.4332 2461191.9332 10.07 00:58:00.23 +57:24:06.3
123.82020 -5.45867 galactic Cas Second-epoch detections are separated by 6.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424135377769652480 | 00:58:01.55 +57:24:26.4 (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 00:58:00.23 +57:24:06.3: 11.90 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:00.23 +57:24:06.3: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 58 00.23 +57 24 06.3 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 424135377769652480,2461191.9332,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424135377769652480 20260531.4332 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.16 00:51:25.51 +62:25:15.0
122.93044 -0.45092 galactic Cas Second-epoch detections are separated by 1.0" 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 | Gaia DR3 427541664790555008 | 00:51:25.03 +62:25:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=11.642+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:25.51 +62:25:15.0: 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 00:51:25.51 +62:25:15.0: 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 31.4332* 00 51 25.51 +62 25 15.0 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 427541664790555008,2461191.9332,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427541664790555008 20260531.4332 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 9.96 01:08:09.36 +60:42:14.9
124.97703 -2.10121 galactic Cas Second-epoch detections are separated by 0.4" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:09.36 +60:42:14.9 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:09.36 +60:42:14.9: 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 01:08:09.36 +60:42:14.9: 12.48 +/- 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 31.4332* 01 08 09.36 +60 42 14.9 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,9.96,0.05,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
target 20260531.4332 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 31.4332 2461191.9332 9.92 00:52:22.50 +58:23:34.3
123.05507 -4.47866 galactic Cas Second-epoch detections are separated by 0.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.1235+58.4006 | 00:52:25.14 +58:23:34.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.558+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:22.50 +58:23:34.3: 10.05 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:22.50 +58:23:34.3: 12.40 +/- 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 31.4332* 00 52 22.50 +58 23 34.3 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J013.1235+58.4006,2461191.9332,9.92,0.05,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 J013.1235+58.4006 20260531.4332 9.92CV 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 31.4332 2461191.9332 9.82 00:36:43.38 +64:22:47.7
121.34153 1.55362 galactic Cas Second-epoch detections are separated by 0.9" and 2.5 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 526988329691788928 | 00:36:41.83 +64:22:31.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.519+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:43.38 +64:22:47.7: 12.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:36:43.38 +64:22:47.7: 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 31.4332* 00 36 43.38 +64 22 47.7 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 526988329691788928,2461191.9332,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 526988329691788928 20260531.4332 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 9.45 01:25:56.68 +59:35:12.0
127.29271 -2.99260 galactic Cas Second-epoch detections are separated by 0.6" and 2.4 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 510075336901717632 | 01:25:55.70 +59:34:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +59 169 J-Ks=0.194+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.68 +59:35:12.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:56.68 +59:35:12.0: 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 31.4332* 01 25 56.68 +59 35 12.0 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510075336901717632,2461191.9332,9.45,0.05,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 510075336901717632 20260531.4332 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 31.4332 2461191.9332 8.12 01:32:39.95 +63:11:27.6
127.56089 0.69039 galactic Cas Second-epoch detections are separated by 1.4" and 2.2 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 | ZTF J013244.52+631133.9 | 01:32:42.83 +63:11:29.6 (Gaia DR3) | RS (local) | 2458481.80000 (local) | Gaia3var=NOT_AVAILABLE SpType: A2V 1928MeUpp..37....1S BD+62 263 J-Ks=0.295+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:39.95 +63:11:27.6: 12.70 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:39.95 +63:11:27.6: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 32 39.95 +63 11 27.6 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
ZTF J013244.52+631133.9,2461191.9332,8.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J013244.52+631133.9 20260531.4332 8.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 7.75 01:35:37.54 +61:16:49.5
128.21593 -1.13717 galactic Cas Second-epoch detections are separated by 0.8" and 2.3 pix
The object was found in VSX 9" Gaia DR3 509978579881384704
Type: E
# Max. Min./Amp. JD0 Period
12.390 G 12.580 G 1.177150000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:37.54 +61:16:49.5: 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 01:35:37.54 +61:16:49.5: 10.19 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.19 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 35 37.54 +61 16 49.5 7.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509978579881384704,2461191.9332,7.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509978579881384704 20260531.4332 7.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 7.99 01:02:34.05 +59:16:48.9
124.35561 -3.56073 galactic Cas Second-epoch detections are separated by 0.4" and 2.5 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 J015.6294+59.2876 | 01:02:37.15 +59:17:12.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K2III: 1935BSD...C01....0S BSD 8- 96 J-Ks=1.151+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:34.05 +59:16:48.9: 7.96 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:34.05 +59:16:48.9: 10.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.25 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 02 34.05 +59 16 48.9 8.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J015.6294+59.2876,2461191.9332,7.99,0.05,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 J015.6294+59.2876 20260531.4332 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 31.4332 2461191.9332 8.22 00:52:16.20 +59:42:57.8
123.03698 -3.15552 galactic Cas Second-epoch detections are separated by 0.4" and 2.5 pix
The object was found in VSX19" Gaia DR3 426857150085138176
Type: ROT
# Max. Min./Amp. JD0 Period
14.420 G 14.440 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 00:52:16.20 +59:42:57.8: 8.72 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:16.20 +59:42:57.8: 10.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.28 +/- 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 31.4332* 00 52 16.20 +59 42 57.8 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
Gaia DR3 426857150085138176,2461191.9332,8.22,0.05,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 426857150085138176 20260531.4332 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 31.4332 2461191.9332 8.26 01:47:13.04 +57:44:19.0
130.34390 -4.32820 galactic Cas Second-epoch detections are separated by 0.6" and 2.5 pix
The object was found in VSX 4" Gaia DR3 505962471920178944
Type: VAR
# Max. Min./Amp. JD0 Period
13.440 G 13.470 G 0.024984900000 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 01:47:13.04 +57:44:19.0: 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 01:47:13.04 +57:44:19.0: 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 31.4332* 01 47 13.04 +57 44 19.0 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
Gaia DR3 505962471920178944,2461191.9332,8.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505962471920178944 20260531.4332 8.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 9.15 00:41:14.65 +61:35:30.9
121.71952 -1.25583 galactic Cas Second-epoch detections are separated by 0.2" and 2.6 pix
The object was found in VSX20" ZTF J004114.30+613550.9
Type: EW
# Max. Min./Amp. JD0 Period
19.942 r Y 0.720 r 2458376.85470 0.297943600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:41:14.65 +61:35:30.9: 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 00:41:14.65 +61:35:30.9: 11.95 +/- 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 31.4332* 00 41 14.65 +61 35 30.9 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
ZTF J004114.30+613550.9,2461191.9332,9.15,0.05,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
ZTF J004114.30+613550.9 20260531.4332 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 31.4332 2461191.9332 9.10 01:44:52.13 +57:41:42.0
130.04567 -4.43689 galactic Cas Second-epoch detections are separated by 1.1" and 2.3 pix
The object was found in VSX 2" Gaia DR3 505969726120091264
Type: ROT
# Max. Min./Amp. JD0 Period
11.620 G 11.650 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 01:44:52.13 +57:41:42.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:52.13 +57:41:42.0: 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 31.4332* 01 44 52.13 +57 41 42.0 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
Gaia DR3 505969726120091264,2461191.9332,9.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505969726120091264 20260531.4332 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 31.4332 2461191.9332 9.46 01:46:30.07 +61:12:58.8
129.51198 -0.94998 galactic Cas Second-epoch detections are separated by 0.5" and 2.2 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 | V0983 Cas | 01:46:27.67 +61:12:25.4 (Gaia DR3) | BE (local) | B8II: (local) | Gaia3var=VARIABLE SpType: B6 1933LicOB..16..119Z Cl* NGC 663 Zug 35 J-Ks=0.193+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:30.07 +61:12:58.8: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:30.07 +61:12:58.8: 12.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.17 +/- 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 31.4332* 01 46 30.07 +61 12 58.8 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0983 Cas,2461191.9332,9.46,0.05,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
V0983 Cas 20260531.4332 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 31.4332 2461191.9332 9.62 01:12:05.87 +59:41:19.7
125.53980 -3.07829 galactic Cas Second-epoch detections are separated by 0.2" and 2.5 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 414281520202963072 | 01:12:02.71 +59:41:17.7 (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 01:12:05.87 +59:41:19.7: 13.16 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:05.87 +59:41:19.7: 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 31.4332* 01 12 05.87 +59 41 19.7 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 414281520202963072,2461191.9332,9.62,0.05,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 414281520202963072 20260531.4332 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 31.4332 2461191.9332 9.48 02:19:17.63 +57:07:29.7
134.67097 -3.73086 galactic Per Second-epoch detections are separated by 0.3" and 2.3 pix
The object was found in VSX 1" Gaia DR3 458374547813352832
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.030 G 12.060 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 02:19:17.63 +57:07:29.7: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:17.63 +57:07:29.7: 12.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 31.4332* 02 19 17.63 +57 07 29.7 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 458374547813352832,2461191.9332,9.48,0.05,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 458374547813352832 20260531.4332 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 31.4332 2461191.9332 9.69 01:40:01.44 +60:52:32.0
128.81171 -1.44032 galactic Cas Second-epoch detections are separated by 0.3" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J013956.73+605213.0 | 01:39:56.73 +60:52:13.0 (Gaia DR3) | SR (local) | 450.000000000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:01.44 +60:52:32.0: 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 01:40:01.44 +60:52:32.0: 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 31.4332* 01 40 01.44 +60 52 32.0 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013956.73+605213.0,2461191.9332,9.69,0.05,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
ASASSN-V J013956.73+605213.0 20260531.4332 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 31.4332 2461191.9332 9.77 01:08:15.62 +63:34:13.6
124.80264 0.75982 galactic Cas Second-epoch detections are separated by 0.5" and 2.3 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 523314311588408704 | 01:08:15.64 +63:34:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.177+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:15.62 +63:34:13.6: 10.09 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:15.62 +63:34:13.6: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.55 +/- 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 31.4332* 01 08 15.62 +63 34 13.6 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 523314311588408704,2461191.9332,9.77,0.05,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 523314311588408704 20260531.4332 9.77CV 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 31.4332 2461191.9332 9.88 01:24:27.18 +58:44:16.9
127.21411 -3.85895 galactic Cas Second-epoch detections are separated by 0.6" 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 | Gaia DR3 413947680984528768 | 01:24:32.24 +58:44:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2 1928AnHar.100...49C HD 236718 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 01:24:27.18 +58:44:16.9: 12.81 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:27.18 +58:44:16.9: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 24 27.18 +58 44 16.9 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413947680984528768,2461191.9332,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413947680984528768 20260531.4332 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.00 00:58:55.96 +58:04:04.8
123.92628 -4.78928 galactic Cas Second-epoch detections are separated by 0.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:58:55.96 +58:04:04.8 (user input) | T | P | (position from user input) J-Ks=0.236+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:58:55.96 +58:04:04.8: 12.28 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:55.96 +58:04:04.8: 12.78 +/- 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 31.4332* 00 58 55.96 +58 04 04.8 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,2461191.9332,10.00,0.05,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
target 20260531.4332 10.00CV 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 31.4332 2461191.9332 9.98 01:58:16.32 +59:38:59.0
131.29072 -2.13298 galactic Cas Second-epoch detections are separated by 0.5" and 2.2 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 | 01:58:16.32 +59:38:59.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:16.32 +59:38:59.0: 12.60 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:16.32 +59:38:59.0: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 58 16.32 +59 38 59.0 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,2461191.9332,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260531.4332 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.04 01:18:14.06 +61:44:36.2
126.09825 -0.96351 galactic Cas Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:14.06 +61:44:36.2 (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 01:18:14.06 +61:44:36.2: 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 01:18:14.06 +61:44:36.2: 12.78 +/- 0.02 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 31.4332* 01 18 14.06 +61 44 36.2 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.04,0.05,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
target 20260531.4332 10.04CV 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 31.4332 2461191.9332 10.24 00:52:31.34 +58:35:21.3
123.07360 -4.28220 galactic Cas Second-epoch detections are separated by 1.7" and 2.4 pix
The object was found in VSX21" Gaia DR3 424455816690418176
Type: ROT
# 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 00:52:31.34 +58:35:21.3: 11.01 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:31.34 +58:35:21.3: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 52 31.34 +58 35 21.3 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
Gaia DR3 424455816690418176,2461191.9332,10.24,0.05,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 424455816690418176 20260531.4332 10.24CV 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 31.4332 2461191.9332 10.12 01:07:57.13 +63:37:29.6
124.76492 0.81193 galactic Cas Second-epoch detections are separated by 1.9" and 2.4 pix
The object was found in VSX23" V1064 Cas
Type: EW
# Max. Min./Amp. JD0 Period
11.300 R1 11.800 R1 2451349.91900 0.457606000000 B2
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:57.13 +63:37:29.6: 10.65 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:57.13 +63:37:29.6: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 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 31.4332* 01 07 57.13 +63 37 29.6 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1064 Cas,2461191.9332,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1064 Cas 20260531.4332 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.24 01:29:32.78 +61:46:26.2
127.42204 -0.76512 galactic Cas Second-epoch detections are separated by 0.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:32.78 +61:46:26.2 (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 01:29:32.78 +61:46:26.2: 12.95 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:32.78 +61:46:26.2: 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 31.4332* 01 29 32.78 +61 46 26.2 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.24,0.05,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
target 20260531.4332 10.24CV 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 31.4332 2461191.9332 10.27 01:14:45.20 +60:30:02.9
125.80055 -2.24102 galactic Cas Second-epoch detections are separated by 2.1" and 2.1 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 510401067222116992 | 01:14:43.22 +60:30:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5: 1935BSD...C01....0S BSD 8- 705 J-Ks=0.606+/-0.039 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:45.20 +60:30:02.9: 12.93 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:45.20 +60:30:02.9: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 14 45.20 +60 30 02.9 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
Gaia DR3 510401067222116992,2461191.9332,10.27,0.05,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 510401067222116992 20260531.4332 10.27CV 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 31.4332 2461191.9332 10.45 01:25:50.10 +61:06:31.1
127.07608 -1.48604 galactic Cas Second-epoch detections are separated by 0.7" and 2.5 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 510673505587551872 | 01:25:46.78 +61:06:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1960IzKry..24..160B [B60] +60 214
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:50.10 +61:06:31.1: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:50.10 +61:06:31.1: 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 31.4332* 01 25 50.10 +61 06 31.1 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510673505587551872,2461191.9332,10.45,0.05,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 510673505587551872 20260531.4332 10.45CV 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 31.4332 2461191.9332 10.36 01:03:22.59 +60:32:13.4
124.40063 -2.30064 galactic Cas Second-epoch detections are separated by 0.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426389926362885504 | 01:03:24.61 +60:32:35.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.064+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:03:22.59 +60:32:13.4: 10.95 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:22.59 +60:32:13.4: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 31.4332* 01 03 22.59 +60 32 13.4 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426389926362885504,2461191.9332,10.36,0.05,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 426389926362885504 20260531.4332 10.36CV 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 31.4332 2461191.9332 10.45 00:51:43.50 +57:16:06.5
122.97091 -5.60325 galactic Cas Second-epoch detections are separated by 0.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 424260206699039744 | 00:51:40.48 +57:16:32.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.418+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:43.50 +57:16:06.5: 11.78 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:43.50 +57:16:06.5: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 51 43.50 +57 16 06.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 424260206699039744,2461191.9332,10.45,0.05,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 424260206699039744 20260531.4332 10.45CV 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 31.4332 2461191.9332 10.45 00:35:28.33 +62:32:36.1
121.09271 -0.27136 galactic Cas Second-epoch detections are separated by 0.7" 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 | Gaia DR3 430687092681614720 | 00:35:32.40 +62:32:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956PMcCO..13a....B AG+62 66 J-Ks=0.134+/-0.038 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:35:28.33 +62:32:36.1: 12.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:35:28.33 +62:32:36.1: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 31.4332* 00 35 28.33 +62 32 36.1 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430687092681614720,2461191.9332,10.45,0.05,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 430687092681614720 20260531.4332 10.45CV 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 31.4332 2461191.9332 10.48 01:03:35.25 +60:28:07.9
