This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.24 01:16:28.89 +60:14:00.6
126.03851 -2.48710 galactic Cas Second-epoch detections are separated by 0.3" and 3.1 pix
The object was found in ASASSN-V 1" ASASSN-V J011628.82+601400.9
Type: SR
MeanMag 13.24 m Amp. 0.36 m Period 128.0 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:28.89 +60:14:00.6: 14.74 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:28.89 +60:14:00.6: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 16 28.89 +60 14 00.6 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
VARIABLE_NAME,2461202.9230,11.24,0.05,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
VARIABLE_NAME 20260611.4230 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 8.69 01:56:38.08 +59:15:34.3
131.18811 -2.56312 galactic Cas Second-epoch detections are separated by 0.2" and 3.2 pix
The object was found in VSX 1" X Cas
Type: M
# Max. Min./Amp. JD0 Period
9.450 V 13.200 V 2457020.00000 415.000000000000 C5,4e(N1e)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.08 +59:15:34.3: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.08 +59:15:34.3: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 56 38.08 +59 15 34.3 8.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X Cas,2461202.9230,8.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
X Cas 20260611.4230 8.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.53 02:21:40.70 +60:54:42.3
133.68140 -0.06260 galactic Cas Second-epoch detections are separated by 0.2" and 3.1 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 02:21:40.70 +60:54:42.3: 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 02:21:40.70 +60:54:42.3: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 21 40.70 +60 54 42.3 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DE Cas,2461202.9230,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DE Cas 20260611.4230 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.53 02:00:42.05 +61:18:04.8
131.14939 -0.46046 galactic Cas Second-epoch detections are separated by 3.4" 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 | target | 02:00:42.05 +61:18:04.8 (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 02:00:42.05 +61:18:04.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:42.05 +61:18:04.8: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 00 42.05 +61 18 04.8 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.46 01:29:16.07 +60:15:48.3
127.61052 -2.26423 galactic Cas Second-epoch detections are separated by 3.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.2936+60.2624 | 01:29:16.07 +60:15:48.3 (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 01:29:16.07 +60:15:48.3: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:16.07 +60:15:48.3: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 29 16.07 +60 15 48.3 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
ATO J022.2936+60.2624,2461202.9230,11.46,0.05,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
ATO J022.2936+60.2624 20260611.4230 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.36 02:41:51.08 +62:00:32.2
135.49883 1.86164 galactic Cas Second-epoch detections are separated by 6.5" and 3.1 pix
The object was found in VSX 3" Gaia DR3 465796079504481920
Type: VAR
# Max. Min./Amp. JD0 Period
13.690 G 13.730 G 0.202867000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:41:51.08 +62:00:32.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:41:51.08 +62:00:32.2: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 41 51.08 +62 00 32.2 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 465796079504481920,2461202.9230,11.36,0.05,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 465796079504481920 20260611.4230 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.60 01:04:16.84 +62:17:14.4
124.42446 -0.54719 galactic Cas Second-epoch detections are separated by 2.4" 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 | 01:04:16.84 +62:17:14.4 (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 01:04:16.84 +62:17:14.4: 11.88 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:16.84 +62:17:14.4: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 04 16.84 +62 17 14.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.38 01:08:25.44 +59:48:04.0
125.06940 -3.00012 galactic Cas Second-epoch detections are separated by 2.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:08:25.44 +59:48:04.0 (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 01:08:25.44 +59:48:04.0: 12.24 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.44 +59:48:04.0: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 08 25.44 +59 48 04.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.38,0.05,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
target 20260611.4230 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.14 02:52:58.74 +63:23:24.0
136.05381 3.65799 galactic Cas Second-epoch detections are separated by 6.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:52:58.74 +63:23:24.0 (user input) | T | P | (position from user input) J-Ks=0.291+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:52:58.74 +63:23:24.0: 12.55 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:52:58.74 +63:23:24.0: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 52 58.74 +63 23 24.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.14,0.05,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
target 20260611.4230 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.24 01:37:41.97 +59:27:45.8
128.78603 -2.88218 galactic Cas Second-epoch detections are separated by 0.8" 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 J024.4151+59.4568 | 01:37:41.97 +59:27:45.8 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:41.97 +59:27:45.8: 13.36 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:41.97 +59:27:45.8: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 37 41.97 +59 27 45.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.4151+59.4568,2461202.9230,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.4151+59.4568 20260611.4230 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.08 02:41:58.35 +60:23:19.7
136.18086 0.39191 galactic Cas Second-epoch detections are separated by 4.5" 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 | 02:41:58.35 +60:23:19.7 (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 02:41:58.35 +60:23:19.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:41:58.35 +60:23:19.7: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 41 58.35 +60 23 19.7 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
target,2461202.9230,11.08,0.05,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 20260611.4230 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.29 00:59:30.61 +62:53:54.5
123.85113 0.04113 galactic Cas Second-epoch detections are separated by 0.8" 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 | 00:59:30.61 +62:53:54.5 (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 00:59:30.61 +62:53:54.5: 12.65 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:59:30.61 +62:53:54.5: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 59 30.61 +62 53 54.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.10 02:38:12.38 +59:36:40.8
136.06659 -0.50975 galactic Cas Second-epoch detections are separated by 8.2" and 4.0 pix
The object was found in VSX21" Gaia DR3 464292462990272896
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.590 G 13.630 G 0.016292200000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:12.38 +59:36:40.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:12.38 +59:36:40.8: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 38 12.38 +59 36 40.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 464292462990272896,2461202.9230,11.10,0.05,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 464292462990272896 20260611.4230 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.54 01:02:45.81 +63:46:48.9
124.18263 0.93601 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 01:02:45.81 +63:46:48.9 (user input) | T | P | (position from user input) J-Ks=0.928+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:45.81 +63:46:48.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:45.81 +63:46:48.9: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 02 45.81 +63 46 48.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.54,0.05,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
target 20260611.4230 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.26 01:55:53.64 +64:36:21.5
129.77478 2.59400 galactic Cas Second-epoch detections are separated by 1.6" and 2.7 pix
The object was found in VSX 6" ASASSN-V J015553.53+643615.5
Type: SR
# Max. Min./Amp. JD0 Period
16.030 g Y 0.620 g 2459493.06800 142.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:53.64 +64:36:21.5: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:53.64 +64:36:21.5: 14.75 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 55 53.64 +64 36 21.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J015553.53+643615.5,2461202.9230,11.26,0.05,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
ASASSN-V J015553.53+643615.5 20260611.4230 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.11 00:52:45.42 +63:28:59.5
123.07915 0.61182 galactic Cas Second-epoch detections are separated by 3.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:52:45.42 +63:28:59.5 (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 00:52:45.42 +63:28:59.5: 12.99 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:45.42 +63:28:59.5: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 52 45.42 +63 28 59.5 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.11,0.05,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
target 20260611.4230 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.34 00:39:51.75 +62:45:29.3
121.60771 -0.08384 galactic Cas Second-epoch detections are separated by 1.1" 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 | 00:39:51.75 +62:45:29.3 (user input) | T | P | (position from user input) J-Ks=0.851+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:39:51.75 +62:45:29.3: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:39:51.75 +62:45:29.3: 14.13 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 39 51.75 +62 45 29.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.12 00:59:24.06 +57:51:42.7
123.99481 -4.99345 galactic Cas Second-epoch detections are separated by 1.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:59:24.06 +57:51:42.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.331+/-0.042 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:59:24.06 +57:51:42.7: 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 00:59:24.06 +57:51:42.7: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 59 24.06 +57 51 42.7 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
target,2461202.9230,11.12,0.05,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
target 20260611.4230 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.04 01:15:35.37 +59:15:09.5
126.02027 -3.47421 galactic Cas Second-epoch detections are separated by 7.7" 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 | ATO J018.8875+59.2574 | 01:15:35.37 +59:15:09.5 (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 01:15:35.37 +59:15:09.5: 11.69 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:35.37 +59:15:09.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 15 35.37 +59 15 09.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.8875+59.2574,2461202.9230,11.04,0.05,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
ATO J018.8875+59.2574 20260611.4230 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.02 00:46:28.44 +58:20:30.0
122.27859 -4.52378 galactic Cas Second-epoch detections are separated by 1.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:46:28.44 +58:20:30.0 (user input) | T | P | (position from user input) J-Ks=0.842+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:46:28.44 +58:20:30.0: 11.79 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:46:28.44 +58:20:30.0: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 46 28.44 +58 20 30.0 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.02,0.05,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
target 20260611.4230 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.96 01:54:24.92 +59:00:13.7
130.97483 -2.88099 galactic Cas Second-epoch detections are separated by 3.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J028.6069+59.0028 | 01:54:24.92 +59:00:13.7 (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 01:54:24.92 +59:00:13.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:24.92 +59:00:13.7: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 54 24.92 +59 00 13.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.6069+59.0028,2461202.9230,10.96,0.05,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
ATO J028.6069+59.0028 20260611.4230 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.82 01:49:30.14 +57:16:28.7
130.74637 -4.71350 galactic Cas Second-epoch detections are separated by 1.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:49:30.14 +57:16:28.7 (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 01:49:30.14 +57:16:28.7: 11.85 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:30.14 +57:16:28.7: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 49 30.14 +57 16 28.7 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
target,2461202.9230,10.82,0.05,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
target 20260611.4230 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 06 11.4230 2461202.9230 10.87 01:52:49.00 +56:57:10.2
131.26006 -4.92314 galactic Per Second-epoch detections are separated by 5.1" and 4.1 pix
The object was found in VSX 8" Gaia DR3 505680863800132096
Type: VAR
# Max. Min./Amp. JD0 Period
13.680 G 13.730 G 0.078408900000 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 01:52:49.00 +56:57:10.2: 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 01:52:49.00 +56:57:10.2: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 52 49.00 +56 57 10.2 10.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505680863800132096,2461202.9230,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505680863800132096 20260611.4230 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.91 01:21:38.69 +59:26:15.1
126.76958 -3.20895 galactic Cas Second-epoch detections are separated by 7.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:21:38.69 +59:26:15.1 (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 01:21:38.69 +59:26:15.1: 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 01:21:38.69 +59:26:15.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 21 38.69 +59 26 15.1 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
target,2461202.9230,10.91,0.05,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 20260611.4230 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.97 00:44:53.41 +58:45:49.8