124.42979 -2.36755 galactic Cas Second-epoch detections are separated by 2.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426387242001692800 | 01:03:37.95 +60:27:48.5 (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 01:03:35.25 +60:28:07.9: 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 01:03:35.25 +60:28:07.9: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 31.4332* 01 03 35.25 +60 28 07.9 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426387242001692800,2461191.9332,10.48,0.05,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 426387242001692800 20260531.4332 10.48CV 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 31.4332 2461191.9332 10.45 01:44:32.29 +58:45:34.5
129.78371 -3.40396 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 | Gaia DR3 506461620135299584 | 01:44:30.78 +58:46:10.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B8: 1955ApJS....2..123F LF 5 +58 58
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:32.29 +58:45:34.5: 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 01:44:32.29 +58:45:34.5: 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 31.4332* 01 44 32.29 +58 45 34.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506461620135299584,2461191.9332,10.45,0.05,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 506461620135299584 20260531.4332 10.45CV 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 31.4332 2461191.9332 10.46 02:06:05.99 +57:07:10.0
132.96611 -4.29060 galactic Per Second-epoch detections are separated by 1.7" 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 | Gaia DR3 505132276218615296 | 02:06:07.93 +57:06:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1932MeUpp..55....1S BD+56 423 J-Ks=0.926+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:06:05.99 +57:07:10.0: 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 02:06:05.99 +57:07:10.0: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 02 06 05.99 +57 07 10.0 10.5 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 505132276218615296,2461191.9332,10.46,0.05,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 505132276218615296 20260531.4332 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.40 02:11:23.08 +61:21:04.9
132.36366 -0.04777 galactic Cas Second-epoch detections are separated by 2.9" and 2.3 pix
The object was found in VSX20" Gaia DR3 507740455237382016
Type: ROT
# Max. Min./Amp. JD0 Period
14.500 G 14.530 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 02:11:23.08 +61:21:04.9: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:23.08 +61:21:04.9: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 02 11 23.08 +61 21 04.9 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507740455237382016,2461191.9332,10.40,0.05,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
Gaia DR3 507740455237382016 20260531.4332 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 31.4332 2461191.9332 10.54 00:52:12.53 +64:57:21.7
123.01356 2.08440 galactic Cas Second-epoch detections are separated by 1.1" and 2.4 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 524435405436784000 | 00:52:06.66 +64:57:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1966UppAn...5d...1O [O66] 9: 83 J-Ks=0.408+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:12.53 +64:57:21.7: 12.63 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:12.53 +64:57:21.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 52 12.53 +64 57 21.7 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 524435405436784000,2461191.9332,10.54,0.05,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 524435405436784000 20260531.4332 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.48 01:08:31.65 +63:35:41.9
124.83068 0.78625 galactic Cas Second-epoch detections are separated by 3.3" and 2.4 pix
The object was found in VSX 5" ASASSN-V J010832.13+633546.2
Type: SR
# Max. Min./Amp. JD0 Period
13.970 V 14.080 V 2458063.00000 185.000000000000
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 01:08:31.65 +63:35:41.9: 10.80 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:31.65 +63:35:41.9: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 31.4332* 01 08 31.65 +63 35 41.9 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J010832.13+633546.2,2461191.9332,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J010832.13+633546.2 20260531.4332 10.48CV 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 31.4332 2461191.9332 10.56 01:15:11.46 +60:07:02.8
125.88961 -2.61783 galactic Cas Second-epoch detections are separated by 1.9" and 2.6 pix
The object was found in VSX22" ZTF J011513.82+600649.3
Type: EW
# Max. Min./Amp. JD0 Period
17.560 r Y 0.505 r 2458297.93010 0.388644000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:11.46 +60:07:02.8: 12.18 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:11.46 +60:07:02.8: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 31.4332* 01 15 11.46 +60 07 02.8 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
ZTF J011513.82+600649.3,2461191.9332,10.56,0.05,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
ZTF J011513.82+600649.3 20260531.4332 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.57 00:47:11.28 +58:29:06.2
122.37493 -4.38210 galactic Cas Second-epoch detections are separated by 1.5" and 2.4 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 J011.7996+58.4919 | 00:47:11.28 +58:29:06.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5) J-Ks=0.295+/-0.043 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:47:11.28 +58:29:06.2: 11.21 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:47:11.28 +58:29:06.2: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.74 +/- 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 31.4332* 00 47 11.28 +58 29 06.2 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.7996+58.4919,2461191.9332,10.57,0.05,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 J011.7996+58.4919 20260531.4332 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.72 01:19:23.90 +58:26:39.0
126.59343 -4.22866 galactic Cas Second-epoch detections are separated by 1.6" and 2.3 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 413883771873740416 | 01:19:25.94 +58:26:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1951UppAn...2j...1B NGC 457 191 J-Ks=0.329+/-0.040 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:23.90 +58:26:39.0: 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 01:19:23.90 +58:26:39.0: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 19 23.90 +58 26 39.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413883771873740416,2461191.9332,10.72,0.05,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 413883771873740416 20260531.4332 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.71 00:48:13.83 +58:19:19.4
122.50951 -4.54706 galactic Cas Second-epoch detections are separated by 1.4" and 2.9 pix
The object was found in VSX23" Gaia DR3 425091574927093504
Type: ROT
# Max. Min./Amp. JD0 Period
17.080 G 17.160 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 00:48:13.83 +58:19:19.4: 11.40 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:48:13.83 +58:19:19.4: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 48 13.83 +58 19 19.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 425091574927093504,2461191.9332,10.71,0.05,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 425091574927093504 20260531.4332 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.59 01:18:39.81 +58:25:50.7
126.49900 -4.25231 galactic Cas Second-epoch detections are separated by 0.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:39.81 +58:25:50.7 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:39.81 +58:25:50.7: 12.20 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:39.81 +58:25:50.7: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 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 31.4332* 01 18 39.81 +58 25 50.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.59,0.05,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
target 20260531.4332 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.63 01:58:39.97 +59:15:59.2
131.43767 -2.49055 galactic Cas Second-epoch detections are separated by 3.1" and 2.7 pix
The object was found in VSX 3" Gaia DR3 507801031456497792
Type: RS
# Max. Min./Amp. JD0 Period
13.250 G 13.370 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 01:58:39.97 +59:15:59.2: 12.96 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:39.97 +59:15:59.2: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 31.4332* 01 58 39.97 +59 15 59.2 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507801031456497792,2461191.9332,10.63,0.05,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 507801031456497792 20260531.4332 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.65 01:10:31.31 +60:31:13.0
125.27957 -2.26445 galactic Cas Second-epoch detections are separated by 1.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.6444+60.5188 | 01:10:31.31 +60:31:13.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.119+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:31.31 +60:31:13.0: 11.67 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:31.31 +60:31:13.0: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 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 31.4332* 01 10 31.31 +60 31 13.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.6444+60.5188,2461191.9332,10.65,0.05,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 J017.6444+60.5188 20260531.4332 10.65CV 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 31.4332 2461191.9332 10.52 02:16:10.72 +64:52:44.6
131.77335 3.47204 galactic Cas Second-epoch detections are separated by 5.3" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:16:10.72 +64:52:44.6 (user input) | T | P | (position from user input) J-Ks=2.439+/- (Very red!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:10.72 +64:52:44.6: 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 02:16:10.72 +64:52:44.6: 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 31.4332* 02 16 10.72 +64 52 44.6 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.52,0.05,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
target 20260531.4332 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.72 00:33:46.78 +63:27:55.5
120.96120 0.66126 galactic Cas Second-epoch detections are separated by 1.7" and 2.3 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 430883355509555584 | 00:33:46.85 +63:28:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.453+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:33:46.78 +63:27:55.5: 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 00:33:46.78 +63:27:55.5: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 31.4332* 00 33 46.78 +63 27 55.5 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430883355509555584,2461191.9332,10.72,0.05,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 430883355509555584 20260531.4332 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.64 00:51:32.88 +59:59:13.7
122.94570 -2.88461 galactic Cas Second-epoch detections are separated by 3.0" and 2.3 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 426864434349441664 | 00:51:36.39 +59:59:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.041 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:32.88 +59:59:13.7: 11.08 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:32.88 +59:59:13.7: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 31.4332* 00 51 32.88 +59 59 13.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426864434349441664,2461191.9332,10.64,0.05,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 426864434349441664 20260531.4332 10.64CV 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 31.4332 2461191.9332 10.56 00:47:19.74 +56:59:25.7
122.36937 -5.87679 galactic Cas Second-epoch detections are separated by 6.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J011.8401+56.9896 | 00:47:20.73 +56:59:58.2 (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 00:47:19.74 +56:59:25.7: 11.25 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:47:19.74 +56:59:25.7: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 31.4332* 00 47 19.74 +56 59 25.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J011.8401+56.9896,2461191.9332,10.56,0.05,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
ATO J011.8401+56.9896 20260531.4332 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.62 01:50:38.77 +56:46:21.4
131.01247 -5.16735 galactic Per Second-epoch detections are separated by 1.0" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:50:38.77 +56:46:21.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:38.77 +56:46:21.4: 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 01:50:38.77 +56:46:21.4: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 50 38.77 +56 46 21.4 10.6 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,2461191.9332,10.62,0.05,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 20260531.4332 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.63 02:19:57.57 +59:32:26.1
133.94463 -1.42507 galactic Cas Second-epoch detections are separated by 2.3" and 2.2 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 J034.9820+59.5389 | 02:19:57.57 +59:32:26.1 (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 02:19:57.57 +59:32:26.1: 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 02:19:57.57 +59:32:26.1: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 02 19 57.57 +59 32 26.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.9820+59.5389,2461191.9332,10.63,0.05,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
ATO J034.9820+59.5389 20260531.4332 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.69 01:59:33.16 +60:01:44.8
131.34811 -1.72491 galactic Cas Second-epoch detections are separated by 0.9" and 2.2 pix
The object was found in VSX18" ZTF J015934.53+600159.8
Type: SR
# Max. Min./Amp. JD0 Period
15.783 r Y 0.432 r 2458492.34860 197.227334200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:33.16 +60:01:44.8: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:33.16 +60:01:44.8: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 31.4332* 01 59 33.16 +60 01 44.8 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
ZTF J015934.53+600159.8,2461191.9332,10.69,0.05,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 J015934.53+600159.8 20260531.4332 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.73 01:49:34.16 +61:03:37.2
129.90736 -1.02167 galactic Cas Second-epoch detections are separated by 1.0" and 2.1 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 | 01:49:34.16 +61:03:37.2 (user input) | T | P | (position from user input) J-Ks=1.043+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:34.16 +61:03:37.2: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:34.16 +61:03:37.2: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 49 34.16 +61 03 37.2 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.73,0.05,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
target 20260531.4332 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.72 01:44:01.00 +61:52:01.8
129.08761 -0.37456 galactic Cas Second-epoch detections are separated by 2.1" and 2.2 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 | 01:44:01.00 +61:52:01.8 (user input) | T | P | (position from user input) SpType: B2V 1999A&AS..136..313S Cl* NGC 654 Sto 97 J-Ks=0.210+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:01.00 +61:52:01.8: 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 01:44:01.00 +61:52:01.8: 13.61 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 44 01.00 +61 52 01.8 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,2461191.9332,10.72,0.05,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
target 20260531.4332 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.66 02:11:32.71 +61:10:00.8
132.43821 -0.21761 galactic Cas Second-epoch detections are separated by 5.3" and 1.7 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 507719152199688448 | 02:11:32.51 +61:09:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1970A&AS....2..201B IRAS 02078+6055
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:32.71 +61:10:00.8: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:32.71 +61:10:00.8: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 02 11 32.71 +61 10 00.8 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507719152199688448,2461191.9332,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507719152199688448 20260531.4332 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.69 01:31:08.96 +59:34:13.3
127.94793 -2.91408 galactic Cas Second-epoch detections are separated by 1.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.7886+59.5702 | 01:31:07.89 +59:33:48.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1955ApJS....2..123F LF 5 +59 28 J-Ks=0.831+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:08.96 +59:34:13.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:08.96 +59:34:13.3: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 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 31.4332* 01 31 08.96 +59 34 13.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.7886+59.5702,2461191.9332,10.69,0.05,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 J022.7886+59.5702 20260531.4332 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.65 01:29:33.02 +63:19:32.3
127.19389 0.76971 galactic Cas Second-epoch detections are separated by 5.7" and 3.2 pix
The object was found in VSX19" Gaia DR3 512422828587465216
Type: S
# Max. Min./Amp. JD0 Period
14.920 G 15.600 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:33.02 +63:19:32.3: 12.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:33.02 +63:19:32.3: 13.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 31.4332* 01 29 33.02 +63 19 32.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512422828587465216,2461191.9332,10.65,0.05,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 512422828587465216 20260531.4332 10.65CV 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 31.4332 2461191.9332 10.86 01:29:21.35 +61:44:15.4
127.40508 -0.80437 galactic Cas Second-epoch detections are separated by 2.2" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:21.35 +61:44:15.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:21.35 +61:44:15.4: 12.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:21.35 +61:44:15.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 29 21.35 +61 44 15.4 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260531.4332 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.78 01:18:36.99 +58:41:38.2
126.46501 -3.99124 galactic Cas Second-epoch detections are separated by 2.5" and 2.1 pix
The object was found in VSX23" Gaia DR3 413902596701682816
Type: ROT
# Max. Min./Amp. JD0 Period
15.180 G 15.220 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 01:18:36.99 +58:41:38.2: 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 01:18:36.99 +58:41:38.2: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 18 36.99 +58 41 38.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413902596701682816,2461191.9332,10.78,0.05,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 413902596701682816 20260531.4332 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.80 01:35:10.85 +60:45:33.1
128.25131 -1.65998 galactic Cas Second-epoch detections are separated by 2.3" and 2.7 pix
The object was found in VSX 3" Gaia DR3 509868044605284992
Type: ROT
# Max. Min./Amp. JD0 Period
13.700 G 13.730 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 01:35:10.85 +60:45:33.1: 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 01:35:10.85 +60:45:33.1: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 31.4332* 01 35 10.85 +60 45 33.1 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509868044605284992,2461191.9332,10.80,0.05,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 509868044605284992 20260531.4332 10.80CV 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 31.4332 2461191.9332 10.81 02:01:38.60 +61:45:15.1
131.13690 0.00596 galactic Cas Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:01:38.60 +61:45:15.1 (user input) | T | P | (position from user input) J-Ks=0.312+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:38.60 +61:45:15.1: 12.24 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:38.60 +61:45:15.1: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 31.4332* 02 01 38.60 +61 45 15.1 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.81,0.05,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
target 20260531.4332 10.81CV 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 31.4332 2461191.9332 10.88 01:19:41.71 +62:51:04.2
126.14893 0.15605 galactic Cas Second-epoch detections are separated by 1.2" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:41.71 +62:51:04.2 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:41.71 +62:51:04.2: 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 01:19:41.71 +62:51:04.2: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 31.4332* 01 19 41.71 +62 51 04.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.88,0.05,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
target 20260531.4332 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.74 02:10:23.89 +60:01:12.9
132.65116 -1.35307 galactic Cas Second-epoch detections are separated by 0.8" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:10:23.89 +60:01:12.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.329+/-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 02:10:23.89 +60:01:12.9: 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 02:10:23.89 +60:01:12.9: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 31.4332* 02 10 23.89 +60 01 12.9 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.74,0.05,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
target 20260531.4332 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.77 01:46:38.37 +60:07:32.0
129.75999 -2.01234 galactic Cas Second-epoch detections are separated by 1.7" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.6591+60.1406 | 01:46:39.63 +60:07:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.37 +60:07:32.0: 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 01:46:38.37 +60:07:32.0: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 31.4332* 01 46 38.37 +60 07 32.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.6591+60.1406,2461191.9332,10.77,0.05,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
ATO J026.6591+60.1406 20260531.4332 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.73 02:03:15.09 +62:12:10.7
131.19691 0.48915 galactic Cas Second-epoch detections are separated by 2.6" and 2.2 pix
The object was found in VSX 3" Gaia DR3 508770319675675392
Type: ROT
# Max. Min./Amp. JD0 Period
13.310 G 13.350 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 02:03:15.09 +62:12:10.7: 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 02:03:15.09 +62:12:10.7: 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 31.4332* 02 03 15.09 +62 12 10.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508770319675675392,2461191.9332,10.73,0.05,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 508770319675675392 20260531.4332 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.88 02:10:32.76 +59:59:55.2
132.67528 -1.36809 galactic Cas Second-epoch detections are separated by 1.2" and 2.1 pix
The object was found in VSX20" Gaia DR3 507519453397787520
Type: ROT
# Max. Min./Amp. JD0 Period
15.090 G 15.130 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 02:10:32.76 +59:59:55.2: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:32.76 +59:59:55.2: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 31.4332* 02 10 32.76 +59 59 55.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507519453397787520,2461191.9332,10.88,0.05,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 507519453397787520 20260531.4332 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.82 02:02:53.99 +60:15:40.7
131.68770 -1.38996 galactic Cas Second-epoch detections are separated by 1.3" and 2.3 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 507950977353541248 | 02:02:48.33 +60:15:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.870+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:53.99 +60:15:40.7: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:53.99 +60:15:40.7: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 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 31.4332* 02 02 53.99 +60 15 40.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507950977353541248,2461191.9332,10.82,0.05,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 507950977353541248 20260531.4332 10.82CV 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 31.4332 2461191.9332 10.95 01:52:48.49 +60:28:34.7
130.42636 -1.49937 galactic Cas Second-epoch detections are separated by 0.5" and 2.2 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 508121436018447744 | 01:52:50.90 +60:27:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1928AnHar.100...49C HD 236896 J-Ks=0.762+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:48.49 +60:28:34.7: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:48.49 +60:28:34.7: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 31.4332* 01 52 48.49 +60 28 34.7 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508121436018447744,2461191.9332,10.95,0.05,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 508121436018447744 20260531.4332 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.95 01:09:51.31 +57:04:44.9
125.44482 -5.70272 galactic Cas Second-epoch detections are separated by 3.7" and 2.1 pix
The object was found in VSX15" Gaia DR3 413511484103439360
Type: E
# Max. Min./Amp. JD0 Period
15.640 G 16.130 G 0.474573000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:51.31 +57:04:44.9: 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 01:09:51.31 +57:04:44.9: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 09 51.31 +57 04 44.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413511484103439360,2461191.9332,10.95,0.05,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 413511484103439360 20260531.4332 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.86 01:40:34.64 +60:45:54.0
128.89881 -1.53619 galactic Cas Second-epoch detections are separated by 1.6" and 2.2 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 J025.1283+60.7735 | 01:40:28.84 +60:45:47.6 (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 01:40:34.64 +60:45:54.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:34.64 +60:45:54.0: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 31.4332* 01 40 34.64 +60 45 54.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.1283+60.7735,2461191.9332,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.1283+60.7735 20260531.4332 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.06 01:36:07.33 +59:27:16.2
128.58995 -2.92548 galactic Cas Second-epoch detections are separated by 5.5" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:36:07.33 +59:27:16.2 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:07.33 +59:27:16.2: 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 01:36:07.33 +59:27:16.2: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 36 07.33 +59 27 16.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.06,0.05,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
target 20260531.4332 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.88 02:01:36.75 +59:57:22.0
131.61591 -1.72718 galactic Cas Second-epoch detections are separated by 3.5" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:01:36.75 +59:57:22.0 (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 02:01:36.75 +59:57:22.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:36.75 +59:57:22.0: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 31.4332* 02 01 36.75 +59 57 22.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.88,0.05,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
target 20260531.4332 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.98 01:07:32.39 +61:11:22.8
124.87139 -1.62143 galactic Cas Second-epoch detections are separated by 1.4" and 2.2 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 522502773234598656 | 01:07:29.57 +61:12:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1935BSD...C01....0S BSD 8-1106
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:32.39 +61:11:22.8: 12.84 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:32.39 +61:11:22.8: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 31.4332* 01 07 32.39 +61 11 22.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522502773234598656,2461191.9332,10.98,0.05,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 522502773234598656 20260531.4332 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.91 01:38:33.68 +60:47:23.0
128.65235 -1.55757 galactic Cas Second-epoch detections are separated by 0.7" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:33.68 +60:47:23.0 (user input) | T | P | (position from user input) J-Ks=0.216+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:33.68 +60:47:23.0: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:33.68 +60:47:23.0: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 38 33.68 +60 47 23.0 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,10.91,0.05,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
target 20260531.4332 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.04 01:01:58.34 +58:30:09.1
124.31148 -4.34100 galactic Cas Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:01:58.34 +58:30:09.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:58.34 +58:30:09.1: 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 01:01:58.34 +58:30:09.1: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 01 58.34 +58 30 09.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.04,0.05,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
target 20260531.4332 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.02 01:13:54.14 +58:12:33.3
125.89644 -4.53313 galactic Cas Second-epoch detections are separated by 2.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J018.4686+58.2100 | 01:13:54.14 +58:12:33.3 (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 01:13:54.14 +58:12:33.3: 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 01:13:54.14 +58:12:33.3: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 31.4332* 01 13 54.14 +58 12 33.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.4686+58.2100,2461191.9332,11.02,0.05,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
ATO J018.4686+58.2100 20260531.4332 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.91 01:54:53.18 +58:16:51.3
131.21013 -3.56738 galactic Cas Second-epoch detections are separated by 2.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J028.7238+58.2897 | 01:54:53.18 +58:16:51.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:53.18 +58:16:51.3: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:53.18 +58:16:51.3: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 54 53.18 +58 16 51.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.7238+58.2897,2461191.9332,10.91,0.05,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 J028.7238+58.2897 20260531.4332 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.01 00:56:24.23 +61:31:26.1
123.52397 -1.34212 galactic Cas Second-epoch detections are separated by 1.3" and 2.3 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 426680541024498432 | 00:56:21.45 +61:31:12.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:56:24.23 +61:31:26.1: 10.95 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:24.23 +61:31:26.1: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 00 56 24.23 +61 31 26.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426680541024498432,2461191.9332,11.01,0.05,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 426680541024498432 20260531.4332 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.98 01:11:41.10 +58:17:28.2
125.59803 -4.47573 galactic Cas Second-epoch detections are separated by 4.5" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.9458+58.3022 | 01:11:42.53 +58:18:10.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3 1928AnHar.100...49C HD 236647 J-Ks=0.537+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:41.10 +58:17:28.2: 11.32 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:41.10 +58:17:28.2: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 11 41.10 +58 17 28.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.9458+58.3022,2461191.9332,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.9458+58.3022 20260531.4332 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.06 01:22:23.35 +61:13:51.6
126.64840 -1.41721 galactic Cas Second-epoch detections are separated by 2.6" and 2.1 pix
The object was found in VSX 3" 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 01:22:23.35 +61:13:51.6: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:23.35 +61:13:51.6: 15.55 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.55 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 22 23.35 +61 13 51.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0122238+611352,2461191.9332,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0122238+611352 20260531.4332 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.08 01:35:47.16 +61:18:13.3
128.23092 -1.11095 galactic Cas Second-epoch detections are separated by 1.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:35:47.16 +61:18:13.3 (user input) | T | P | (position from user input) J-Ks=0.513+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:47.16 +61:18:13.3: 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 01:35:47.16 +61:18:13.3: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 31.4332* 01 35 47.16 +61 18 13.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.08,0.05,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
target 20260531.4332 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.01 01:38:06.41 +58:10:40.1
129.06913 -4.13675 galactic Cas Second-epoch detections are separated by 1.0" and 2.6 pix
The object was found in VSX11" Gaia DR3 508962699851411840
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
16.190 G 16.240 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:06.41 +58:10:40.1: 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 01:38:06.41 +58:10:40.1: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 31.4332* 01 38 06.41 +58 10 40.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508962699851411840,2461191.9332,11.01,0.05,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 508962699851411840 20260531.4332 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.03 01:31:48.04 +64:21:56.1
127.28130 1.83522 galactic Cas Second-epoch detections are separated by 1.3" and 2.1 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 | 01:31:48.04 +64:21:56.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.04 +64:21:56.1: 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 01:31:48.04 +64:21:56.1: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 31 48.04 +64 21 56.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.03,0.05,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 20260531.4332 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.07 01:55:52.83 +64:15:23.8
129.85981 2.25512 galactic Cas Second-epoch detections are separated by 1.1" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:55:52.83 +64:15:23.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:52.83 +64:15:23.8: 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 01:55:52.83 +64:15:23.8: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 55 52.83 +64 15 23.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461191.9332,11.07,0.05,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
target 20260531.4332 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.04 00:39:36.45 +60:06:50.0
121.45703 -2.72398 galactic Cas Second-epoch detections are separated by 0.6" and 2.7 pix
The object was found in VSX25" Gaia DR3 427068256319084672
Type: ROT
# Max. Min./Amp. JD0 Period
14.030 G 14.050 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 00:39:36.45 +60:06:50.0: 12.02 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:39:36.45 +60:06:50.0: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 31.4332* 00 39 36.45 +60 06 50.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 427068256319084672,2461191.9332,11.04,0.05,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 427068256319084672 20260531.4332 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.05 01:43:03.20 +58:57:12.7
129.55614 -3.25278 galactic Cas Second-epoch detections are separated by 2.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.7767+58.9545 | 01:43:03.20 +58:57:12.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.236+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:03.20 +58:57:12.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:03.20 +58:57:12.7: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 31.4332* 01 43 03.20 +58 57 12.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.7767+58.9545,2461191.9332,11.05,0.05,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 J025.7767+58.9545 20260531.4332 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.11 00:47:38.45 +60:34:44.6
122.46526 -2.28925 galactic Cas Second-epoch detections are separated by 1.0" 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 | Gaia DR3 426944561263800576 | 00:47:32.96 +60:34:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1966UppAn...5d...1O [O66] 9: 22
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:47:38.45 +60:34:44.6: 10.95 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:47:38.45 +60:34:44.6: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.14 +/- 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 31.4332* 00 47 38.45 +60 34 44.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426944561263800576,2461191.9332,11.11,0.05,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 426944561263800576 20260531.4332 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.16 01:22:10.81 +59:09:03.1
126.87149 -3.48553 galactic Cas Second-epoch detections are separated by 2.3" 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 413976852405588480 | 01:22:13.31 +59:08:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +58 184 J-Ks=0.462+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:10.81 +59:09:03.1: 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 01:22:10.81 +59:09:03.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 22 10.81 +59 09 03.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413976852405588480,2461191.9332,11.16,0.05,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 413976852405588480 20260531.4332 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.31 01:36:51.89 +60:55:57.8
128.42354 -1.45374 galactic Cas Second-epoch detections are separated by 1.3" and 2.1 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 509917110306382208 | 01:36:53.71 +60:55:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.245+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:51.89 +60:55:57.8: 11.92 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:51.89 +60:55:57.8: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 31.4332* 01 36 51.89 +60 55 57.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509917110306382208,2461191.9332,11.31,0.05,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 509917110306382208 20260531.4332 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.18 01:11:56.50 +58:41:04.4
125.60030 -4.08092 galactic Cas Second-epoch detections are separated by 1.9" and 2.5 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 J017.9933+58.6776 | 01:11:56.50 +58:41:04.4 (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 01:11:56.50 +58:41:04.4: 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 01:11:56.50 +58:41:04.4: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 11 56.50 +58 41 04.4 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.9933+58.6776,2461191.9332,11.18,0.05,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 J017.9933+58.6776 20260531.4332 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.38 02:05:23.00 +59:19:30.2
132.24811 -2.20259 galactic Cas Second-epoch detections are separated by 0.3" and 2.3 pix
The object was found in VSX17" Gaia DR3 507054012083283584
Type: ROT
# Max. Min./Amp. JD0 Period
18.020 G 18.120 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 02:05:23.00 +59:19:30.2: 12.07 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:23.00 +59:19:30.2: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 31.4332* 02 05 23.00 +59 19 30.2 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507054012083283584,2461191.9332,11.38,0.05,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 507054012083283584 20260531.4332 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.48 01:18:57.79 +59:46:45.7
126.39373 -2.90725 galactic Cas Second-epoch detections are separated by 0.5" and 2.4 pix
The object was found in VSX21" Gaia DR3 510314893000038144
Type: VAR
# Max. Min./Amp. JD0 Period
17.040 G 17.070 G 0.025319800000 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 01:18:57.79 +59:46:45.7: 13.02 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:57.79 +59:46:45.7: 14.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 18 57.79 +59 46 45.7 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510314893000038144,2461191.9332,11.48,0.05,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 510314893000038144 20260531.4332 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.56 01:21:12.70 +59:45:44.2
126.67725 -2.89278 galactic Cas Second-epoch detections are separated by 1.1" and 2.5 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 510130003239608832 | 01:21:17.18 +59:45:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1960IzKry..24..160B [B60] +59 134 J-Ks=1.017+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:12.70 +59:45:44.2: 12.70 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:12.70 +59:45:44.2: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 21 12.70 +59 45 44.2 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510130003239608832,2461191.9332,11.56,0.05,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 510130003239608832 20260531.4332 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 11.46 01:27:31.61 +59:41:05.3
127.47760 -2.86805 galactic Cas Second-epoch detections are separated by 2.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510079700591073920 | 01:27:25.91 +59:41:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1960IzKry..24..160B [B60] +59 191 J-Ks=0.213+/- (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:31.61 +59:41:05.3: 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 01:27:31.61 +59:41:05.3: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 27 31.61 +59 41 05.3 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510079700591073920,2461191.9332,11.46,0.05,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 510079700591073920 20260531.4332 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.04 01:21:54.46 +61:20:57.4
126.57690 -1.30665 galactic Cas Second-epoch detections are separated by 2.0" and 2.1 pix
The object was found in ASASSN-V 3" 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 01:21:54.46 +61:20:57.4: 13.14 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:54.46 +61:20:57.4: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 01 21 54.46 +61 20 57.4 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
VARIABLE_NAME,2461191.9332,10.04,0.05,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
VARIABLE_NAME 20260531.4332 10.04CV 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 31.4332 2461191.9332 10.37 01:02:56.70 +59:37:23.2
124.38850 -3.21609 galactic Cas Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:02:56.70 +59:37:23.2 (user input) | T | P | (position from user input) J-Ks=0.210+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:56.70 +59:37:23.2: 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 01:02:56.70 +59:37:23.2: 12.91 +/- 0.02 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 31.4332* 01 02 56.70 +59 37 23.2 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
target,2461191.9332,10.37,0.05,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
target 20260531.4332 10.37CV 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 31.4332 2461191.9332 10.71 02:39:28.93 +63:32:02.4
134.62739 3.14276 galactic Cas Second-epoch detections are separated by 2.2" and 2.2 pix
The object was found in VSX24" ZTF J023932.46+633157.8
Type: EW