122.08097 -4.09710 galactic Cas Second-epoch detections are separated by 3.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:44:53.41 +58:45:49.8 (user input) | T | P | (position from user input) J-Ks=0.921+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:44:53.41 +58:45:49.8: 10.97 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:53.41 +58:45:49.8: 13.47 +/- 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 06 11.4230* 00 44 53.41 +58 45 49.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.91 01:48:02.36 +60:59:06.6
129.74316 -1.13585 galactic Cas Second-epoch detections are separated by 1.3" and 3.1 pix
The object was found in VSX10" Gaia DR3 511199312662429568
Type: ROT
# Max. Min./Amp. JD0 Period
13.710 G 13.750 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 01:48:02.36 +60:59:06.6: 12.97 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:02.36 +60:59:06.6: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 48 02.36 +60 59 06.6 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
Gaia DR3 511199312662429568,2461202.9230,10.91,0.05,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 511199312662429568 20260611.4230 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.00 01:10:11.71 +59:17:24.9
125.32918 -3.49416 galactic Cas Second-epoch detections are separated by 1.0" 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 | ATO J017.5672+59.2942 | 01:10:11.71 +59:17:24.9 (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 01:10:11.71 +59:17:24.9: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:11.71 +59:17:24.9: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 10 11.71 +59 17 24.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.5672+59.2942,2461202.9230,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.5672+59.2942 20260611.4230 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.79 02:15:24.05 +59:54:56.8
133.27882 -1.25848 galactic Cas Second-epoch detections are separated by 1.7" 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 | ATO J033.8681+59.9093 | 02:15:24.05 +59:54:56.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:24.05 +59:54:56.8: 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 02:15:24.05 +59:54:56.8: 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 06 11.4230* 02 15 24.05 +59 54 56.8 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 J033.8681+59.9093,2461202.9230,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J033.8681+59.9093 20260611.4230 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.88 01:11:44.76 +61:13:57.4
125.37369 -1.54282 galactic Cas Second-epoch detections are separated by 1.6" and 3.2 pix
The object was found in VSX 0" 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 01:11:44.76 +61:13:57.4: 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 01:11:44.76 +61:13:57.4: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 11 44.76 +61 13 57.4 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
ZTF J011144.73+611356.9,2461202.9230,10.88,0.05,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
ZTF J011144.73+611356.9 20260611.4230 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 06 11.4230 2461202.9230 10.80 02:33:58.68 +56:29:45.2
136.77626 -3.59444 galactic Per Second-epoch detections are separated by 2.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:33:58.68 +56:29:45.2 (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 02:33:58.68 +56:29:45.2: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:58.68 +56:29:45.2: 13.23 +/- 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 06 11.4230* 02 33 58.68 +56 29 45.2 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.80,0.05,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
target 20260611.4230 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 06 11.4230 2461202.9230 10.84 00:52:38.68 +58:02:49.1
123.09214 -4.82440 galactic Cas Second-epoch detections are separated by 1.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.1739+58.0472 | 00:52:38.68 +58:02:49.1 (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 00:52:38.68 +58:02:49.1: 11.46 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:38.68 +58:02:49.1: 13.37 +/- 0.04 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 06 11.4230* 00 52 38.68 +58 02 49.1 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
ATO J013.1739+58.0472,2461202.9230,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J013.1739+58.0472 20260611.4230 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.78 02:04:54.31 +64:12:10.2
130.82088 2.46218 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 | target | 02:04:54.31 +64:12:10.2 (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 02:04:54.31 +64:12:10.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:54.31 +64:12:10.2: 14.25 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 04 54.31 +64 12 10.2 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
target,2461202.9230,10.78,0.05,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
target 20260611.4230 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.76 01:39:23.91 +58:23:02.3
129.19866 -3.90301 galactic Cas Second-epoch detections are separated by 3.8" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509053684438626432 | 01:39:28.48 +58:23:29.9 (Gaia DR3) | ROT (local) | G (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:23.91 +58:23:02.3: 12.43 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:23.91 +58:23:02.3: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 39 23.91 +58 23 02.3 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 509053684438626432,2461202.9230,10.76,0.05,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 509053684438626432 20260611.4230 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.78 00:45:11.09 +57:46:43.2
122.09518 -5.08292 galactic Cas Second-epoch detections are separated by 1.6" and 3.1 pix
The object was found in VSX16" Gaia DR3 424722413899081088
Type: RS
# Max. Min./Amp. JD0 Period
14.080 G 14.190 G 1.703290000000 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 00:45:11.09 +57:46:43.2: 11.40 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:45:11.09 +57:46:43.2: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 45 11.09 +57 46 43.2 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 424722413899081088,2461202.9230,10.78,0.05,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 424722413899081088 20260611.4230 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.73 00:54:31.19 +59:24:00.6
123.32483 -3.46923 galactic Cas Second-epoch detections are separated by 1.3" and 3.2 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 00:54:31.19 +59:24:00.6: 11.83 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:31.19 +59:24:00.6: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 54 31.19 +59 24 00.6 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
V0415 Cas,2461202.9230,10.73,0.05,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
V0415 Cas 20260611.4230 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.41 02:30:17.42 +57:10:05.2
136.05338 -3.16372 galactic Per Second-epoch detections are separated by 1.3" and 3.6 pix
The object was found in VSX 3" ZTF J023017.53+571002.6
Type: SR
# Max. Min./Amp. JD0 Period
15.746 g Y 0.446 g 2458302.47860 111.573594700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:17.42 +57:10:05.2: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:17.42 +57:10:05.2: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 30 17.42 +57 10 05.2 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J023017.53+571002.6,2461202.9230,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J023017.53+571002.6 20260611.4230 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.73 00:44:13.57 +56:48:03.6
121.93929 -6.05685 galactic Cas Second-epoch detections are separated by 2.3" and 3.3 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 00:44:13.57 +56:48:03.6: 11.23 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:13.57 +56:48:03.6: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 44 13.57 +56 48 03.6 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 424525670035286912,2461202.9230,10.73,0.05,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 424525670035286912 20260611.4230 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.55 00:56:47.69 +60:38:48.5
123.58884 -2.21811 galactic Cas Second-epoch detections are separated by 1.4" 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 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 00:56:47.69 +60:38:48.5: 10.71 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:47.69 +60:38:48.5: 13.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 56 47.69 +60 38 48.5 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 426546125736902528,2461202.9230,10.55,0.05,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 426546125736902528 20260611.4230 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 06 11.4230 2461202.9230 10.66 00:55:30.17 +62:23:46.1
123.40279 -0.47189 galactic Cas Second-epoch detections are separated by 1.4" 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 523558751070852096 | 00:55:32.88 +62:23:32.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.541+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:55:30.17 +62:23:46.1: 12.33 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:55:30.17 +62:23:46.1: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 55 30.17 +62 23 46.1 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 523558751070852096,2461202.9230,10.66,0.05,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 523558751070852096 20260611.4230 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 06 11.4230 2461202.9230 10.30 01:40:55.79 +57:55:16.6
129.48490 -4.31940 galactic Cas Second-epoch detections are separated by 4.3" 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 J025.2276+57.9295 | 01:40:55.79 +57:55:16.6 (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 01:40:55.79 +57:55:16.6: 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 01:40:55.79 +57:55:16.6: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 40 55.79 +57 55 16.6 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
ATO J025.2276+57.9295,2461202.9230,10.30,0.05,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
ATO J025.2276+57.9295 20260611.4230 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 06 11.4230 2461202.9230 10.56 01:02:08.11 +60:49:21.2
124.23614 -2.02210 galactic Cas Second-epoch detections are separated by 2.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 426590174917195776 | 01:02:05.27 +60:49:22.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:08.11 +60:49:21.2: 11.74 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:08.11 +60:49:21.2: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 02 08.11 +60 49 21.2 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
Large-amplitude variable Gaia DR2 426590174917195776,2461202.9230,10.56,0.05,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
Large-amplitude variable Gaia DR2 426590174917195776 20260611.4230 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.29 00:52:55.15 +58:28:52.4
123.12608 -4.38997 galactic Cas Second-epoch detections are separated by 2.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.2201+58.4812 | 00:52:55.15 +58:28:52.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.367+/-0.026 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:55.15 +58:28:52.4: 11.30 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:55.15 +58:28:52.4: 12.92 +/- 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 06 11.4230* 00 52 55.15 +58 28 52.4 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
ATO J013.2201+58.4812,2461202.9230,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J013.2201+58.4812 20260611.4230 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.26 01:12:40.87 +61:20:38.1
125.47670 -1.42282 galactic Cas Second-epoch detections are separated by 1.6" 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 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 01:12:40.87 +61:20:38.1: 12.36 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:40.87 +61:20:38.1: 12.71 +/- 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 06 11.4230* 01 12 40.87 +61 20 38.1 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522563173351220736,2461202.9230,10.26,0.05,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 522563173351220736 20260611.4230 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.61 02:07:04.56 +58:31:27.6
132.68655 -2.90758 galactic Per Second-epoch detections are separated by 6.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J031.7888+58.5228 | 02:07:04.66 +58:31:10.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B5 1928AnHar.100...49C HD 236945
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:04.56 +58:31:27.6: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:04.56 +58:31:27.6: 11.31 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.31 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 07 04.56 +58 31 27.6 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J031.7888+58.5228,2461202.9230,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J031.7888+58.5228 20260611.4230 9.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.62 00:36:55.09 +62:40:47.3
121.26679 -0.14499 galactic Cas Second-epoch detections are separated by 2.1" 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 430706329831264640 | 00:36:57.75 +62:40:57.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:55.09 +62:40:47.3: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:36:55.09 +62:40:47.3: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 36 55.09 +62 40 47.3 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430706329831264640,2461202.9230,9.62,0.05,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 430706329831264640 20260611.4230 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 06 11.4230 2461202.9230 8.21 00:52:16.25 +59:42:58.7
123.03708 -3.15527 galactic Cas Second-epoch detections are separated by 1.0" and 3.2 pix
The object was found in VSX18" 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 00:52:16.25 +59:42:58.7: 8.66 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:16.25 +59:42:58.7: 10.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 52 16.25 +59 42 58.7 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 426857150085138176,2461202.9230,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426857150085138176 20260611.4230 8.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.20 00:52:30.72 +59:43:27.2
123.06750 -3.14724 galactic Cas Second-epoch detections are separated by 0.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426857012646129536 | 00:52:31.09 +59:43:23.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A8: 1935BSD...C01....0S BSD 8- 287