# Max. Min./Amp. JD0 Period
19.964 r Y 0.738 r 2458310.94650 0.306171600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:39:28.93 +63:32:02.4: 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 02:39:28.93 +63:32:02.4: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 02 39 28.93 +63 32 02.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J023932.46+633157.8,2461191.9332,10.71,0.05,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
ZTF J023932.46+633157.8 20260531.4332 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 31.4332 2461191.9332 10.04 02:49:56.80 +63:51:39.7
135.54118 3.92934 galactic Cas Second-epoch detections are separated by 0.7" and 2.0 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 467697169465689088 | 02:49:53.99 +63:51:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.456+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:49:56.80 +63:51:39.7: 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 02:49:56.80 +63:51:39.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 31.4332* 02 49 56.80 +63 51 39.7 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 467697169465689088,2461191.9332,10.04,0.05,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 467697169465689088 20260531.4332 10.04CV 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
## 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: 2461191.93346046 31.05.2026 10:24:00.984 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 18
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): 29588
Objects passed selection criteria: 29451
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 21972.8
Average stars matched: 21357.8 (97.2011 %)
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 05:37:46 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: 2461191.93346046 31.05.2026 10:24:00.984 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 404
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 86 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): 202540
Objects passed selection criteria: 202079
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 160155
Average stars matched: 154823 (96.6707 %)
Memory usage VmPeak: 2153924 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 05:45:08 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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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: 2461191.93302642
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits'
wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
Image size: 941.7'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:28.898 +61:58:18.40 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 01:42:28.898 +61:58:18.40
Angular distance between the image centers 0.0134 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_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
Image size: 941.7'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:27.391 +61:58:26.57 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 01:42:27.391 +61:58:26.57
Angular distance between the image centers 0.0114 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 01:42:28.898 +61:58:18.40
Second-epoch second image center 01:42:27.391 +61:58:26.57
Angular distance between the image centers 0.00372 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.3BigGTF2cj
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.5t4mi6d4EU
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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits &> /tmp/tmp.xTDATu0ujw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits &> /tmp/tmp.AbQEnawEkV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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 17 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
2.3 pix fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
2.3 pix fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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
14.2 mag. fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
14.2 mag. fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.3 (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.3BigGTF2cj (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_052435_TTUQ1b1x1_1136561_iesUTh2n/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.5t4mi6d4EU (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_052435_TTUQ1b1x1_1136561_iesUTh2n/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.xTDATu0ujw (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_052435_TTUQ1b1x1_1136561_iesUTh2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.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_05-23-23_20.00sec_-0.00C_LIGHTs_0414.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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1181, passed=12590
Got 12590 stars (including 11401 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits.cat
util/solve_plate_with_UCAC5 got 12590 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 11921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 11923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 11923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits N_match=968 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.394 sigma_q4_arcsec=0.361 n_q1=239 n_q2=360 n_q3=213 n_q4=156 worst_quadrant_to_overall_ratio=1.081
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits -region wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.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.AbQEnawEkV (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_052435_TTUQ1b1x1_1136561_iesUTh2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1183, passed=12577
Got 12577 stars (including 11377 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits.cat
util/solve_plate_with_UCAC5 got 12577 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 12027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 12027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 12027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits N_match=968 sigma_overall_arcsec=0.399 sigma_q1_arcsec=0.438 sigma_q2_arcsec=0.383 sigma_q3_arcsec=0.422 sigma_q4_arcsec=0.326 n_q1=238 n_q2=354 n_q3=214 n_q4=162 worst_quadrant_to_overall_ratio=1.097
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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_052435_TTUQ1b1x1_1136561_iesUTh2n/fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits -region wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits sigma_overall=0.379 worst_q_ratio=1.081
new2=fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits sigma_overall=0.399 worst_q_ratio=1.097
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_05-23-23_20.00sec_-0.00C_LIGHTs_0414_astrometric_residuals.png (968 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415_astrometric_residuals.png (968 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-23-23_20.00sec_-0.00C_LIGHTs_0414.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Cas-03-Q1b1x1_052435_TTUQ1b1x1_1136561_iesUTh2n/wcs_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415.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 01:02:34.00 +59:16:48.7: 10.05 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:11.30 +58:01:02.3: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:16.18 +59:42:57.8: 11.00 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:30.17 +60:39:17.5: 15.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:19.52 +61:15:48.4: 15.42 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:40.73 +60:54:42.6: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:11.30 +58:01:02.3: 10.54 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:30.17 +60:39:17.5: 10.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.54 +/- 0.00
Forced photometry reference-image weighted average: 10.13 +/- 0.01
Forced photometry filter REJECTED candidate at 02:09:11.30 +58:01:02.3: ref_mag=10.54 +/- 0.00 new_mean_mag=10.8608 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:33:30.17 +60:39:17.5: ref_mag=10.13 +/- 0.01 new_mean_mag=10.4707 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:16.18 +59:42:57.8: 10.68 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:34.00 +59:16:48.7: 10.41 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.80 +/- 0.00
Forced photometry filter REJECTED candidate at 00:52:16.18 +59:42:57.8: ref_mag=10.80 +/- 0.00 new_mean_mag=10.8468 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 10.19 +/- 0.00
Forced photometry filter REJECTED candidate at 01:02:34.00 +59:16:48.7: ref_mag=10.19 +/- 0.00 new_mean_mag=10.6702 delta=-0.48 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:19.52 +61:15:48.4: 11.16 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.73 +60:54:42.6: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.01
Forced photometry filter REJECTED candidate at 01:46:19.52 +61:15:48.4: ref_mag=11.17 +/- 0.01 new_mean_mag=11.4048 delta=-0.23 (need > 0.90)
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter KEPT candidate at 02:21:40.73 +60:54:42.6: ref_mag=11.02 +/- 0.00 new_mean_mag=9.8537 delta=1.17 (need > 0.90)
Adding exclusion_list_local.txt__out12304.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52170_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52170_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 52212_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52212_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:36:59.79 +63:08:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52234_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52234_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:19:06.74 +57:08:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52262_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52262_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:19:46.41 +58:12:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52264_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52264_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 52281_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52281_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 52290_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52290_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:02:37.92 +59:16:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52297_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52297_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:19:16.34 +57:10:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52305_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52305_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 52325_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52325_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:33:24.25 +60:39:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52375_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52375_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:18:52.54 +57:06:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52400_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 52400_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 51449_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 51449_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:30:27.35 +62:31:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26424_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 26424_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:51:52.99 +57:12:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23703_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 23703_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:54:53.95 +58:33:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12304_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 12304_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 08339_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 08339_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:04:34.54 +61:06:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250693_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250693_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250694_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250694_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 250697_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250697_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250698_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250698_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250699_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250699_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:55:02.37 +58:24:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250700_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250700_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250703_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250703_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250707_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250707_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:49:01.99 +63:36:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250711_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250711_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250712_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250712_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:29:22.23 +63:18:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250714_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250714_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:57:27.41 +62:06:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250728_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250728_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250730_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250730_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:17:14.86 +58:35:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250737_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250737_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250738_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250738_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250739_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250739_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250742_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250742_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250749_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250749_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250750_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250750_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250751_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250751_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:04:18.92 +59:00:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250754_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250754_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:59:03.87 +63:01:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250756_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250756_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250757_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250757_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250759_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250759_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250760_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250760_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250765_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250765_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250766_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250766_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250767_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250767_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250768_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250768_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250769_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250769_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:56:44.50 +59:40:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250771_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250771_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250772_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250772_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250773_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250773_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:44:49.39 +61:12:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250775_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250775_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:13:52.48 +58:12:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250776_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250776_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250783_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250783_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250785_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250785_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 250787_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250787_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250788_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250788_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250789_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250789_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250790_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250790_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:57:03.83 +59:44:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250791_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250791_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:49:07.06 +61:06:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250793_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250793_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:52:17.01 +58:00:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250797_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250797_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:00:12.13 +57:31:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250798_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250798_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 250799_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250799_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:02:17.76 +58:15:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250800_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250800_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250801_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250801_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250802_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250802_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:20:40.29 +56:58:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250804_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250804_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250805_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250805_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250806_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250806_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250808_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250808_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250809_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250809_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:39:19.35 +64:29:12.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250811_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250811_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250814_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250814_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:08:27.78 +57:06:48.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250815_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250815_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:03:21.44 +57:48:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250816_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250816_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:09:39.89 +61:05:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250818_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250818_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250819_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250819_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:49:08.63 +60:10:27.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250820_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250820_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250821_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250821_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250822_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250822_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:50:06.78 +58:35:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250823_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250823_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:45:38.76 +59:44:19.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250824_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250824_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:21:51.00 +59:55:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250826_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250826_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250827_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250827_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250828_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250828_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250830_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250830_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:44:54.03 +58:19:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250831_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250831_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250832_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250832_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250835_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250835_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250837_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250837_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:01:38.23 +58:50:08.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250838_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250838_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:07:07.82 +57:44:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250839_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250839_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:33:20.16 +61:32:21.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250840_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250840_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:31:14.21 +65:24:57.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250844_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250844_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250845_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250845_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250846_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250846_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:43:59.14 +61:55:17.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250847_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250847_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:53:35.04 +56:58:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250851_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250851_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250852_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250852_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:55:14.53 +59:32:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250853_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250853_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:16:20.65 +62:42:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250854_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250854_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:45:00.91 +60:52:14.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250855_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250855_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:34:26.69 +60:30:31.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250856_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250856_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250858_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250858_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250860_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250860_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:53:28.91 +57:10:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250861_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250861_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:56:58.77 +60:15:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250862_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250862_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:49:13.11 +64:11:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250866_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250866_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250867_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250867_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250868_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250868_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:58:40.42 +58:55:21.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250869_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250869_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:22:08.21 +60:22:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250871_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250871_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:16:00.99 +62:41:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250872_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250872_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:02:14.44 +61:54:04.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250873_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250873_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250915_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250915_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:48:46.95 +56:41:43.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250949_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250949_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:19:06.78 +57:09:00.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250966_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250966_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250979_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 250979_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250983_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 250983_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 251011_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251011_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251014_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251014_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 251018_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251018_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251019_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251019_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:19:16.41 +57:10:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251035_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251035_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 251166_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251166_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251174_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251174_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:26:40.83 +60:46:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251189_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251189_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251203_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251203_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:19:10.90 +58:20:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251209_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251209_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 251226_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251226_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:56:38.32 +59:13:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251238_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251238_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:44:02.16 +61:53:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251253_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251253_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:48:23.25 +60:58:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251286_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251286_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:16:47.26 +57:00:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251293_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251293_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251295_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251295_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:38:00.37 +57:56:45.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251306_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251306_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:37:17.14 +62:49:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251321_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251321_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251333_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251333_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:49:48.07 +65:05:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251334_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251334_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:46:06.00 +58:14:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251335_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251335_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251337_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251337_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:03:46.79 +61:03:18.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251338_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251338_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:13:48.17 +59:03:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251372_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251372_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:45:52.25 +64:24:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251393_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251393_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251397_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251397_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251400_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251400_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:53:16.12 +61:08:53.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251422_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251422_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:09:28.65 +59:41:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251425_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251425_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:21:50.63 +57:15:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251438_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251438_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:24:15.73 +63:03:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251459_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251459_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 251472_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251472_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:26:46.63 +57:46:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251493_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251493_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:46:47.94 +59:52:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251497_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251497_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:03:36.60 +61:02:59.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251498_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251498_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:28:15.33 +58:44:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251501_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251501_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:31:15.13 +58:01:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251514_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251514_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251521_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251521_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251548_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251548_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251559_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251559_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:04:32.42 +57:59:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251560_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251560_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 251576_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251576_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:56:22.89 +59:10:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251584_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251584_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251596_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251596_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:51:37.45 +62:56:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251622_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251622_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:45:43.22 +56:47:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251627_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251627_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:51:46.51 +57:14:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251650_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251650_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:46:34.09 +63:01:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251666_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251666_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:49:03.86 +57:59:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251673_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251673_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:35:14.73 +63:00:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251675_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251675_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:20:10.96 +58:12:08.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251686_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251686_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:56:15.03 +64:18:42.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251695_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251695_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251701_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251701_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:04:31.74 +58:01:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251706_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251706_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251712_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251712_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 251713_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251713_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:19:12.06 +65:35:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251717_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251717_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:18:19.04 +57:42:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251719_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251719_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251727_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251727_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:05:03.51 +64:21:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251735_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251735_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:54:00.37 +60:01:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251739_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251739_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:31:03.97 +66:05:02.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251744_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251744_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251748_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251748_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:46:34.85 +59:33:37.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251761_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251761_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251768_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251768_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:43:53.06 +61:53:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251778_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251778_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 251783_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251783_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:44:17.57 +61:53:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251786_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251786_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:46:33.56 +61:16:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251804_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251804_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:21:27.83 +57:48:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251813_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251813_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:00:41.06 +60:35:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251820_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251820_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:16:08.55 +58:49:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251822_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251822_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:38:33.02 +60:48:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251823_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251823_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 251829_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251829_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:23:23.51 +63:36:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251832_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251832_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251837_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251837_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:20:18.17 +58:13:41.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251868_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251868_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:57:33.29 +57:46:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251870_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251870_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:00:51.76 +58:31:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251896_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251896_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251901_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251901_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:16:59.85 +57:02:24.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251905_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251905_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251919_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251919_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:50:48.18 +64:16:19.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251940_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251940_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251944_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251944_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:57:15.08 +58:47:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251949_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251949_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:39:31.44 +60:01:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251952_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251952_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:47:06.00 +63:48:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251956_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251956_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:51:02.17 +64:49:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251961_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251961_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 251968_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251968_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251971_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251971_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 251973_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 251973_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:43:03.28 +58:08:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251991_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 251991_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252022_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252022_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252027_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252027_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:02:54.72 +64:24:57.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252035_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252035_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:04:17.12 +57:09:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252042_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252042_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252043_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252043_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:17:08.19 +56:45:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252065_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252065_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252068_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252068_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252070_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252070_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:00:36.65 +58:30:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252071_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252071_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:16:38.54 +57:02:20.