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:30.72 +59:43:27.2: 9.57 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:30.72 +59:43:27.2: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 52 30.72 +59 43 27.2 9.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426857012646129536,2461202.9230,9.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426857012646129536 20260611.4230 9.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.31 01:03:22.65 +60:32:13.7
124.40075 -2.30055 galactic Cas Second-epoch detections are separated by 2.1" 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 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 01:03:22.65 +60:32:13.7: 10.90 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:22.65 +60:32:13.7: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 03 22.65 +60 32 13.7 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 426389926362885504,2461202.9230,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426389926362885504 20260611.4230 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.16 01:29:32.92 +61:46:25.9
127.42232 -0.76517 galactic Cas Second-epoch detections are separated by 0.8" 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 | target | 01:29:32.92 +61:46:25.9 (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 01:29:32.92 +61:46:25.9: 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 01:29:32.92 +61:46:25.9: 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 06 11.4230* 01 29 32.92 +61 46 25.9 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,2461202.9230,10.16,0.05,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
target 20260611.4230 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 06 11.4230 2461202.9230 10.18 01:20:56.88 +62:03:30.3
126.38155 -0.61552 galactic Cas Second-epoch detections are separated by 2.3" 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 510938036905942144 | 01:20:56.96 +62:03:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.519+/-0.032 (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 01:20:56.88 +62:03:30.3: 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 01:20:56.88 +62:03:30.3: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 20 56.88 +62 03 30.3 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 510938036905942144,2461202.9230,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510938036905942144 20260611.4230 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.37 00:36:55.70 +62:32:56.0
121.26058 -0.27576 galactic Cas Second-epoch detections are separated by 1.1" 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 430697366244614272 | 00:37:00.66 +62:32:35.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1956PMcCO..13a....B AG+62 73
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:55.70 +62:32:56.0: 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 00:36:55.70 +62:32:56.0: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 36 55.70 +62 32 56.0 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
Gaia DR3 430697366244614272,2461202.9230,10.37,0.05,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
Gaia DR3 430697366244614272 20260611.4230 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 06 11.4230 2461202.9230 10.39 01:03:35.55 +60:28:10.7
124.43037 -2.36674 galactic Cas Second-epoch detections are separated by 2.9" 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 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 01:03:35.55 +60:28:10.7: 11.75 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:35.55 +60:28:10.7: 13.14 +/- 0.04 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 06 11.4230* 01 03 35.55 +60 28 10.7 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 426387242001692800,2461202.9230,10.39,0.05,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 426387242001692800 20260611.4230 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 06 11.4230 2461202.9230 10.44 01:22:23.86 +61:13:51.7
126.64941 -1.41706 galactic Cas Second-epoch detections are separated by 0.4" and 2.9 pix
The object was found in VSX 1" NSVS J0122238+611352
Type: M
# Max. Min./Amp. JD0 Period
14.871 r Y 3.740 r 2458328.87710 325.120339600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:23.86 +61:13:51.7: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:23.86 +61:13:51.7: 15.74 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.74 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 22 23.86 +61 13 51.7 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
NSVS J0122238+611352,2461202.9230,10.44,0.05,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
NSVS J0122238+611352 20260611.4230 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 06 11.4230 2461202.9230 10.45 00:52:12.56 +64:57:22.2
123.01361 2.08454 galactic Cas Second-epoch detections are separated by 1.4" 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 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 00:52:12.56 +64:57:22.2: 12.61 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:12.56 +64:57:22.2: 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 06 11.4230* 00 52 12.56 +64 57 22.2 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
Gaia DR3 524435405436784000,2461202.9230,10.45,0.05,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 524435405436784000 20260611.4230 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 06 11.4230 2461202.9230 10.55 00:45:37.79 +56:46:42.5
122.13194 -6.08425 galactic Cas Second-epoch detections are separated by 1.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:45:37.79 +56:46:42.5 (user input) | T | P | (position from user input) J-Ks=0.721+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:45:37.79 +56:46:42.5: 11.01 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:45:37.79 +56:46:42.5: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 45 37.79 +56 46 42.5 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,2461202.9230,10.55,0.05,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
target 20260611.4230 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 06 11.4230 2461202.9230 10.61 02:10:23.90 +60:01:13.3
132.65115 -1.35295 galactic Cas Second-epoch detections are separated by 1.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:10:23.90 +60:01:13.3 (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 02:10:23.90 +60:01:13.3: 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 02:10:23.90 +60:01:13.3: 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 06 11.4230* 02 10 23.90 +60 01 13.3 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,2461202.9230,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.59 01:59:33.44 +60:01:44.9
131.34867 -1.72474 galactic Cas Second-epoch detections are separated by 0.2" and 3.0 pix
The object was found in VSX17" 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 01:59:33.44 +60:01:44.9: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:33.44 +60:01:44.9: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 59 33.44 +60 01 44.9 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 J015934.53+600159.8,2461202.9230,10.59,0.05,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
ZTF J015934.53+600159.8 20260611.4230 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 06 11.4230 2461202.9230 10.79 01:29:32.90 +63:19:35.9
127.19352 0.77066 galactic Cas Second-epoch detections are separated by 1.5" and 2.5 pix
The object was found in VSX21" Gaia DR3 512422828587465216
Type: S
# Max. Min./Amp. JD0 Period
14.920 G 15.600 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:32.90 +63:19:35.9: 12.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:32.90 +63:19:35.9: 13.47 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 29 32.90 +63 19 35.9 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
Gaia DR3 512422828587465216,2461202.9230,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512422828587465216 20260611.4230 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.55 02:22:13.26 +59:08:19.8
134.35235 -1.70509 galactic Cas Second-epoch detections are separated by 2.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:22:13.26 +59:08:19.8 (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 02:22:13.26 +59:08:19.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:13.26 +59:08:19.8: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 22 13.26 +59 08 19.8 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
target,2461202.9230,10.55,0.05,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
target 20260611.4230 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 06 11.4230 2461202.9230 10.73 00:38:04.03 +62:29:01.6
121.38826 -0.34789 galactic Cas Second-epoch detections are separated by 1.0" 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 430694583105869184 | 00:38:09.59 +62:29:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1966UppAn...5d...1O [O66] 8:1247 J-Ks=12.006+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:38:04.03 +62:29:01.6: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:38:04.03 +62:29:01.6: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 38 04.03 +62 29 01.6 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 430694583105869184,2461202.9230,10.73,0.05,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 430694583105869184 20260611.4230 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.78 01:19:41.77 +62:51:04.8
126.14902 0.15623 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 | target | 01:19:41.77 +62:51:04.8 (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 01:19:41.77 +62:51:04.8: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:41.77 +62:51:04.8: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 19 41.77 +62 51 04.8 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,2461202.9230,10.78,0.05,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
target 20260611.4230 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.73 01:18:36.92 +58:41:37.9
126.46487 -3.99133 galactic Cas Second-epoch detections are separated by 1.7" and 3.3 pix
The object was found in VSX22" 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 01:18:36.92 +58:41:37.9: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:36.92 +58:41:37.9: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 18 36.92 +58 41 37.9 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
Gaia DR3 413902596701682816,2461202.9230,10.73,0.05,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 413902596701682816 20260611.4230 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.81 01:03:24.22 +61:12:24.3
124.37283 -1.63152 galactic Cas Second-epoch detections are separated by 1.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:03:24.22 +61:12:24.3 (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 01:03:24.22 +61:12:24.3: 10.94 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:24.22 +61:12:24.3: 13.57 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 03 24.22 +61 12 24.3 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,2461202.9230,10.81,0.05,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 20260611.4230 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 06 11.4230 2461202.9230 10.78 02:02:54.01 +60:15:41.7
131.68766 -1.38968 galactic Cas Second-epoch detections are separated by 0.9" 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 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 02:02:54.01 +60:15:41.7: 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 02:02:54.01 +60:15:41.7: 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 06 11.4230* 02 02 54.01 +60 15 41.7 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 507950977353541248,2461202.9230,10.78,0.05,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 507950977353541248 20260611.4230 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.88 01:18:48.42 +64:12:22.2
125.90449 1.49250 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 | target | 01:18:48.42 +64:12:22.2 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.42 +64:12:22.2: 11.69 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.42 +64:12:22.2: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 18 48.42 +64 12 22.2 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,2461202.9230,10.88,0.05,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 20260611.4230 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 06 11.4230 2461202.9230 10.72 02:19:57.66 +59:32:25.7
133.94485 -1.42511 galactic Cas Second-epoch detections are separated by 3.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.9820+59.5389 | 02:19:57.66 +59:32:25.7 (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 02:19:57.66 +59:32:25.7: 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 02:19:57.66 +59:32:25.7: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 19 57.66 +59 32 25.7 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
ATO J034.9820+59.5389,2461202.9230,10.72,0.05,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
ATO J034.9820+59.5389 20260611.4230 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.89 01:34:42.46 +58:42:14.7
128.53838 -3.69586 galactic Cas Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:34:42.46 +58:42:14.7 (user input) | T | P | (position from user input) J-Ks=0.903+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:42.46 +58:42:14.7: 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 01:34:42.46 +58:42:14.7: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 34 42.46 +58 42 14.7 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
target,2461202.9230,10.89,0.05,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
target 20260611.4230 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.88 00:54:25.57 +60:12:30.4
123.30349 -2.66115 galactic Cas Second-epoch detections are separated by 1.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426149030239670016 | 00:54:21.76 +60:12:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1935BSD...C01....0S BSD 8- 343 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 00:54:25.57 +60:12:30.4: 11.38 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:25.57 +60:12:30.4: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 54 25.57 +60 12 30.4 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
Gaia DR3 426149030239670016,2461202.9230,10.88,0.05,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 426149030239670016 20260611.4230 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 06 11.4230 2461202.9230 10.83 01:09:51.36 +57:04:44.5
125.44494 -5.70282 galactic Cas Second-epoch detections are separated by 1.9" and 3.0 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 01:09:51.36 +57:04:44.5: 11.15 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:51.36 +57:04:44.5: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 09 51.36 +57 04 44.5 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 413511484103439360,2461202.9230,10.83,0.05,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