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252073_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252073_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:19:22.19 +58:19:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252077_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252077_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:13:35.90 +57:52:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252083_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252083_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252094_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252094_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252104_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252104_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:37:21.38 +64:05:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252108_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252108_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:17:00.61 +61:40:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252110_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252110_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:39:35.23 +57:10:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252112_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252112_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252115_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252115_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:36:28.66 +62:40:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252124_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252124_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:07:40.69 +63:30:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252129_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252129_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252131_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252131_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:27:49.77 +62:54:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252132_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252132_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252137_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252137_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:45:07.98 +56:50:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252138_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252138_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:15:09.55 +60:09:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252139_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252139_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:54:50.62 +62:25:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252142_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252142_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 252144_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252144_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:52:33.16 +60:18:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252147_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252147_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:16:36.19 +64:57:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252157_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252157_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:50:11.39 +62:29:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252159_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252159_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:38:59.95 +61:11:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252163_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252163_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:33:22.98 +57:44:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252179_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252179_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:06:45.07 +59:50:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252185_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252185_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:19:58.78 +59:04:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252187_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252187_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252190_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252190_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252196_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252196_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252198_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252198_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252202_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252202_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:16:05.20 +58:49:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252210_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252210_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:39:56.65 +60:52:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252212_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252212_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:06:23.47 +62:44:01.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252225_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252225_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:37:44.51 +64:45:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252226_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252226_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:45:59.93 +60:27:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252228_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252228_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252229_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252229_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:13:33.80 +57:53:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252234_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252234_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:24:45.14 +63:08:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252241_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252241_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252244_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252244_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:07:47.83 +57:02:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252247_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252247_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:23:00.97 +57:15:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252249_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252249_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:13:29.82 +58:34:24.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252259_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252259_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:35:50.47 +61:27:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252261_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252261_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252269_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252269_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252272_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252272_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:07:34.77 +57:33:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252276_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252276_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:47:18.96 +63:38:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252277_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252277_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252280_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252280_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:07:59.12 +57:06:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252284_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252284_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:15:34.12 +59:17:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252285_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252285_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:58:36.36 +63:43:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252288_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252288_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:56:59.39 +64:33:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252296_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252296_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252298_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252298_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252304_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252304_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 252309_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252309_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:56:05.13 +57:09:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252310_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252310_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252316_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252316_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:03:58.11 +58:23:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252317_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252317_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 252329_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252329_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:35:54.09 +60:13:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252344_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252344_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:27:52.44 +62:46:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252345_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252345_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:16:12.59 +62:42:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252348_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252348_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:19:03.63 +63:57:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252350_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252350_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252356_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252356_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:21:01.39 +57:11:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252368_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252368_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:42:33.02 +63:52:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252370_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252370_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:58:04.11 +57:58:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252372_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252372_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252373_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252373_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:59:38.50 +63:14:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252382_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252382_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:54:51.12 +60:05:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252394_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252394_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:33:32.43 +60:40:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252404_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252404_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:33:47.51 +62:08:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252407_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252407_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:30:08.81 +57:48:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252409_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252409_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:49:18.53 +64:11:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252416_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252416_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252419_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252419_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:04:26.56 +65:05:54.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252422_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252422_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 252442_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252442_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252445_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252445_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:11:50.52 +59:02:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252446_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252446_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:38:11.95 +61:01:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252447_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252447_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:16:02.28 +58:49:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252453_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252453_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:48:23.94 +65:06:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252454_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252454_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:48:38.09 +61:49:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252457_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252457_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:34:10.26 +62:09:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252458_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252458_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252460_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252460_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:24:58.24 +59:22:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252469_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252469_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:41:47.72 +59:55:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252473_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252473_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:46:55.39 +59:35:27.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252483_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252483_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252486_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252486_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252498_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252498_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252521_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252521_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:53:29.79 +60:20:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252525_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252525_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:14:00.54 +59:02:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252528_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252528_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252532_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252532_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:08:33.09 +63:34:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252545_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252545_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:41:50.75 +61:02:07.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252546_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252546_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252547_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252547_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252552_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252552_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:07:55.75 +62:45:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252568_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252568_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252576_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252576_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:38:08.30 +61:03:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252582_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252582_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252590_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252590_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 252597_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252597_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:23:02.65 +57:15:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252602_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252602_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252605_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252605_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252614_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252614_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252618_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252618_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252623_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252623_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:58:13.38 +60:44:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252624_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252624_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 252625_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252625_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:36:16.49 +60:12:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252626_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252626_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252631_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252631_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:01:15.14 +59:23:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252634_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252634_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:41:55.74 +63:42:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252645_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252645_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:35:21.41 +61:07:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252650_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252650_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:54:47.12 +56:58:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252654_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252654_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:37:41.35 +58:37:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252659_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252659_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252666_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252666_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:44:56.61 +59:46:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252673_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252673_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252684_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252684_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 252685_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252685_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 252687_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252687_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:24:44.29 +60:58:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252692_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252692_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252694_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252694_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252699_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252699_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252719_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252719_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:27:56.47 +62:46:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252724_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252724_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:07:04.07 +59:51:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252732_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252732_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:46:21.85 +64:39:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252772_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252772_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 252773_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252773_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:48:39.87 +59:09:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252779_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252779_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:01:29.59 +62:28:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252797_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252797_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252801_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252801_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252804_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252804_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:07:03.78 +59:18:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252807_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252807_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:20:40.30 +60:23:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252830_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252830_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
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Considering the candidate 252841_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252841_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:23:07.41 +61:11:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252857_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252857_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252866_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252866_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:46:50.46 +60:39:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252872_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252872_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252874_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252874_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252880_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252880_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:58:56.47 +58:04:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252900_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252900_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252925_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252925_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:31:32.26 +61:02:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252928_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252928_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252937_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252937_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:43:12.82 +64:00:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252945_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252945_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:56:16.06 +60:00:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252947_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 252947_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