Gaia DR3 413511484103439360 20260611.4230 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.82 01:38:08.14 +61:01:39.6
128.55838 -1.33292 galactic Cas Second-epoch detections are separated by 2.8" 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 | 01:38:08.14 +61:01:39.6 (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 01:38:08.14 +61:01:39.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:08.14 +61:01:39.6: 13.65 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 38 08.14 +61 01 39.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.82,0.05,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
target 20260611.4230 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 06 11.4230 2461202.9230 10.86 02:00:32.97 +59:40:07.0
131.56369 -2.03989 galactic Cas Second-epoch detections are separated by 2.4" and 2.9 pix
The object was found in VSX 2" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.97 +59:40:07.0: 11.61 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.97 +59:40:07.0: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 00 32.97 +59 40 07.0 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
ZTF J020033.07+594008.7,2461202.9230,10.86,0.05,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
ZTF J020033.07+594008.7 20260611.4230 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.85 02:02:50.62 +60:13:57.8
131.68880 -1.41936 galactic Cas Second-epoch detections are separated by 1.2" and 2.8 pix
The object was found in VSX21" Gaia DR3 507950766893076736
Type: E
# Max. Min./Amp. JD0 Period
18.720 G 19.250 G 0.254094000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:50.62 +60:13:57.8: 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 02:02:50.62 +60:13:57.8: 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 06 11.4230* 02 02 50.62 +60 13 57.8 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 507950766893076736,2461202.9230,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507950766893076736 20260611.4230 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.95 01:29:49.78 +58:44:46.4
127.90526 -3.75431 galactic Cas Second-epoch detections are separated by 3.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J022.4742+58.7371 | 01:29:49.78 +58:44:46.4 (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 01:29:49.78 +58:44:46.4: 12.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:49.78 +58:44:46.4: 13.83 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 29 49.78 +58 44 46.4 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 J022.4742+58.7371,2461202.9230,10.95,0.05,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
ATO J022.4742+58.7371 20260611.4230 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.94 01:43:03.65 +58:57:14.1
129.55701 -3.25220 galactic Cas Second-epoch detections are separated by 1.1" 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 | ATO J025.7767+58.9545 | 01:43:03.65 +58:57:14.1 (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 01:43:03.65 +58:57:14.1: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:03.65 +58:57:14.1: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 43 03.65 +58 57 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
ATO J025.7767+58.9545,2461202.9230,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7767+58.9545 20260611.4230 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.88 01:51:09.55 +64:52:45.9
129.21849 2.73913 galactic Cas Second-epoch detections are separated by 2.3" and 2.7 pix
The object was found in VSX 3" Gaia DR3 518229967963921664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.55 +64:52:45.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.55 +64:52:45.9: 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 06 11.4230* 01 51 09.55 +64 52 45.9 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 518229967963921664,2461202.9230,10.88,0.05,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 518229967963921664 20260611.4230 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 06 11.4230 2461202.9230 10.98 02:02:24.51 +64:38:24.6
130.44072 2.80809 galactic Cas Second-epoch detections are separated by 1.5" and 2.3 pix
The object was found in VSX 9" ASASSN-V J020225.96+643822.9
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.200 V 2457555.11300 70.630000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:24.51 +64:38:24.6: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:24.51 +64:38:24.6: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 02 24.51 +64 38 24.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020225.96+643822.9,2461202.9230,10.98,0.05,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
ASASSN-V J020225.96+643822.9 20260611.4230 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.16 00:44:39.75 +62:06:29.5
122.13955 -0.75313 galactic Cas Second-epoch detections are separated by 5.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:44:39.75 +62:06:29.5 (user input) | T | P | (position from user input) J-Ks=0.450+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:44:39.75 +62:06:29.5: 12.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:39.75 +62:06:29.5: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 44 39.75 +62 06 29.5 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,2461202.9230,11.16,0.05,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
target 20260611.4230 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.00 01:14:21.78 +59:59:49.2
125.79752 -2.74713 galactic Cas Second-epoch detections are separated by 3.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:14:21.78 +59:59:49.2 (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 01:14:21.78 +59:59:49.2: 12.20 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:21.78 +59:59:49.2: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 14 21.78 +59 59 49.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.00,0.05,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 20260611.4230 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.03 00:50:25.40 +60:08:08.8
122.80547 -2.73572 galactic Cas Second-epoch detections are separated by 2.7" 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 | 00:50:25.40 +60:08:08.8 (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 00:50:25.40 +60:08:08.8: 11.80 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:50:25.40 +60:08:08.8: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 50 25.40 +60 08 08.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.03,0.05,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 20260611.4230 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.07 01:23:46.01 +60:53:25.2
126.85562 -1.73489 galactic Cas Second-epoch detections are separated by 0.2" 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 | 01:23:46.01 +60:53:25.2 (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 01:23:46.01 +60:53:25.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:46.01 +60:53:25.2: 14.11 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 23 46.01 +60 53 25.2 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,2461202.9230,11.07,0.05,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 20260611.4230 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.12 01:11:56.69 +58:41:05.6
125.60068 -4.08056 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 J017.9933+58.6776 | 01:11:56.69 +58:41:05.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.669+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:56.69 +58:41:05.6: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:56.69 +58:41:05.6: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 11 56.69 +58 41 05.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.9933+58.6776,2461202.9230,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.9933+58.6776 20260611.4230 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.11 01:31:48.55 +64:22:28.2
127.28081 1.84417 galactic Cas Second-epoch detections are separated by 1.7" 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 | target | 01:31:48.55 +64:22:28.2 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.55 +64:22:28.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.55 +64:22:28.2: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 31 48.55 +64 22 28.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.11,0.05,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
target 20260611.4230 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.09 01:25:19.00 +62:14:40.2
126.86507 -0.36825 galactic Cas Second-epoch detections are separated by 4.0" 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 | ASASSN-V J012524.70+621420.4 | 01:25:24.69 +62:14:20.3 (Gaia DR3) | L: (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:19.00 +62:14:40.2: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:19.00 +62:14:40.2: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 25 19.00 +62 14 40.2 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
ASASSN-V J012524.70+621420.4,2461202.9230,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J012524.70+621420.4 20260611.4230 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.11 01:05:51.59 +60:27:36.2
124.71015 -2.36189 galactic Cas Second-epoch detections are separated by 1.3" and 3.2 pix
The object was found in VSX 3" Gaia DR3 426379206124772608
Type: RS
# Max. Min./Amp. JD0 Period
13.760 G 13.830 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 01:05:51.59 +60:27:36.2: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:51.59 +60:27:36.2: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 05 51.59 +60 27 36.2 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
Gaia DR3 426379206124772608,2461202.9230,11.11,0.05,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 426379206124772608 20260611.4230 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.06 01:02:13.99 +59:56:04.8
124.28536 -2.90871 galactic Cas Second-epoch detections are separated by 2.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | V1062 Cas | 01:02:09.15 +59:55:43.1 (Gaia DR3) | EB (local) | 1.164421000000 (local) | Gaia3var=VARIABLE SpType: F4 1935BSD...C01....0S BSD 8- 466 J-Ks=0.497+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:13.99 +59:56:04.8: 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 01:02:13.99 +59:56:04.8: 13.90 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 02 13.99 +59 56 04.8 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
V1062 Cas,2461202.9230,11.06,0.05,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
V1062 Cas 20260611.4230 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.99 01:55:53.02 +64:15:25.6
129.86002 2.25569 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 | target | 01:55:53.02 +64:15:25.6 (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 01:55:53.02 +64:15:25.6: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:53.02 +64:15:25.6: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 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 06 11.4230* 01 55 53.02 +64 15 25.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.99,0.05,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
target 20260611.4230 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.96 02:39:11.03 +63:43:56.9
134.51667 3.31089 galactic Cas Second-epoch detections are separated by 3.6" 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 | target | 02:39:11.03 +63:43:56.9 (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 02:39:11.03 +63:43:56.9: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:39:11.03 +63:43:56.9: 13.70 +/- 0.05 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 06 11.4230* 02 39 11.03 +63 43 56.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.96,0.05,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
target 20260611.4230 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.13 02:01:21.95 +66:30:18.0
129.83240 4.57465 galactic Cas Second-epoch detections are separated by 3.8" 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 | 02:01:21.95 +66:30:18.0 (user input) | T | P | (position from user input) J-Ks=0.990+/-0.036 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:21.95 +66:30:18.0: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:21.95 +66:30:18.0: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 01 21.95 +66 30 18.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.13,0.05,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
target 20260611.4230 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.41 01:20:34.92 +64:02:26.7
126.11517 1.34928 galactic Cas Second-epoch detections are separated by 1.5" 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 | 01:20:34.92 +64:02:26.7 (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 01:20:34.92 +64:02:26.7: 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 01:20:34.92 +64:02:26.7: 14.17 +/- 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 06 11.4230* 01 20 34.92 +64 02 26.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.28 01:06:55.38 +59:18:56.7
124.91002 -3.49651 galactic Cas Second-epoch detections are separated by 5.5" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.38 +59:18:56.7 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.38 +59:18:56.7: 13.05 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.38 +59:18:56.7: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 06 55.38 +59 18 56.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.52 01:08:11.42 +62:14:22.3
124.88137 -0.56879 galactic Cas Second-epoch detections are separated by 2.7" and 2.7 pix
The object was found in VSX 3" Gaia DR3 522685876279259136
Type: ROT
# Max. Min./Amp. JD0 Period
14.350 G 14.370 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:11.42 +62:14:22.3: 12.14 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:11.42 +62:14:22.3: 14.15 +/- 0.07 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 06 11.4230* 01 08 11.42 +62 14 22.3 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 522685876279259136,2461202.9230,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522685876279259136 20260611.4230 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.78 01:07:44.51 +59:03:02.7
125.03131 -3.75452 galactic Cas Second-epoch detections are separated by 1.8" and 3.4 pix
The object was found in VSX 1" V0890 Cas
Type: M
# Max. Min./Amp. JD0 Period
10.400 I 15.700 I 2440228.00000 493.000000000000 S?,6e
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:44.51 +59:03:02.7: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:44.51 +59:03:02.7: 16.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 07 44.51 +59 03 02.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0890 Cas,2461202.9230,11.78,0.05,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
V0890 Cas 20260611.4230 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 11.98 01:17:07.44 +62:50:32.4
125.85811 0.11661 galactic Cas Second-epoch detections are separated by 0.6" and 2.6 pix
The object was found in VSX 1" Gaia DR3 523123275743387904
Type: L
# Max. Min./Amp. JD0 Period
13.580 G 13.720 G C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:07.44 +62:50:32.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:07.44 +62:50:32.4: 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 06 11.4230* 01 17 07.44 +62 50 32.4 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523123275743387904,2461202.9230,11.98,0.05,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 523123275743387904 20260611.4230 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.80 01:58:48.47 +62:43:32.2
130.56274 0.85624 galactic Cas Second-epoch detections are separated by 0.6" and 2.7 pix
The object was found in VSX 5" NSVS 1820604
Type: SR
# Max. Min./Amp. JD0 Period
13.494 r Y 0.450 R1 2458369.29680 125.813204600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:48.47 +62:43:32.2: 13.41 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:48.47 +62:43:32.2: 14.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 58 48.47 +62 43 32.2 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
NSVS 1820604,2461202.9230,10.80,0.05,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
NSVS 1820604 20260611.4230 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 06 11.4230 2461202.9230 10.45 02:47:29.79 +65:31:27.8
134.57523 5.31076 galactic Cas Second-epoch detections are separated by 0.1" 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 | 02:47:29.79 +65:31:27.8 (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 02:47:29.79 +65:31:27.8: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:47:29.79 +65:31:27.8: 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 06 11.4230* 02 47 29.79 +65 31 27.8 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,2461202.9230,10.45,0.05,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
target 20260611.4230 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 06 11.4230 2461202.9230 10.21 02:26:23.38 +56:29:19.8
135.80488 -3.99110 galactic Per Second-epoch detections are separated by 1.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:26:23.38 +56:29:19.8 (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 02:26:23.38 +56:29:19.8: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:23.38 +56:29:19.8: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 26 23.38 +56 29 19.8 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.21,0.05,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 20260611.4230 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 06 11.4230 2461202.9230 10.13 02:44:05.83 +62:19:56.7
135.60246 2.26489 galactic Cas Second-epoch detections are separated by 1.2" 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 | 02:44:05.83 +62:19:56.7 (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 02:44:05.83 +62:19:56.7: 10.73 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:44:05.83 +62:19:56.7: 13.02 +/- 0.03 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 06 11.4230* 02 44 05.83 +62 19 56.7 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.13,0.05,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
target 20260611.4230 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.98 01:41:47.05 +59:03:48.5
129.37405 -3.17711 galactic Cas Second-epoch detections are separated by 0.8" and 3.2 pix
The object was found in VSX 2" ASASSN-V J014146.93+590346.7
Type: SR
# Max. Min./Amp. JD0 Period
13.670 V 14.220 V 2457304.00000 93.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:47.05 +59:03:48.5: 11.53 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:47.05 +59:03:48.5: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 41 47.05 +59 03 48.5 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014146.93+590346.7,2461202.9230,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J014146.93+590346.7 20260611.4230 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 06 11.4230 2461202.9230 10.95 02:10:17.83 +60:58:59.7
132.34993 -0.43830 galactic Cas Second-epoch detections are separated by 1.4" and 3.1 pix
The object was found in VSX 2" NSVS J0210179+605902
Type: SR
# Max. Min./Amp. JD0 Period
14.153 r Y 0.631 r 2458450.25450 296.241215300000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:17.83 +60:58:59.7: 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 02:10:17.83 +60:58:59.7: 14.73 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.73 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 10 17.83 +60 58 59.7 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
NSVS J0210179+605902,2461202.9230,10.95,0.05,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
NSVS J0210179+605902 20260611.4230 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.36 01:21:54.89 +61:20:56.5
126.57778 -1.30679 galactic Cas Second-epoch detections are separated by 0.1" and 2.9 pix
The object was found in ASASSN-V 2" ASASSN-V J012154.67+612055.1
Type: SR
MeanMag 14.81 m Amp. 2.24 m Period 397.1456143 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:54.89 +61:20:56.5: 13.29 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:54.89 +61:20:56.5: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 21 54.89 +61 20 56.5 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461202.9230,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260611.4230 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.70 02:48:41.14 +63:58:46.1
135.36424 3.97494 galactic Cas Second-epoch detections are separated by 1.6" 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 | 02:48:41.14 +63:58:46.1 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:48:41.14 +63:58:46.1: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:48:41.14 +63:58:46.1: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 48 41.14 +63 58 46.1 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
target,2461202.9230,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 8.34 02:24:29.80 +59:24:31.9
134.53111 -1.35087 galactic Cas Second-epoch detections are separated by 0.4" and 3.2 pix
The object was found in VSX 1" V0672 Cas
Type: SR
# Max. Min./Amp. JD0 Period
15.000 B 17.400 B 302.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:29.80 +59:24:31.9: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:29.80 +59:24:31.9: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 24 29.80 +59 24 31.9 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
V0672 Cas,2461202.9230,8.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0672 Cas 20260611.4230 8.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.53 01:33:46.78 +58:39:46.2
128.42606 -3.75651 galactic Cas Second-epoch detections are separated by 1.1" and 3.3 pix
The object was found in VSX24" Gaia DR3 509038428716371072
Type: ROT
# Max. Min./Amp. JD0 Period
18.180 G 18.290 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 01:33:46.78 +58:39:46.2: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:46.78 +58:39:46.2: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 33 46.78 +58 39 46.2 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509038428716371072,2461202.9230,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509038428716371072 20260611.4230 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.64 01:32:51.46 +62:40:37.1
127.66448 0.18643 galactic Cas Second-epoch detections are separated by 1.1" and 2.9 pix
The object was found in VSX 2" ASASSN-V J013251.56+624035.5
Type: SR
# Max. Min./Amp. JD0 Period
14.830 V 15.470 V 2458353.38020 131.762706400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:51.46 +62:40:37.1: 13.05 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:51.46 +62:40:37.1: 14.33 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 32 51.46 +62 40 37.1 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
ASASSN-V J013251.56+624035.5,2461202.9230,10.64,0.05,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
ASASSN-V J013251.56+624035.5 20260611.4230 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 06 11.4230 2461202.9230 9.55 01:45:35.83 +63:07:08.5
129.00909 0.88809 galactic Cas Second-epoch detections are separated by 0.6" and 2.8 pix
The object was found in VSX 6" ASASSN-V J014535.87+630702.7
Type: SR
# Max. Min./Amp. JD0 Period
13.890 V 15.100 V 2457012.80000 462.000000000000
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 01:45:35.83 +63:07:08.5: 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 01:45:35.83 +63:07:08.5: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 45 35.83 +63 07 08.5 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014535.87+630702.7,2461202.9230,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J014535.87+630702.7 20260611.4230 9.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.21 02:34:46.49 +56:12:07.0
136.99231 -3.82270 galactic Per Second-epoch detections are separated by 2.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:34:46.49 +56:12:07.0 (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 02:34:46.49 +56:12:07.0: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:46.49 +56:12:07.0: 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 06 11.4230* 02 34 46.49 +56 12 07.0 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.21,0.05,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 20260611.4230 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 06 11.4230 2461202.9230 8.80 02:19:16.61 +59:42:22.6
133.80789 -1.29774 galactic Cas Second-epoch detections are separated by 0.3" and 3.1 pix
The object was found in VSX 2" ZTF J021916.76+594221.6
Type: SR
# Max. Min./Amp. JD0 Period
14.063 g Y 0.424 g 2458349.86040 72.477681200000 MS
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:16.61 +59:42:22.6: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:16.61 +59:42:22.6: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 19 16.61 +59 42 22.6 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J021916.76+594221.6,2461202.9230,8.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J021916.76+594221.6 20260611.4230 8.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.13 01:39:32.59 +64:53:04.2
128.01045 2.48815 galactic Cas Second-epoch detections are separated by 0.9" and 2.5 pix
The object was found in VSX 2" ASASSN-V J013932.54+645302.3
Type: YSO
# Max. Min./Amp. JD0 Period
12.800 g 16.100 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 01:39:32.59 +64:53:04.2: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:32.59 +64:53:04.2: 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 06 11.4230* 01 39 32.59 +64 53 04.2 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
ASASSN-V J013932.54+645302.3,2461202.9230,10.13,0.05,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
ASASSN-V J013932.54+645302.3 20260611.4230 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.52 02:07:46.81 +62:11:12.5
131.70808 0.62293 galactic Cas Second-epoch detections are separated by 1.8" and 3.1 pix
The object was found in ASASSN-V 0" ASASSN-V J020746.87+621112.3
Type: SR
MeanMag 15.53 m Amp. 1.57 m Period 397.2118966 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:46.81 +62:11:12.5: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:46.81 +62:11:12.5: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 07 46.81 +62 11 12.5 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
VARIABLE_NAME,2461202.9230,10.52,0.05,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
VARIABLE_NAME 20260611.4230 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.40 02:06:50.44 +63:27:21.8
131.23801 1.80685 galactic Cas Second-epoch detections are separated by 1.5" and 2.9 pix
The object was found in VSX13" Gaia DR3 514874361558005760
Type: ROT
# Max. Min./Amp. JD0 Period
15.770 G 15.800 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 02:06:50.44 +63:27:21.8: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:06:50.44 +63:27:21.8: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 06 50.44 +63 27 21.8 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
Gaia DR3 514874361558005760,2461202.9230,10.40,0.05,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 514874361558005760 20260611.4230 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 06 11.4230 2461202.9230 10.61 02:27:17.51 +56:07:13.9
136.05512 -4.28945 galactic Per Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:27:17.51 +56:07:13.9 (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 02:27:17.51 +56:07:13.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:17.51 +56:07:13.9: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 27 17.51 +56 07 13.9 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,2461202.9230,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.86 02:15:26.79 +62:47:46.4
132.36528 1.47329 galactic Cas Second-epoch detections are separated by 0.2" and 2.8 pix
The object was found in VSX 1" ASASSN-V J021526.89+624746.2
Type: SR
# Max. Min./Amp. JD0 Period
14.070 V 14.780 V 2458439.05750 300.903027600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:26.79 +62:47:46.4: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:26.79 +62:47:46.4: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 15 26.79 +62 47 46.4 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J021526.89+624746.2,2461202.9230,9.86,0.05,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
ASASSN-V J021526.89+624746.2 20260611.4230 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 06 11.4230 2461202.9230 10.29 02:48:49.50 +61:53:28.2
136.29155 2.10308 galactic Cas Second-epoch detections are separated by 1.0" 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 | ZTF J024848.61+615302.4 | 02:48:49.52 +61:53:26.4 (Gaia DR3) | RS (local) | 2458376.93210 (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.492+/-0.034 (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 02:48:49.50 +61:53:28.2: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:48:49.50 +61:53:28.2: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 48 49.50 +61 53 28.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J024848.61+615302.4,2461202.9230,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J024848.61+615302.4 20260611.4230 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.15 01:32:28.17 +61:03:28.1
127.87717 -1.41936 galactic Cas Second-epoch detections are separated by 0.6" 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 509890859471064960 | 01:32:26.28 +61:04:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:28.17 +61:03:28.1: 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 01:32:28.17 +61:03:28.1: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 32 28.17 +61 03 28.1 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