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Considering the candidate 252970_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 252970_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253024_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 253024_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253051_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 253051_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253080_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 253080_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253087_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 253087_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:26:05.38 +59:01:14.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253099_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 253099_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253114_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 253114_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253123_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 253123_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253124_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 253124_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253130_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 253130_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253135_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 253135_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176011_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 176011_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:32:45.89 +56:29:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34359_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 34359_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:34:27.07 +64:32:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104399_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 104399_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:21:40.72 +60:54:42.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 112593_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211999_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 211999_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:51:53.01 +57:12:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46105_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 46105_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:38:01.00 +63:01:45.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67097_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 67097_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:36:59.80 +63:08:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 72532_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:45:35.58 +63:07:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152801_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 152801_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153855_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 153855_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 76113_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:02:02.00 +62:41:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 70271_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:20:32.67 +62:32:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235808_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 235808_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:53:02.61 +60:35:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55535_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 55535_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 39378_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 01:47:55.67 +64:32:56.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 210668_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 210668_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:43:57.08 +57:03:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193780_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 193780_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 00:54:53.94 +58:33:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34163_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 34163_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63215_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
The candidate 63215_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415 did not pass the final checks
**** FOUND 02:30:27.34 +62:31:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21028_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
Preparing report for the candidate 21028_fd_Cas-03-Q1b1x1_2026-05-31_05-24-00_20.00sec_-0.00C_LIGHTs_0415
make_report_in_HTML.sh Phase 2 (HTML assembly): 11s
make_report_in_HTML.sh TOTAL: 301s
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 ####
02:21:40.73 +60:54:42.6
01:21:54.46 +61:20:57.4
01:02:56.70 +59:37:23.2
02:49:56.80 +63:51:39.7
01:30:59.69 +63:14:35.6
01:33:01.77 +59:16:33.3
01:10:07.77 +57:43:55.5
00:44:53.02 +61:53:14.0
01:00:39.98 +59:11:28.2
01:35:49.43 +58:50:38.6
01:06:12.88 +59:33:45.3
01:08:25.50 +59:48:04.1
01:16:59.09 +59:52:02.2
01:26:38.88 +59:41:40.0
02:47:16.64 +64:40:11.5
00:52:38.59 +58:02:49.0
00:44:13.32 +56:48:04.1
01:15:17.38 +57:44:02.4
00:44:18.27 +64:55:14.6
01:05:37.92 +58:00:04.3
00:56:49.03 +57:22:46.2
01:02:12.07 +57:26:33.3
02:10:56.02 +62:17:07.8
00:57:40.76 +56:52:14.1
01:25:19.92 +59:52:22.3
01:20:45.89 +57:55:24.6
01:01:47.58 +57:23:13.9
01:11:44.61 +61:13:56.2
00:36:45.76 +61:48:23.5
00:56:04.04 +60:39:34.5
01:22:28.16 +61:07:36.1
01:32:21.98 +60:27:29.4
00:54:30.96 +59:23:59.6
01:46:42.34 +61:09:51.6
00:56:47.36 +60:38:48.1
01:02:45.62 +58:39:34.2
01:15:00.94 +57:58:06.1
01:30:10.08 +59:36:18.7
00:54:20.36 +57:41:46.4
00:51:09.78 +60:42:30.8
01:26:05.85 +57:30:37.8
01:17:48.19 +57:17:33.7
01:27:51.63 +56:56:50.7
01:01:25.35 +57:50:14.0
00:56:45.50 +58:52:46.3
00:52:52.78 +58:28:52.0
01:25:15.32 +64:40:32.7
00:40:25.91 +61:07:15.7
00:40:43.95 +61:40:52.1
01:25:38.45 +59:16:00.4
01:12:40.83 +61:20:37.3
00:58:00.23 +57:24:06.3
00:51:25.51 +62:25:15.0
01:08:09.36 +60:42:14.9
00:52:22.50 +58:23:34.3
00:36:43.38 +64:22:47.7
01:25:56.68 +59:35:12.0
01:32:39.95 +63:11:27.6
01:35:37.54 +61:16:49.5
01:02:34.05 +59:16:48.9
00:52:16.20 +59:42:57.8
01:47:13.04 +57:44:19.0
00:41:14.65 +61:35:30.9
01:44:52.13 +57:41:42.0
01:46:30.07 +61:12:58.8
01:12:05.87 +59:41:19.7
02:19:17.63 +57:07:29.7
01:40:01.44 +60:52:32.0
01:08:15.62 +63:34:13.6
01:24:27.18 +58:44:16.9
00:58:55.96 +58:04:04.8
01:58:16.32 +59:38:59.0
01:18:14.06 +61:44:36.2
00:52:31.34 +58:35:21.3
01:07:57.13 +63:37:29.6
01:29:32.78 +61:46:26.2
01:14:45.20 +60:30:02.9
01:25:50.10 +61:06:31.1
01:03:22.59 +60:32:13.4
00:51:43.50 +57:16:06.5
00:35:28.33 +62:32:36.1
01:03:35.25 +60:28:07.9
01:44:32.29 +58:45:34.5
02:06:05.99 +57:07:10.0
02:11:23.08 +61:21:04.9
00:52:12.53 +64:57:21.7
01:08:31.65 +63:35:41.9
01:15:11.46 +60:07:02.8
00:47:11.28 +58:29:06.2
01:19:23.90 +58:26:39.0
00:48:13.83 +58:19:19.4
01:18:39.81 +58:25:50.7
01:58:39.97 +59:15:59.2
01:10:31.31 +60:31:13.0
02:16:10.72 +64:52:44.6
00:33:46.78 +63:27:55.5
00:51:32.88 +59:59:13.7
00:47:19.74 +56:59:25.7
01:50:38.77 +56:46:21.4
02:19:57.57 +59:32:26.1
01:59:33.16 +60:01:44.8
01:49:34.16 +61:03:37.2
01:44:01.00 +61:52:01.8
02:11:32.71 +61:10:00.8
01:31:08.96 +59:34:13.3
01:29:33.02 +63:19:32.3
01:29:21.35 +61:44:15.4
01:18:36.99 +58:41:38.2
01:35:10.85 +60:45:33.1
02:01:38.60 +61:45:15.1
01:19:41.71 +62:51:04.2
02:10:23.89 +60:01:12.9
01:46:38.37 +60:07:32.0
02:03:15.09 +62:12:10.7
02:10:32.76 +59:59:55.2
02:02:53.99 +60:15:40.7
01:52:48.49 +60:28:34.7
01:09:51.31 +57:04:44.9
01:40:34.64 +60:45:54.0
01:36:07.33 +59:27:16.2
02:01:36.75 +59:57:22.0
01:07:32.39 +61:11:22.8
01:38:33.68 +60:47:23.0
01:01:58.34 +58:30:09.1
01:13:54.14 +58:12:33.3
01:54:53.18 +58:16:51.3
00:56:24.23 +61:31:26.1
01:11:41.10 +58:17:28.2
01:22:23.35 +61:13:51.6
01:35:47.16 +61:18:13.3
01:38:06.41 +58:10:40.1
01:31:48.04 +64:21:56.1
01:55:52.83 +64:15:23.8
00:39:36.45 +60:06:50.0
01:43:03.20 +58:57:12.7
00:47:38.45 +60:34:44.6
01:22:10.81 +59:09:03.1
01:36:51.89 +60:55:57.8
01:11:56.50 +58:41:04.4
02:05:23.00 +59:19:30.2
01:18:57.79 +59:46:45.7
01:21:12.70 +59:45:44.2
01:27:31.61 +59:41:05.3
02:39:28.93 +63:32:02.4
########### Completed Cas-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
02:21:40.73 +60:54:42.6
01:30:59.69 +63:14:35.6
01:33:01.77 +59:16:33.3
01:10:07.77 +57:43:55.5
00:44:53.02 +61:53:14.0
01:00:39.98 +59:11:28.2
01:35:49.43 +58:50:38.6
01:06:12.88 +59:33:45.3
01:08:25.50 +59:48:04.1
01:16:59.09 +59:52:02.2
01:26:38.88 +59:41:40.0
02:47:16.64 +64:40:11.5
00:52:38.59 +58:02:49.0
00:44:13.32 +56:48:04.1
01:15:17.38 +57:44:02.4
00:44:18.27 +64:55:14.6
01:05:37.92 +58:00:04.3
00:56:49.03 +57:22:46.2
01:02:12.07 +57:26:33.3
02:10:56.02 +62:17:07.8
00:57:40.76 +56:52:14.1
01:25:19.92 +59:52:22.3
01:20:45.89 +57:55:24.6
01:01:47.58 +57:23:13.9
01:11:44.61 +61:13:56.2
00:36:45.76 +61:48:23.5
00:56:04.04 +60:39:34.5
01:22:28.16 +61:07:36.1
01:32:21.98 +60:27:29.4
00:54:30.96 +59:23:59.6
01:46:42.34 +61:09:51.6
00:56:47.36 +60:38:48.1
01:02:45.62 +58:39:34.2
01:15:00.94 +57:58:06.1
01:30:10.08 +59:36:18.7
00:54:20.36 +57:41:46.4
00:51:09.78 +60:42:30.8
01:26:05.85 +57:30:37.8
01:17:48.19 +57:17:33.7
01:27:51.63 +56:56:50.7
01:01:25.35 +57:50:14.0
00:56:45.50 +58:52:46.3
00:52:52.78 +58:28:52.0
01:25:15.32 +64:40:32.7
00:40:25.91 +61:07:15.7
00:40:43.95 +61:40:52.1
01:25:38.45 +59:16:00.4
01:12:40.83 +61:20:37.3
00:58:00.23 +57:24:06.3
00:51:25.51 +62:25:15.0
01:08:09.36 +60:42:14.9
00:52:22.50 +58:23:34.3
00:36:43.38 +64:22:47.7
01:25:56.68 +59:35:12.0
01:32:39.95 +63:11:27.6
01:35:37.54 +61:16:49.5
01:02:34.05 +59:16:48.9
00:52:16.20 +59:42:57.8
01:47:13.04 +57:44:19.0
00:41:14.65 +61:35:30.9
01:44:52.13 +57:41:42.0
01:46:30.07 +61:12:58.8
01:12:05.87 +59:41:19.7
02:19:17.63 +57:07:29.7
01:40:01.44 +60:52:32.0
01:08:15.62 +63:34:13.6
01:24:27.18 +58:44:16.9
00:58:55.96 +58:04:04.8
01:58:16.32 +59:38:59.0
01:18:14.06 +61:44:36.2
00:52:31.34 +58:35:21.3
01:07:57.13 +63:37:29.6
01:29:32.78 +61:46:26.2
01:14:45.20 +60:30:02.9
01:25:50.10 +61:06:31.1
01:03:22.59 +60:32:13.4
00:51:43.50 +57:16:06.5
00:35:28.33 +62:32:36.1
01:03:35.25 +60:28:07.9
01:44:32.29 +58:45:34.5
02:06:05.99 +57:07:10.0
02:11:23.08 +61:21:04.9
00:52:12.53 +64:57:21.7
01:08:31.65 +63:35:41.9
01:15:11.46 +60:07:02.8
00:47:11.28 +58:29:06.2
01:19:23.90 +58:26:39.0
00:48:13.83 +58:19:19.4
01:18:39.81 +58:25:50.7
01:58:39.97 +59:15:59.2
01:10:31.31 +60:31:13.0
02:16:10.72 +64:52:44.6
00:33:46.78 +63:27:55.5
00:51:32.88 +59:59:13.7
00:47:19.74 +56:59:25.7
01:50:38.77 +56:46:21.4
02:19:57.57 +59:32:26.1
01:59:33.16 +60:01:44.8
01:49:34.16 +61:03:37.2
01:44:01.00 +61:52:01.8
02:11:32.71 +61:10:00.8
01:31:08.96 +59:34:13.3
01:29:33.02 +63:19:32.3
01:29:21.35 +61:44:15.4
01:18:36.99 +58:41:38.2
01:35:10.85 +60:45:33.1
02:01:38.60 +61:45:15.1
01:19:41.71 +62:51:04.2
02:10:23.89 +60:01:12.9
01:46:38.37 +60:07:32.0
02:03:15.09 +62:12:10.7
02:10:32.76 +59:59:55.2
02:02:53.99 +60:15:40.7
01:52:48.49 +60:28:34.7
01:09:51.31 +57:04:44.9
01:40:34.64 +60:45:54.0
01:36:07.33 +59:27:16.2
02:01:36.75 +59:57:22.0
01:07:32.39 +61:11:22.8
01:38:33.68 +60:47:23.0
01:01:58.34 +58:30:09.1
01:13:54.14 +58:12:33.3
01:54:53.18 +58:16:51.3
00:56:24.23 +61:31:26.1
01:11:41.10 +58:17:28.2
01:22:23.35 +61:13:51.6
01:35:47.16 +61:18:13.3
01:38:06.41 +58:10:40.1
01:31:48.04 +64:21:56.1
01:55:52.83 +64:15:23.8
00:39:36.45 +60:06:50.0
01:43:03.20 +58:57:12.7
00:47:38.45 +60:34:44.6
01:22:10.81 +59:09:03.1
01:36:51.89 +60:55:57.8
01:11:56.50 +58:41:04.4
02:05:23.00 +59:19:30.2
01:18:57.79 +59:46:45.7
01:21:12.70 +59:45:44.2
01:27:31.61 +59:41:05.3
01:21:54.46 +61:20:57.4
01:02:56.70 +59:37:23.2
02:39:28.93 +63:32:02.4
02:49:56.80 +63:51:39.7
###################################################################################
02:21:40.73 +60:54:42.6 -- not an asteroid (will add it to exclusion list)
01:30:59.69 +63:14:35.6 -- not an asteroid (will add it to exclusion list)
01:33:01.77 +59:16:33.3 -- not an asteroid (will add it to exclusion list)
01:10:07.77 +57:43:55.5 -- not an asteroid (will add it to exclusion list)
00:44:53.02 +61:53:14.0 -- not an asteroid (will add it to exclusion list)
01:00:39.98 +59:11:28.2 -- not an asteroid (will add it to exclusion list)
01:35:49.43 +58:50:38.6 -- not an asteroid (will add it to exclusion list)
01:06:12.88 +59:33:45.3 -- not an asteroid (will add it to exclusion list)
01:08:25.50 +59:48:04.1 -- not an asteroid (will add it to exclusion list)
01:16:59.09 +59:52:02.2 -- not an asteroid (will add it to exclusion list)
01:26:38.88 +59:41:40.0 -- not an asteroid (will add it to exclusion list)
02:47:16.64 +64:40:11.5 -- not an asteroid (will add it to exclusion list)
00:52:38.59 +58:02:49.0 -- not an asteroid (will add it to exclusion list)
00:44:13.32 +56:48:04.1 -- not an asteroid (will add it to exclusion list)
01:15:17.38 +57:44:02.4 -- not an asteroid (will add it to exclusion list)
00:44:18.27 +64:55:14.6 -- not an asteroid (will add it to exclusion list)
01:05:37.92 +58:00:04.3 -- not an asteroid (will add it to exclusion list)
00:56:49.03 +57:22:46.2 -- not an asteroid (will add it to exclusion list)
01:02:12.07 +57:26:33.3 -- not an asteroid (will add it to exclusion list)
02:10:56.02 +62:17:07.8 -- not an asteroid (will add it to exclusion list)
00:57:40.76 +56:52:14.1 -- not an asteroid (will add it to exclusion list)
01:25:19.92 +59:52:22.3 -- not an asteroid (will add it to exclusion list)
01:20:45.89 +57:55:24.6 -- not an asteroid (will add it to exclusion list)
01:01:47.58 +57:23:13.9 -- not an asteroid (will add it to exclusion list)
01:11:44.61 +61:13:56.2 -- not an asteroid (will add it to exclusion list)
00:36:45.76 +61:48:23.5 -- not an asteroid (will add it to exclusion list)
00:56:04.04 +60:39:34.5 -- not an asteroid (will add it to exclusion list)
01:22:28.16 +61:07:36.1 -- not an asteroid (will add it to exclusion list)
01:32:21.98 +60:27:29.4 -- not an asteroid (will add it to exclusion list)
00:54:30.96 +59:23:59.6 -- not an asteroid (will add it to exclusion list)
01:46:42.34 +61:09:51.6 -- not an asteroid (will add it to exclusion list)
00:56:47.36 +60:38:48.1 -- not an asteroid (will add it to exclusion list)
01:02:45.62 +58:39:34.2 -- not an asteroid (will add it to exclusion list)
01:15:00.94 +57:58:06.1 -- not an asteroid (will add it to exclusion list)
01:30:10.08 +59:36:18.7 -- not an asteroid (will add it to exclusion list)
00:54:20.36 +57:41:46.4 -- not an asteroid (will add it to exclusion list)
00:51:09.78 +60:42:30.8 -- not an asteroid (will add it to exclusion list)
01:26:05.85 +57:30:37.8 -- not an asteroid (will add it to exclusion list)
01:17:48.19 +57:17:33.7 -- not an asteroid (will add it to exclusion list)
01:27:51.63 +56:56:50.7 -- not an asteroid (will add it to exclusion list)
01:01:25.35 +57:50:14.0 -- not an asteroid (will add it to exclusion list)
00:56:45.50 +58:52:46.3 -- not an asteroid (will add it to exclusion list)
00:52:52.78 +58:28:52.0 -- not an asteroid (will add it to exclusion list)
01:25:15.32 +64:40:32.7 -- not an asteroid (will add it to exclusion list)
00:40:25.91 +61:07:15.7 -- not an asteroid (will add it to exclusion list)
00:40:43.95 +61:40:52.1 -- not an asteroid (will add it to exclusion list)
01:25:38.45 +59:16:00.4 -- not an asteroid (will add it to exclusion list)
01:12:40.83 +61:20:37.3 -- not an asteroid (will add it to exclusion list)
00:58:00.23 +57:24:06.3 -- not an asteroid (will add it to exclusion list)
00:51:25.51 +62:25:15.0 -- not an asteroid (will add it to exclusion list)
01:08:09.36 +60:42:14.9 -- not an asteroid (will add it to exclusion list)
00:52:22.50 +58:23:34.3 -- not an asteroid (will add it to exclusion list)
00:36:43.38 +64:22:47.7 -- not an asteroid (will add it to exclusion list)
01:25:56.68 +59:35:12.0 -- not an asteroid (will add it to exclusion list)
01:32:39.95 +63:11:27.6 -- not an asteroid (will add it to exclusion list)
01:35:37.54 +61:16:49.5 -- not an asteroid (will add it to exclusion list)
01:02:34.05 +59:16:48.9 -- not an asteroid (will add it to exclusion list)
00:52:16.20 +59:42:57.8 -- not an asteroid (will add it to exclusion list)
01:47:13.04 +57:44:19.0 -- not an asteroid (will add it to exclusion list)
00:41:14.65 +61:35:30.9 -- not an asteroid (will add it to exclusion list)
01:44:52.13 +57:41:42.0 -- not an asteroid (will add it to exclusion list)
01:46:30.07 +61:12:58.8 -- not an asteroid (will add it to exclusion list)
01:12:05.87 +59:41:19.7 -- not an asteroid (will add it to exclusion list)
02:19:17.63 +57:07:29.7 -- not an asteroid (will add it to exclusion list)
01:40:01.44 +60:52:32.0 -- not an asteroid (will add it to exclusion list)
01:08:15.62 +63:34:13.6 -- not an asteroid (will add it to exclusion list)
01:24:27.18 +58:44:16.9 -- not an asteroid (will add it to exclusion list)
00:58:55.96 +58:04:04.8 -- not an asteroid (will add it to exclusion list)
01:58:16.32 +59:38:59.0 -- not an asteroid (will add it to exclusion list)
01:18:14.06 +61:44:36.2 -- not an asteroid (will add it to exclusion list)
00:52:31.34 +58:35:21.3 -- not an asteroid (will add it to exclusion list)
01:07:57.13 +63:37:29.6 -- not an asteroid (will add it to exclusion list)
01:29:32.78 +61:46:26.2 -- not an asteroid (will add it to exclusion list)
01:14:45.20 +60:30:02.9 -- not an asteroid (will add it to exclusion list)
01:25:50.10 +61:06:31.1 -- not an asteroid (will add it to exclusion list)
01:03:22.59 +60:32:13.4 -- not an asteroid (will add it to exclusion list)
00:51:43.50 +57:16:06.5 -- not an asteroid (will add it to exclusion list)
00:35:28.33 +62:32:36.1 -- not an asteroid (will add it to exclusion list)
01:03:35.25 +60:28:07.9 -- not an asteroid (will add it to exclusion list)
01:44:32.29 +58:45:34.5 -- not an asteroid (will add it to exclusion list)
02:06:05.99 +57:07:10.0 -- not an asteroid (will add it to exclusion list)
02:11:23.08 +61:21:04.9 -- not an asteroid (will add it to exclusion list)
00:52:12.53 +64:57:21.7 -- not an asteroid (will add it to exclusion list)
01:08:31.65 +63:35:41.9 -- not an asteroid (will add it to exclusion list)
01:15:11.46 +60:07:02.8 -- not an asteroid (will add it to exclusion list)
00:47:11.28 +58:29:06.2 -- not an asteroid (will add it to exclusion list)
01:19:23.90 +58:26:39.0 -- not an asteroid (will add it to exclusion list)
00:48:13.83 +58:19:19.4 -- not an asteroid (will add it to exclusion list)
01:18:39.81 +58:25:50.7 -- not an asteroid (will add it to exclusion list)
01:58:39.97 +59:15:59.2 -- not an asteroid (will add it to exclusion list)
01:10:31.31 +60:31:13.0 -- not an asteroid (will add it to exclusion list)
02:16:10.72 +64:52:44.6 -- not an asteroid (will add it to exclusion list)
00:33:46.78 +63:27:55.5 -- not an asteroid (will add it to exclusion list)
00:51:32.88 +59:59:13.7 -- not an asteroid (will add it to exclusion list)
00:47:19.74 +56:59:25.7 -- not an asteroid (will add it to exclusion list)
01:50:38.77 +56:46:21.4 -- not an asteroid (will add it to exclusion list)
02:19:57.57 +59:32:26.1 -- not an asteroid (will add it to exclusion list)
01:59:33.16 +60:01:44.8 -- not an asteroid (will add it to exclusion list)
01:49:34.16 +61:03:37.2 -- not an asteroid (will add it to exclusion list)
01:44:01.00 +61:52:01.8 -- not an asteroid (will add it to exclusion list)
02:11:32.71 +61:10:00.8 -- not an asteroid (will add it to exclusion list)
01:31:08.96 +59:34:13.3 -- not an asteroid (will add it to exclusion list)
01:29:33.02 +63:19:32.3 -- not an asteroid (will add it to exclusion list)
01:29:21.35 +61:44:15.4 -- not an asteroid (will add it to exclusion list)
01:18:36.99 +58:41:38.2 -- not an asteroid (will add it to exclusion list)
01:35:10.85 +60:45:33.1 -- not an asteroid (will add it to exclusion list)
02:01:38.60 +61:45:15.1 -- not an asteroid (will add it to exclusion list)
01:19:41.71 +62:51:04.2 -- not an asteroid (will add it to exclusion list)
02:10:23.89 +60:01:12.9 -- not an asteroid (will add it to exclusion list)
01:46:38.37 +60:07:32.0 -- not an asteroid (will add it to exclusion list)
02:03:15.09 +62:12:10.7 -- not an asteroid (will add it to exclusion list)
02:10:32.76 +59:59:55.2 -- not an asteroid (will add it to exclusion list)
02:02:53.99 +60:15:40.7 -- not an asteroid (will add it to exclusion list)
01:52:48.49 +60:28:34.7 -- not an asteroid (will add it to exclusion list)
01:09:51.31 +57:04:44.9 -- not an asteroid (will add it to exclusion list)
01:40:34.64 +60:45:54.0 -- not an asteroid (will add it to exclusion list)
01:36:07.33 +59:27:16.2 -- not an asteroid (will add it to exclusion list)
02:01:36.75 +59:57:22.0 -- not an asteroid (will add it to exclusion list)
01:07:32.39 +61:11:22.8 -- not an asteroid (will add it to exclusion list)
01:38:33.68 +60:47:23.0 -- not an asteroid (will add it to exclusion list)
01:01:58.34 +58:30:09.1 -- not an asteroid (will add it to exclusion list)
01:13:54.14 +58:12:33.3 -- not an asteroid (will add it to exclusion list)
01:54:53.18 +58:16:51.3 -- not an asteroid (will add it to exclusion list)
00:56:24.23 +61:31:26.1 -- not an asteroid (will add it to exclusion list)
01:11:41.10 +58:17:28.2 -- not an asteroid (will add it to exclusion list)
01:22:23.35 +61:13:51.6 -- not an asteroid (will add it to exclusion list)
01:35:47.16 +61:18:13.3 -- not an asteroid (will add it to exclusion list)
01:38:06.41 +58:10:40.1 -- not an asteroid (will add it to exclusion list)
01:31:48.04 +64:21:56.1 -- not an asteroid (will add it to exclusion list)
01:55:52.83 +64:15:23.8 -- not an asteroid (will add it to exclusion list)
00:39:36.45 +60:06:50.0 -- not an asteroid (will add it to exclusion list)
01:43:03.20 +58:57:12.7 -- not an asteroid (will add it to exclusion list)
00:47:38.45 +60:34:44.6 -- not an asteroid (will add it to exclusion list)
01:22:10.81 +59:09:03.1 -- not an asteroid (will add it to exclusion list)
01:36:51.89 +60:55:57.8 -- not an asteroid (will add it to exclusion list)
01:11:56.50 +58:41:04.4 -- not an asteroid (will add it to exclusion list)
02:05:23.00 +59:19:30.2 -- not an asteroid (will add it to exclusion list)
01:18:57.79 +59:46:45.7 -- not an asteroid (will add it to exclusion list)