Gaia DR3 509890859471064960,2461202.9230,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509890859471064960 20260611.4230 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.87 02:35:19.15 +56:39:41.2
136.88240 -3.37018 galactic Per Second-epoch detections are separated by 3.0" and 3.7 pix
The object was found in VSX 7" NSVS 1919841
Type: SR
# Max. Min./Amp. JD0 Period
13.201 r Y 0.986 r 2451450.11000 262.553069500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:19.15 +56:39:41.2: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:19.15 +56:39:41.2: 14.94 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 35 19.15 +56 39 41.2 10.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1919841,2461202.9230,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1919841 20260611.4230 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.91 02:18:24.74 +58:37:27.8
134.06207 -2.35519 galactic Per Second-epoch detections are separated by 0.5" and 3.3 pix
The object was found in VSX 2" TSVSC1 TN-N311132011-556-86-2
Type: SR
# Max. Min./Amp. JD0 Period
13.035 r Y 0.802 r 2458469.04980 210.487596000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:24.74 +58:37:27.8: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:24.74 +58:37:27.8: 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 06 11.4230* 02 18 24.74 +58 37 27.8 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TSVSC1 TN-N311132011-556-86-2,2461202.9230,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N311132011-556-86-2 20260611.4230 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.33 00:44:01.60 +58:23:35.1
121.95805 -4.46465 galactic Cas Second-epoch detections are separated by 1.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:44:01.60 +58:23:35.1 (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 00:44:01.60 +58:23:35.1: 11.00 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:01.60 +58:23:35.1: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 44 01.60 +58 23 35.1 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461202.9230,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.01 01:20:18.28 +64:28:06.2
126.03716 1.77082 galactic Cas Second-epoch detections are separated by 0.8" and 2.7 pix
The object was found in VSX 1" V0898 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
12.800 V 13.800 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:18.28 +64:28:06.2: 10.35 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:18.28 +64:28:06.2: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 20 18.28 +64 28 06.2 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0898 Cas,2461202.9230,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0898 Cas 20260611.4230 9.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.49 01:22:27.49 +65:23:26.6
126.15681 2.71339 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 | 01:22:27.49 +65:23:26.6 (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 01:22:27.49 +65:23:26.6: 11.37 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:27.49 +65:23:26.6: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 22 27.49 +65 23 26.6 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,2461202.9230,10.49,0.05,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 20260611.4230 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 06 11.4230 2461202.9230 10.68 02:46:03.81 +63:32:43.4
135.29033 3.45825 galactic Cas Second-epoch detections are separated by 0.8" 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 | 02:46:03.81 +63:32:43.4 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.026 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:46:03.81 +63:32:43.4: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:46:03.81 +63:32:43.4: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 46 03.81 +63 32 43.4 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,2461202.9230,10.68,0.05,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
target 20260611.4230 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 06 11.4230 2461202.9230 9.93 01:49:47.63 +65:03:22.0
129.03750 2.87842 galactic Cas Second-epoch detections are separated by 0.3" and 2.6 pix
The object was found in VSX 1" ASASSN-V J014947.64+650321.4
Type: SR
# Max. Min./Amp. JD0 Period
14.000 V 15.100 V 2458390.66790 121.379022800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:47.63 +65:03:22.0: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:47.63 +65:03:22.0: 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 06 11.4230* 01 49 47.63 +65 03 22.0 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014947.64+650321.4,2461202.9230,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J014947.64+650321.4 20260611.4230 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.32 02:09:55.23 +56:59:24.0
133.50219 -4.26235 galactic Per Second-epoch detections are separated by 1.0" and 3.4 pix
The object was found in VSX 3" ASASSN-V J020955.15+565920.6
Type: SR
# Max. Min./Amp. JD0 Period
14.620 V 15.150 V 2458358.04680 150.234053800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:55.23 +56:59:24.0: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:55.23 +56:59:24.0: 14.32 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 09 55.23 +56 59 24.0 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020955.15+565920.6,2461202.9230,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J020955.15+565920.6 20260611.4230 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.92 00:42:54.80 +62:48:25.7
121.95819 -0.04849 galactic Cas Second-epoch detections are separated by 2.0" and 3.1 pix
The object was found in VSX 9" Gaia DR3 427808296361981312
Type: ROT
# Max. Min./Amp. JD0 Period
14.770 G 14.820 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 00:42:54.80 +62:48:25.7: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:42:54.80 +62:48:25.7: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 00 42 54.80 +62 48 25.7 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 427808296361981312,2461202.9230,10.92,0.05,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
Gaia DR3 427808296361981312 20260611.4230 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 06 11.4230 2461202.9230 10.05 01:09:37.99 +59:05:15.2
125.27184 -3.70150 galactic Cas Second-epoch detections are separated by 2.7" and 3.5 pix
The object was found in VSX 2" NSVS 1731355
Type: SR
# Max. Min./Amp. JD0 Period
13.050 r Y 0.760 r 2458523.08150 271.469883000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:37.99 +59:05:15.2: 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 01:09:37.99 +59:05:15.2: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 09 37.99 +59 05 15.2 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1731355,2461202.9230,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1731355 20260611.4230 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.49 01:33:44.42 +60:46:19.9
128.07564 -1.67638 galactic Cas Second-epoch detections are separated by 2.6" 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 | target | 01:33:44.42 +60:46:19.9 (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 01:33:44.42 +60:46:19.9: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.42 +60:46:19.9: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 06 11.4230* 01 33 44.42 +60 46 19.9 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
target,2461202.9230,10.49,0.05,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 20260611.4230 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 06 11.4230 2461202.9230 8.58 02:33:23.74 +64:25:00.4
133.66409 3.69069 galactic Cas Second-epoch detections are separated by 0.7" and 2.8 pix
The object was found in VSX 2" V0940 Cas
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 14.100 V 2458188.78170 420.688461000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:23.74 +64:25:00.4: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:23.74 +64:25:00.4: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 33 23.74 +64 25 00.4 8.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0940 Cas,2461202.9230,8.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0940 Cas 20260611.4230 8.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.32 02:03:07.39 +57:18:15.1
132.52629 -4.22614 galactic Per Second-epoch detections are separated by 0.5" and 3.4 pix
The object was found in VSX 2" ASASSN-V J020307.46+571813.2
Type: SR
# Max. Min./Amp. JD0 Period
13.470 V 13.900 V 2458312.63550 148.824620900000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:07.39 +57:18:15.1: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:07.39 +57:18:15.1: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 03 07.39 +57 18 15.1 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J020307.46+571813.2,2461202.9230,9.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J020307.46+571813.2 20260611.4230 9.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.61 02:48:30.05 +61:37:04.3
136.37621 1.84039 galactic Cas Second-epoch detections are separated by 2.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:48:30.05 +61:37:04.3 (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 02:48:30.05 +61:37:04.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:48:30.05 +61:37:04.3: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 48 30.05 +61 37 04.3 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,2461202.9230,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260611.4230 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.06 02:13:47.76 +63:11:27.0
132.06266 1.78844 galactic Cas Second-epoch detections are separated by 1.2" and 2.9 pix
The object was found in VSX 0" NSVS J0213478+631127
Type: L:
# Max. Min./Amp. JD0 Period
11.122 R1 Y 0.644 R1 355.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.76 +63:11:27.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.76 +63:11:27.0: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 13 47.76 +63 11 27.0 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0213478+631127,2461202.9230,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0213478+631127 20260611.4230 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.85 02:49:57.11 +63:51:37.9
135.54191 3.92914 galactic Cas Second-epoch detections are separated by 1.1" 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 467697169465689088 | 02:49:53.99 +63:51:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:49:57.11 +63:51:37.9: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:49:57.11 +63:51:37.9: 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 06 11.4230* 02 49 57.11 +63 51 37.9 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 467697169465689088,2461202.9230,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 467697169465689088 20260611.4230 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 10.02 02:40:38.88 +60:07:58.7
136.13611 0.09120 galactic Cas Second-epoch detections are separated by 1.0" and 3.2 pix
The object was found in VSX 7" NSVS J0240393+600752
Type: L:
# Max. Min./Amp. JD0 Period
11.294 R1 Y 0.308 R1 730.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:40:38.88 +60:07:58.7: 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 02:40:38.88 +60:07:58.7: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 40 38.88 +60 07 58.7 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
NSVS J0240393+600752,2461202.9230,10.02,0.05,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
NSVS J0240393+600752 20260611.4230 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.40 02:18:22.64 +58:47:11.0
134.00429 -2.20376 galactic Per Second-epoch detections are separated by 0.1" and 3.2 pix
The object was found in VSX 3" NSVS J0218236+584716
Type: SR
# Max. Min./Amp. JD0 Period
12.694 r Y 0.560 r 2458351.79460 241.646383300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:22.64 +58:47:11.0: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:22.64 +58:47:11.0: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 02 18 22.64 +58 47 11.0 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0218236+584716,2461202.9230,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0218236+584716 20260611.4230 9.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 11.4230 2461202.9230 9.47 01:35:09.77 +60:17:10.9
128.32903 -2.12639 galactic Cas Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX 1" Mis V0883
Type: L:
# Max. Min./Amp. JD0 Period
10.600 CR 11.500 CR 188.000000000000 S
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:09.77 +60:17:10.9: 13.11 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:09.77 +60:17:10.9: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 11.4230* 01 35 09.77 +60 17 10.9 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0883,2461202.9230,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0883 20260611.4230 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461202.92320050 11.06.2026 10:09:14.523 /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 21
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: 11 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): 29903
Objects passed selection criteria: 29851
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 26782.8
Average stars matched: 26117.2 (97.5152 %)
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 Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 11 06:00:46 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: 2461202.92320050 11.06.2026 10:09:14.523 /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 340
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: 123 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): 202959
Objects passed selection criteria: 202518
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 168727
Average stars matched: 163481 (96.891 %)
Memory usage VmPeak: 1957324 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 11 06:08:33 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_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.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_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.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: 2461202.92271319
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_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits'
wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.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_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
Image size: 941.3'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 01:42:28.986 +62:00:27.08 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 01:42:28.986 +62:00:27.08
Angular distance between the image centers 0.0224 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
Image size: 941.3'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 01:42:26.524 +62:00:26.85 J2000 4789.000 3195.000
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# 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 01:42:26.524 +62:00:26.85
Angular distance between the image centers 0.0227 deg.