01:21:12.70 +59:45:44.2 -- not an asteroid (will add it to exclusion list)
01:27:31.61 +59:41:05.3 -- not an asteroid (will add it to exclusion list)
01:21:54.46 +61:20:57.4 -- not an asteroid (will add it to exclusion list)
01:02:56.70 +59:37:23.2 -- not an asteroid (will add it to exclusion list)
02:39:28.93 +63:32:02.4 -- not an asteroid (will add it to exclusion list)
02:49:56.80 +63:51:39.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:33:46.78 +63:27:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:28.33 +62:32:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:43.38 +64:22:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:45.76 +61:48:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:36.45 +60:06:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:25.91 +61:07:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:43.95 +61:40:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:14.65 +61:35:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:13.32 +56:48:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:18.27 +64:55:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:53.02 +61:53:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:11.28 +58:29:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:19.74 +56:59:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:38.45 +60:34:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:13.83 +58:19:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:09.78 +60:42:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:25.51 +62:25:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:32.88 +59:59:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:43.50 +57:16:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:12.53 +64:57:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:16.20 +59:42:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:22.50 +58:23:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:31.34 +58:35:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:38.59 +58:02:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:52.78 +58:28:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:20.36 +57:41:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:30.96 +59:23:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:04.04 +60:39:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:24.23 +61:31:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:45.50 +58:52:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:47.36 +60:38:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:49.03 +57:22:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:40.76 +56:52:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:00.23 +57:24:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:55.96 +58:04:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:39.98 +59:11:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:25.35 +57:50:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:47.58 +57:23:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:58.34 +58:30:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:12.07 +57:26:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:34.05 +59:16:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:45.62 +58:39:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:56.70 +59:37:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:22.59 +60:32:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:35.25 +60:28:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:37.92 +58:00:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:12.88 +59:33:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:32.39 +61:11:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:57.13 +63:37:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:09.36 +60:42:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:15.62 +63:34:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:25.50 +59:48:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:31.65 +63:35:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:51.31 +57:04:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:07.77 +57:43:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:31.31 +60:31:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:41.10 +58:17:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:44.61 +61:13:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:56.50 +58:41:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:05.87 +59:41:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:40.83 +61:20:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:54.14 +58:12:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:45.20 +60:30:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:00.94 +57:58:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:11.46 +60:07:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:17.38 +57:44:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:59.09 +59:52:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:48.19 +57:17:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:14.06 +61:44:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:36.99 +58:41:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:39.81 +58:25:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:57.79 +59:46:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:23.90 +58:26:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:41.71 +62:51:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:45.89 +57:55:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:12.70 +59:45:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:54.46 +61:20:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:10.81 +59:09:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:23.35 +61:13:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:28.16 +61:07:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:27.18 +58:44:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:15.32 +64:40:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:19.92 +59:52:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:38.45 +59:16:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:50.10 +61:06:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:56.68 +59:35:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.85 +57:30:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:38.88 +59:41:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:31.61 +59:41:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:51.63 +56:56:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:21.35 +61:44:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.78 +61:46:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:33.02 +63:19:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:10.08 +59:36:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:59.69 +63:14:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:08.96 +59:34:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.04 +64:21:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:21.98 +60:27:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:39.95 +63:11:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:01.77 +59:16:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:10.85 +60:45:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:37.54 +61:16:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:47.16 +61:18:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:49.43 +58:50:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:07.33 +59:27:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:51.89 +60:55:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:06.41 +58:10:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:33.68 +60:47:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:01.44 +60:52:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:34.64 +60:45:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.20 +58:57:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:01.00 +61:52:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:32.29 +58:45:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:52.13 +57:41:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:30.07 +61:12:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.37 +60:07:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:42.34 +61:09:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:13.04 +57:44:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:34.16 +61:03:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:38.77 +56:46:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:48.49 +60:28:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:53.18 +58:16:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:52.83 +64:15:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:16.32 +59:38:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:39.97 +59:15:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:33.16 +60:01:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:36.75 +59:57:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:38.60 +61:45:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:53.99 +60:15:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:15.09 +62:12:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:23.00 +59:19:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:05.99 +57:07:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:23.89 +60:01:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:32.76 +59:59:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:56.02 +62:17:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:23.08 +61:21:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:32.71 +61:10:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:10.72 +64:52:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:17.63 +57:07:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:57.57 +59:32:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:40.73 +60:54:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:28.93 +63:32:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:47:16.64 +64:40:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:56.80 +63:51:39.7 -- 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)
00:33:46.78 +63:27:55.5 -- not a known variable star
00:35:28.33 +62:32:36.1 -- not a known variable star
00:36:43.38 +64:22:47.7 -- not a known variable star
00:36:45.76 +61:48:23.5 -- a known variable star
00:39:36.45 +60:06:50.0 -- a known variable star
00:40:25.91 +61:07:15.7 -- not a known variable star
00:40:43.95 +61:40:52.1 -- not a known variable star
00:41:14.65 +61:35:30.9 -- a known variable star
00:44:13.32 +56:48:04.1 -- a known variable star
00:44:18.27 +64:55:14.6 -- not a known variable star
00:44:53.02 +61:53:14.0 -- not a known variable star
00:47:11.28 +58:29:06.2 -- not a known variable star
00:47:19.74 +56:59:25.7 -- not a known variable star
00:47:38.45 +60:34:44.6 -- not a known variable star
00:48:13.83 +58:19:19.4 -- a known variable star
00:51:09.78 +60:42:30.8 -- not a known variable star
00:51:25.51 +62:25:15.0 -- not a known variable star
00:51:32.88 +59:59:13.7 -- not a known variable star
00:51:43.50 +57:16:06.5 -- not a known variable star
00:52:12.53 +64:57:21.7 -- not a known variable star
00:52:16.20 +59:42:57.8 -- a known variable star
00:52:22.50 +58:23:34.3 -- not a known variable star
00:52:31.34 +58:35:21.3 -- a known variable star
00:52:38.59 +58:02:49.0 -- not a known variable star
00:52:52.78 +58:28:52.0 -- not a known variable star
00:54:20.36 +57:41:46.4 -- not a known variable star
00:54:30.96 +59:23:59.6 -- a known variable star
00:56:04.04 +60:39:34.5 -- a known variable star
00:56:24.23 +61:31:26.1 -- not a known variable star
00:56:45.50 +58:52:46.3 -- not a known variable star
00:56:47.36 +60:38:48.1 -- not a known variable star
00:56:49.03 +57:22:46.2 -- not a known variable star
00:57:40.76 +56:52:14.1 -- not a known variable star
00:58:00.23 +57:24:06.3 -- not a known variable star
00:58:55.96 +58:04:04.8 -- not a known variable star
01:00:39.98 +59:11:28.2 -- not a known variable star
01:01:25.35 +57:50:14.0 -- not a known variable star
01:01:47.58 +57:23:13.9 -- not a known variable star
01:01:58.34 +58:30:09.1 -- not a known variable star
01:02:12.07 +57:26:33.3 -- not a known variable star
01:02:34.05 +59:16:48.9 -- not a known variable star
01:02:45.62 +58:39:34.2 -- a known variable star
01:02:56.70 +59:37:23.2 -- not a known variable star
01:03:22.59 +60:32:13.4 -- not a known variable star
01:03:35.25 +60:28:07.9 -- not a known variable star
01:05:37.92 +58:00:04.3 -- not a known variable star
01:06:12.88 +59:33:45.3 -- not a known variable star
01:07:32.39 +61:11:22.8 -- not a known variable star
01:07:57.13 +63:37:29.6 -- a known variable star
01:08:09.36 +60:42:14.9 -- not a known variable star
01:08:15.62 +63:34:13.6 -- not a known variable star
01:08:25.50 +59:48:04.1 -- not a known variable star
01:08:31.65 +63:35:41.9 -- a known variable star
01:09:51.31 +57:04:44.9 -- a known variable star
01:10:07.77 +57:43:55.5 -- not a known variable star
01:10:31.31 +60:31:13.0 -- not a known variable star
01:11:41.10 +58:17:28.2 -- not a known variable star
01:11:44.61 +61:13:56.2 -- a known variable star
01:11:56.50 +58:41:04.4 -- not a known variable star
01:12:05.87 +59:41:19.7 -- not a known variable star
01:12:40.83 +61:20:37.3 -- not a known variable star
01:13:54.14 +58:12:33.3 -- not a known variable star
01:14:45.20 +60:30:02.9 -- not a known variable star
01:15:00.94 +57:58:06.1 -- not a known variable star
01:15:11.46 +60:07:02.8 -- a known variable star
01:15:17.38 +57:44:02.4 -- not a known variable star
01:16:59.09 +59:52:02.2 -- a known variable star
01:17:48.19 +57:17:33.7 -- not a known variable star
01:18:14.06 +61:44:36.2 -- not a known variable star
01:18:36.99 +58:41:38.2 -- a known variable star
01:18:39.81 +58:25:50.7 -- not a known variable star
01:18:57.79 +59:46:45.7 -- a known variable star
01:19:23.90 +58:26:39.0 -- not a known variable star
01:19:41.71 +62:51:04.2 -- not a known variable star
01:20:45.89 +57:55:24.6 -- not a known variable star
01:21:12.70 +59:45:44.2 -- not a known variable star
01:21:54.46 +61:20:57.4 -- a known variable star
01:22:10.81 +59:09:03.1 -- not a known variable star
01:22:23.35 +61:13:51.6 -- a known variable star
01:22:28.16 +61:07:36.1 -- a known variable star
01:24:27.18 +58:44:16.9 -- not a known variable star
01:25:15.32 +64:40:32.7 -- not a known variable star
01:25:19.92 +59:52:22.3 -- not a known variable star
01:25:38.45 +59:16:00.4 -- not a known variable star
01:25:50.10 +61:06:31.1 -- not a known variable star
01:25:56.68 +59:35:12.0 -- not a known variable star
01:26:05.85 +57:30:37.8 -- not a known variable star
01:26:38.88 +59:41:40.0 -- a known variable star
01:27:31.61 +59:41:05.3 -- not a known variable star
01:27:51.63 +56:56:50.7 -- not a known variable star
01:29:21.35 +61:44:15.4 -- not a known variable star
01:29:32.78 +61:46:26.2 -- not a known variable star
01:29:33.02 +63:19:32.3 -- a known variable star
01:30:10.08 +59:36:18.7 -- not a known variable star
01:30:59.69 +63:14:35.6 -- not a known variable star
01:31:08.96 +59:34:13.3 -- not a known variable star
01:31:48.04 +64:21:56.1 -- not a known variable star
01:32:21.98 +60:27:29.4 -- not a known variable star
01:32:39.95 +63:11:27.6 -- not a known variable star
01:33:01.77 +59:16:33.3 -- not a known variable star
01:35:10.85 +60:45:33.1 -- a known variable star
01:35:37.54 +61:16:49.5 -- a known variable star
01:35:47.16 +61:18:13.3 -- not a known variable star
01:35:49.43 +58:50:38.6 -- not a known variable star
01:36:07.33 +59:27:16.2 -- not a known variable star
01:36:51.89 +60:55:57.8 -- not a known variable star
01:38:06.41 +58:10:40.1 -- a known variable star
01:38:33.68 +60:47:23.0 -- not a known variable star
01:40:01.44 +60:52:32.0 -- not a known variable star
01:40:34.64 +60:45:54.0 -- not a known variable star
01:43:03.20 +58:57:12.7 -- not a known variable star
01:44:01.00 +61:52:01.8 -- not a known variable star
01:44:32.29 +58:45:34.5 -- not a known variable star
01:44:52.13 +57:41:42.0 -- a known variable star
01:46:30.07 +61:12:58.8 -- not a known variable star
01:46:38.37 +60:07:32.0 -- not a known variable star
01:46:42.34 +61:09:51.6 -- a known variable star
01:47:13.04 +57:44:19.0 -- a known variable star
01:49:34.16 +61:03:37.2 -- not a known variable star
01:50:38.77 +56:46:21.4 -- not a known variable star
01:52:48.49 +60:28:34.7 -- not a known variable star
01:54:53.18 +58:16:51.3 -- not a known variable star
01:55:52.83 +64:15:23.8 -- not a known variable star
01:58:16.32 +59:38:59.0 -- not a known variable star
01:58:39.97 +59:15:59.2 -- a known variable star
01:59:33.16 +60:01:44.8 -- a known variable star
02:01:36.75 +59:57:22.0 -- not a known variable star
02:01:38.60 +61:45:15.1 -- not a known variable star
02:02:53.99 +60:15:40.7 -- not a known variable star
02:03:15.09 +62:12:10.7 -- a known variable star
02:05:23.00 +59:19:30.2 -- a known variable star
02:06:05.99 +57:07:10.0 -- not a known variable star
02:10:23.89 +60:01:12.9 -- not a known variable star
02:10:32.76 +59:59:55.2 -- a known variable star
02:10:56.02 +62:17:07.8 -- a known variable star
02:11:23.08 +61:21:04.9 -- a known variable star
02:11:32.71 +61:10:00.8 -- not a known variable star
02:16:10.72 +64:52:44.6 -- not a known variable star
02:19:17.63 +57:07:29.7 -- a known variable star
02:19:57.57 +59:32:26.1 -- not a known variable star
02:21:40.73 +60:54:42.6 -- a known variable star
02:39:28.93 +63:32:02.4 -- a known variable star
02:47:16.64 +64:40:11.5 -- not a known variable star
02:49:56.80 +63:51:39.7 -- not a known variable star
Found 105 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
144 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 144 (excluding asteroids and hot pixels, 105 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)2461191.93302642 -observatory V36
05:50:14.96 +25:33:30.1 Mercury (-0.6mag)
07:03:14.48 +24:33:52.7 Venus (-3.9mag)
02:27:09.55 +13:53:07.9 Mars (1.3mag)
07:42:06.62 +21:46:52.1 Jupiter (-1.9mag)
00:47:01.86 +02:35:41.6 Saturn (0.9mag)
03:58:20.65 +20:20:03.5 Uranus (5.8mag)
00:15:38.00 +00:13:54.9 Neptune (7.8mag)
20:33:44.25 -23:01:46.7 Pluto (14.5mag)
16:29:07.05 -27:32:26.8 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 363 May 31 05:37 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461191.93302642:
07:42:03.04 +21:47:01.1 Io (6.0mag)
07:41:57.48 +21:47:19.5 Europa (6.1mag)
07:41:53.27 +21:47:27.2 Ganymede (5.5mag)
07:41:57.45 +21:47:24.7 Callisto (6.8mag)
07:42:52.38 +21:22:58.1 Himalia (15.6mag)
07:42:04.10 +21:47:00.5 Thebe (16.5mag)
07:43:03.92 +21:41:53.6 Elara (17.5mag)
07:43:52.31 +22:02:47.2 Pasiphae (17.7mag)
07:49:01.34 +21:48:01.9 Carme (18.8mag)
00:47:11.97 +02:35:53.1 Titan (8.7mag)
00:47:00.18 +02:35:38.3 Rhea (10.0mag)
00:47:32.10 +02:36:45.3 Iapetus (11.4mag)
00:46:59.58 +02:36:12.2 Hyperion (14.7mag)
00:47:53.41 +02:38:44.5 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 31 05:37 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461191.93302642:
17:20:45.90 -34:18:27.4 JWST
15:25:03.15 +52:13:31.3 Chandra
01:37:53.74 +63:57:27.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 31 05:37 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461191.93302642 -observatory V36
18:48:20.65 -32:04:06.4 13.7mag P/2010 H2 (Vales)
05:45:54.46 -68:10:10.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:46:13.79 +31:52:13.6 17.5mag C/2017 K2 (PANSTARRS)
17:17:49.42 +14:54:30.4 17.8mag C/2021 G2 (ATLAS)
20:08:40.29 -51:31:01.7 17.6mag P/2021 N1 (ZTF)
23:13:59.89 +31:16:38.6 17.2mag C/2022 E2 (ATLAS)
05:24:29.66 +26:54:54.3 16.4mag C/2022 N2 (PANSTARRS)
09:24:21.36 +31:20:17.0 16.6mag C/2022 QE78 (ATLAS)
08:46:32.65 +03:31:39.8 17.6mag C/2022 R6 (PANSTARRS)
18:33:10.06 +21:23:58.9 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:22:18.85 -11:00:54.1 17.5mag P/2023 B1 (PANSTARRS)
22:16:04.21 +66:01:34.5 17.7mag C/2023 H5 (Lemmon)
18:05:06.77 -05:58:17.4 13.7mag C/2023 R1 (PANSTARRS)
13:26:27.67 +84:42:31.0 17.9mag C/2023 X2 (Lemmon)
07:00:01.78 +64:04:05.9 17.6mag C/2024 A1 (ATLAS)
06:35:16.01 +27:04:26.0 13.3mag C/2024 E1 (Wierzchos)
15:43:31.80 +12:46:55.9 17.4mag C/2024 G6 (ATLAS)
20:17:30.16 +28:47:16.7 14.1mag C/2024 J3 (ATLAS)
04:10:14.50 -16:40:21.0 16.1mag C/2024 T5 (ATLAS)
05:58:37.60 +35:51:43.0 17.9mag C/2025 J1 (Borisov)
11:40:11.10 +53:08:41.2 17.1mag C/2025 L1 (ATLAS)
06:34:11.71 -10:30:05.8 13.3mag C/2025 R3 (PANSTARRS)
09:18:12.09 +23:24:32.3 18.0mag C/2025 V2 (Rankin)
12:40:13.76 +04:40:27.9 17.2mag C/2025 Y1 (ATLAS)
01:46:32.65 +42:49:32.5 15.9mag C/2026 B2 (Sun-Gao)
11:10:20.89 -06:42:19.8 16.3mag A/2026 E1
20:09:23.95 -08:12:04.4 9.2mag 10P/Tempel
11:00:27.54 -00:53:14.1 15.9mag 29P/Schwassmann-Wachmann
10:54:58.41 -02:37:07.2 17.9mag 43P/Wolf-Harrington
02:59:39.65 +24:34:56.0 17.6mag 47P/Ashbrook-Jackson
08:43:25.63 +25:56:36.0 16.9mag 63P/Wild
00:19:56.40 -06:54:37.2 15.7mag 65P/Gunn
06:18:23.99 +32:29:30.1 16.7mag 76P/West-Kohoutek-Ikemura
02:50:30.27 +16:09:54.3 13.9mag 78P/Gehrels
01:03:24.75 +03:05:16.1 15.4mag 88P/Howell
04:29:38.22 +29:34:55.3 15.2mag 93P/Lovas
02:21:27.52 +26:18:42.0 17.8mag 114P/Wiseman-Skiff
06:32:12.33 +33:15:06.3 15.7mag 123P/West-Hartley
09:36:49.55 +17:58:57.3 16.5mag 124P/Mrkos
03:46:14.40 +18:41:54.3 16.4mag 128P/Shoemaker-Holt
04:18:04.95 +18:40:41.5 17.7mag 131P/Mueller
05:23:37.82 +19:23:02.8 13.7mag 141P/Machholz
05:26:06.98 +17:03:14.5 13.6mag 141P-A/Machholz
04:14:11.97 +14:51:56.1 10.9mag 141P-D/Machholz
02:52:05.30 -25:49:50.7 17.1mag 161P/Hartley-IRAS
03:16:26.92 +20:33:47.4 14.9mag 162P/SidingSpring
19:36:07.60 -00:24:32.6 17.3mag 169P/NEAT
23:57:16.78 +00:53:44.5 18.0mag 220P/McNaught
16:58:14.83 -08:56:47.0 16.3mag 235P/LINEAR
07:17:01.81 +35:45:16.9 17.4mag 240P/NEAT
00:12:06.99 -05:41:11.9 16.6mag 260P/McNaught
03:43:32.90 +30:59:54.3 17.6mag 295P/LINEAR
22:54:12.54 -20:21:55.5 17.6mag 320P/McNaught
15:18:58.72 +08:17:58.2 17.4mag 391P/Kowalski
08:01:06.79 +20:55:53.4 17.9mag 450P/LONEOS
06:47:18.75 +42:14:07.8 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K May 31 05:37 comets.txt
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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 05:37 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 31 05:37 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:06:45.820 +14:12:31.59 AT 2026nej 2026-05-17.91 20.02
18:31:04.068 +41:19:12.55 AT 2026nei 2026-05-19.07 19.8
21:33:15.841 +03:06:48.93 SN 2026neh 2026-05-18.17 20.15
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
-rw-r--r-- 1 apache apache 30K May 31 05:37 tns_transients_list.txt