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# 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 01:42:28.986 +62:00:27.08
Second-epoch second image center 01:42:26.524 +62:00:26.85
Angular distance between the image centers 0.00481 deg.
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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.gqEdTPWdEn
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.8JX8oPpSBb
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_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits &> /tmp/tmp.FdwVy5Mai3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits &> /tmp/tmp.r8R4H5oISr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.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.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-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.wcscat
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.wcscat
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.wcscat) found
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.937800
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 20 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
3.6 pix fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
3.6 pix fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.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
14.5 mag. fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
14.5 mag. fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gqEdTPWdEn (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_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/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.wcscat 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.wcscat 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.wcscat
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.wcscat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 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.wcscat.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.wcscat.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.wcscat.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.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8JX8oPpSBb (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_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/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.wcscat 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.wcscat 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.wcscat
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.wcscat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 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.wcscat.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.wcscat.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.wcscat.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.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FdwVy5Mai3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.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_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1524, passed=22482
Got 22482 stars (including 20944 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat
util/solve_plate_with_UCAC5 got 22482 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 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: 970 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: 970 matched stars entering correct_measured_positions(), 21819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 21822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 21822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 969 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits N_match=969 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.365 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.396 n_q1=268 n_q2=350 n_q3=202 n_q4=149 worst_quadrant_to_overall_ratio=1.053
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits -region wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.r8R4H5oISr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.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_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat
SExtractor catalog parsing summary: zero_flux=7, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1483, passed=22053
Got 22053 stars (including 20557 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat
util/solve_plate_with_UCAC5 got 22053 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 21427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 21425 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 21415 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 970 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits N_match=970 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.456 n_q1=266 n_q2=343 n_q3=207 n_q4=154 worst_quadrant_to_overall_ratio=1.099
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits -region wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-03-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_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits sigma_overall=0.376 worst_q_ratio=1.053
new2=fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits sigma_overall=0.415 worst_q_ratio=1.099
reference average sigma_overall=3.8485 worst_q_ratio=2.561
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: 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.wcscat.astrometric_residuals, image 9576x6388, median residual 3.06 arcsec)
plot_astrometric_residuals_xy.py: 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.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458_astrometric_residuals.png (969 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459_astrometric_residuals.png (970 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-08-32_20.00sec_-0.00C_LIGHTs_0458.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-11_CI_Cas-03-Q1b1x1_055240_TTUQ1b1x1_3244969_qsBVIoa7/wcs_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459.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 01:21:54.76 +61:20:56.5: 15.72 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:46:24.81 +64:19:53.2: 15.69 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:07.38 +57:18:15.4: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:18.26 +64:28:06.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:54.76 +61:20:56.5: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.06
Forced photometry filter KEPT candidate at 01:21:54.76 +61:20:56.5: ref_mag=14.12 +/- 0.06 new_mean_mag=11.9014 delta=2.22 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:09.74 +60:17:11.0: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:07.38 +57:18:15.4: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 02:03:07.38 +57:18:15.4: ref_mag=12.82 +/- 0.02 new_mean_mag=11.9577 delta=0.86 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:46:24.81 +64:19:53.2: 11.20 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:18.26 +64:28:06.7: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry filter REJECTED candidate at 02:46:24.81 +64:19:53.2: ref_mag=11.20 +/- 0.01 new_mean_mag=11.4315 delta=-0.23 (need > 0.90)
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 01:20:18.26 +64:28:06.7: ref_mag=12.56 +/- 0.01 new_mean_mag=11.5277 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.08 +59:15:34.3: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:28.89 +60:14:00.6: 14.74 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:09.74 +60:17:11.0: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 01:35:09.74 +60:17:11.0: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1286 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.08 +59:15:34.3: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.08 +59:15:34.3: ref_mag=9.75 +/- 0.00 new_mean_mag=8.6858 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:40.70 +60:54:42.3: 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 01:16:28.89 +60:14:00.6: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 01:16:28.89 +60:14:00.6: ref_mag=12.33 +/- 0.01 new_mean_mag=11.2461 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.70 +60:54:42.3: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter KEPT candidate at 02:21:40.70 +60:54:42.3: ref_mag=11.02 +/- 0.00 new_mean_mag=9.5241 delta=1.49 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out52398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out12304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 52171_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52171_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
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Considering the candidate 52203_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52203_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:36:59.78 +63:08:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52330_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52330_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:34:26.93 +64:32:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52365_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52365_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:18:56.91 +57:10:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52398_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52398_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:20:18.26 +64:28:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 0.034 524828343402056448 020.07609894905 +64.46853446171 9.8729 8.4133 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52412_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52412_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:26:41.00 +60:46:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52421_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52421_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:56:24.02 +60:44:30.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 52481_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52481_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:21:54.76 +61:20:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.435 510881966115283968 020.47798671404 +61.34863869013 10.4485 9.3924 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52517_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52517_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
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Considering the candidate 52527_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52527_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:38:01.01 +63:01:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52549_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 52549_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:35:09.74 +60:17:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.034 509781389340597888 023.79046296373 +60.28610796879 10.7712 9.4171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 02633_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 02633_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:15:23.74 +65:01:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18044_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 18044_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 26424_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 26424_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:51:53.08 +57:12:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20109_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 20109_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 51449_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 51449_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:30:27.35 +62:31:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23703_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 23703_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:54:53.90 +58:33:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12304_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 12304_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 29658_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 29658_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:22:51.58 +57:50:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08339_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 08339_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 250672_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250672_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250674_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250674_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250679_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250679_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250680_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250680_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250682_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250682_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250683_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250683_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:03:08.82 +63:52:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250692_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250692_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250696_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250696_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250697_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250697_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250702_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250702_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:30:11.94 +64:43:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250704_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250704_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250705_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250705_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250713_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250713_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250718_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250718_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250722_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250722_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250723_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250723_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250725_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250725_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250728_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250728_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250730_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250730_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250731_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250731_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:05:21.39 +64:15:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250734_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250734_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250738_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250738_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250739_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250739_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250741_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250741_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250743_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250743_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250744_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250744_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250747_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250747_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250754_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250754_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250756_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250756_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 250762_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250762_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250763_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250763_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250764_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250764_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250765_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250765_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:59:46.00 +63:47:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250766_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250766_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250768_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250768_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:58:07.76 +64:50:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250771_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250771_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250772_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250772_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
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Considering the candidate 250773_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250773_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250774_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250774_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250776_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250776_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250778_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250778_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250779_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250779_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:01:30.92 +65:05:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250780_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250780_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250782_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250782_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250785_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250785_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:57:03.82 +59:44:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250789_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250789_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250790_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250790_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250791_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250791_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250794_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250794_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:55:14.58 +59:32:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250795_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250795_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250796_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250796_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 250797_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250797_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
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Considering the candidate 250839_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250839_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:48:46.93 +56:41:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250900_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250900_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 250903_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 250903_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 250928_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 250928_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251045_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251045_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:26:41.02 +60:46:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251049_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251049_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 251090_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251090_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251130_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251130_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:48:23.37 +60:58:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251145_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251145_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:56:38.49 +59:13:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251161_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251161_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:38:00.53 +57:56:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251167_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251167_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 251214_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251214_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:49:48.29 +65:05:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251241_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251241_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:53:16.22 +61:08:53.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251251_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251251_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:08:15.80 +63:34:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251288_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251288_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:21:50.70 +57:15:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251295_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251295_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:37:02.76 +66:22:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251353_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251353_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:31:15.28 +58:01:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251395_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251395_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:04:32.57 +57:59:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251401_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251401_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
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Considering the candidate 251412_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251412_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:56:28.43 +60:47:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251420_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251420_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:19:12.19 +65:36:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251437_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251437_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:16:08.15 +58:49:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251447_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251447_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:45:43.44 +56:47:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251479_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251479_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 251490_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251490_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:35:15.01 +63:00:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251508_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251508_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:05:03.78 +64:21:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251518_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251518_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251522_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251522_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251530_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251530_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251556_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251556_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:58:01.41 +65:22:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251563_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251563_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:46:34.31 +63:01:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251573_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251573_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:46:33.73 +61:16:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251594_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251594_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:44:17.54 +61:53:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251611_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251611_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:49:03.91 +57:59:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251616_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251616_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251620_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251620_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:08:32.24 +63:35:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251642_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251642_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:16:59.53 +57:02:27.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251679_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251679_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:23:23.70 +63:36:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251688_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251688_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:40:50.68 +64:17:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251693_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251693_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:16:38.86 +57:02:19.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251705_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251705_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251719_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251719_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:39:56.94 +60:52:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251721_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251721_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:00:37.08 +58:30:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251733_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251733_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:36:28.89 +62:40:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251759_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251759_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:51:02.86 +64:49:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251769_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251769_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:33:32.82 +60:40:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251770_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251770_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:20:40.51 +56:58:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251774_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251774_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251778_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251778_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:29:34.24 +63:19:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251782_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251782_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:41:56.16 +63:42:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251784_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251784_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:07:40.57 +63:30:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251791_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251791_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251795_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251795_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:40:41.82 +62:41:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251816_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251816_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:56:04.54 +63:37:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251837_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251837_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:26:03.83 +56:05:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251843_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251843_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:02:22.08 +60:42:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251844_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251844_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:23:00.92 +57:15:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251872_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251872_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:11:50.38 +59:02:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251876_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251876_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251879_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251879_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:27:52.94 +62:46:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251880_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251880_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:54:00.98 +63:31:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251883_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251883_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251886_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251886_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:06:23.66 +62:44:02.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251897_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251897_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 251901_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251901_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:13:30.36 +58:34:24.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251909_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251909_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:07:59.12 +57:06:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251913_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251913_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:46:55.25 +59:35:28.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251914_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251914_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:30:08.41 +57:48:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251937_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251937_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:50:02.75 +57:18:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251942_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251942_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:42:33.18 +63:52:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251943_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251943_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:33:23.25 +57:44:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251955_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251955_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:54:51.32 +60:05:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251963_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251963_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:16:12.75 +62:42:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251969_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251969_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:21:01.35 +57:11:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251983_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251983_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
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Considering the candidate 251987_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 251987_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:38:08.01 +61:03:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251994_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 251994_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 252002_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252002_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:51:09.30 +62:24:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252004_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252004_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:04:27.04 +65:05:53.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252005_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252005_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:08:30.85 +58:24:16.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252026_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252026_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:35:50.50 +61:27:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252027_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252027_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:10:27.24 +60:30:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252030_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252030_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 252045_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252045_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 252047_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252047_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 252053_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252053_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:25:50.33 +61:32:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252054_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252054_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:04:08.82 +61:47:28.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252055_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252055_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:17:21.92 +59:22:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252058_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252058_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:19:03.79 +63:57:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252069_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252069_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:01:15.01 +59:23:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252086_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252086_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:11:35.66 +57:37:19.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252092_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252092_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:47:18.93 +63:38:09.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252095_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252095_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252101_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252101_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:38:11.86 +61:01:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252111_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252111_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252115_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252115_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:08:33.26 +63:34:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252124_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252124_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252133_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252133_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252138_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252138_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:00:53.43 +63:25:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252144_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252144_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:45:14.66 +64:24:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252148_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252148_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252155_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252155_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:07:04.00 +59:51:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252163_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252163_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:20:49.41 +64:40:20.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252171_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252171_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252187_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252187_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252191_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252191_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:01:30.04 +62:28:56.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252193_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252193_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252194_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252194_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:45:25.46 +61:12:27.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252203_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252203_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252209_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252209_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:42:42.61 +64:18:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252211_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252211_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:33:12.29 +61:30:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252219_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252219_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:54:06.67 +61:05:11.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252220_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252220_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:23:07.54 +61:11:23.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252222_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252222_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:16:36.99 +64:56:42.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252226_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252226_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252229_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252229_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:55:04.81 +64:32:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252234_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252234_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252236_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252236_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252237_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252237_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252238_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252238_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:11:41.86 +58:41:49.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252240_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252240_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:31:29.36 +58:12:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252249_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252249_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252256_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252256_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:20:13.65 +65:31:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252264_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252264_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:47:28.65 +61:15:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252270_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252270_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:07:03.82 +59:18:17.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252271_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252271_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252280_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252280_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:48:39.98 +59:09:17.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252287_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252287_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:10:45.61 +64:05:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252293_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252293_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:55:40.78 +63:34:27.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252306_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252306_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:31:32.67 +61:02:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252328_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252328_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252341_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252341_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:06:12.41 +57:43:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252343_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252343_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:51:36.24 +60:57:53.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252349_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252349_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:58:56.53 +58:04:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252377_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252377_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:00:23.55 +59:45:40.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252389_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252389_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252400_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252400_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:35:22.05 +61:07:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252412_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252412_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252419_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252419_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:34:34.62 +65:48:56.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252437_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252437_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252445_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252445_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:42:28.23 +58:17:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252449_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252449_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:18:04.50 +65:36:25.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252455_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252455_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:42:55.14 +64:01:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252456_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252456_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:14:00.46 +59:02:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252459_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252459_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:26:05.67 +59:01:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252463_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252463_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252464_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252464_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:39:46.05 +65:53:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252465_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252465_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252476_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252476_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252477_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252477_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:27:04.02 +64:43:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252486_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252486_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:01:43.94 +63:37:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252498_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252498_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252500_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252500_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:27:56.51 +62:46:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252501_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252501_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:41:35.80 +57:32:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252516_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252516_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252522_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252522_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:14:00.41 +61:42:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252523_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252523_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252527_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252527_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:16:02.59 +60:36:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252528_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252528_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:41:41.11 +57:56:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252534_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252534_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:45:39.11 +64:38:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252537_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252537_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252543_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252543_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252547_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252547_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:58:09.47 +61:55:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252557_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252557_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:15:05.66 +64:08:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252571_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252571_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:16:14.05 +66:06:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252577_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252577_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252597_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252597_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:33:47.03 +62:31:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252616_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252616_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 252618_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252618_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 252626_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252626_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:20:24.51 +64:00:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252666_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252666_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252671_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252671_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252673_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252673_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 252684_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252684_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252738_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252738_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:17:01.25 +63:21:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252748_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252748_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252755_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252755_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:44:32.47 +61:36:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252765_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252765_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 252803_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252803_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252836_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252836_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 252892_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 252892_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252905_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252905_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 252937_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252937_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 252952_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252952_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 252975_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 252975_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:35:24.05 +64:45:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253015_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 253015_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253038_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 253038_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253059_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 253059_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 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 76951_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 76951_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 176011_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 176011_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:32:45.90 +56:29:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233858_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 233858_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233893_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 233893_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55535_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 55535_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165523_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 165523_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11582_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 11582_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:47:22.39 +66:08:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67097_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 67097_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:36:59.78 +63:08:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106568_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 106568_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 112593_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19936_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 19936_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104399_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 104399_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:21:40.70 +60:54:42.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 70687_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 70687_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:37:09.85 +61:55:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21138_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 21138_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:15:23.74 +65:01:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46105_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 46105_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:38:00.99 +63:01:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134816_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 134816_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211999_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 211999_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:51:53.08 +57:12:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214517_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 214517_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:06:39.53 +56:51:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62860_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 62860_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:11:58.64 +63:39:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195316_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 195316_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84648_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 84648_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 72532_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 72532_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 220870_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 220870_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 130602_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 130602_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 34158_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 34158_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 34359_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 34359_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:34:26.98 +64:32:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76113_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 76113_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:02:02.21 +62:41:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84112_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 84112_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 140285_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 140285_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:16:28.91 +60:14:00.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 235808_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 235808_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:53:02.89 +60:35:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56031_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 56031_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 212003_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 212003_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 70271_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 70271_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:20:32.72 +62:32:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173490_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 173490_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:22:51.59 +57:50:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66586_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 66586_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 60720_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 60720_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 117965_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 117965_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 182857_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 182857_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 157256_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 157256_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 196494_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 196494_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:01:28.11 +58:18:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12954_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 12954_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:13:30.92 +65:37:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233873_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 233873_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 45963_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 45963_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 233707_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 233707_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 15018_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 15018_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:58:56.46 +65:44:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233560_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 233560_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 28797_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 28797_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 219425_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 219425_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 233455_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 233455_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 16229_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 16229_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:28:05.36 +64:58:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168042_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 168042_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 39378_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 39378_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:47:55.71 +64:32:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124535_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 124535_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 213022_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 213022_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:14:49.77 +57:23:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156692_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 156692_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:56:38.09 +59:15:34.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 209662_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 209662_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:31:04.80 +57:13:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178813_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 178813_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:04:41.82 +57:30:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22840_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 22840_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 210668_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 210668_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:43:57.39 +57:03:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173182_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 173182_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 193780_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 193780_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 00:54:53.89 +58:33:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63215_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 63215_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:30:27.35 +62:31:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67187_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 67187_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 08809_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 08809_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 02:27:30.89 +65:38:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58464_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 58464_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 21028_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 21028_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 241160_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 241160_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 104341_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 104341_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 92255_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
The candidate 92255_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459 did not pass the final checks
**** FOUND 01:00:48.99 +62:16:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153703_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 153703_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
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Considering the candidate 137025_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
Preparing report for the candidate 137025_fd_Cas-03-Q1b1x1_2026-06-11_05-09-14_20.00sec_-0.00C_LIGHTs_0459
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 365s
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 ####
02:21:40.70 +60:54:42.3
01:16:28.89 +60:14:00.6
01:56:38.08 +59:15:34.3
02:40:38.88 +60:07:58.7
02:10:17.83 +60:58:59.7
01:21:54.89 +61:20:56.5
01:32:28.17 +61:03:28.1
01:33:44.42 +60:46:19.9
02:19:16.61 +59:42:22.6
02:24:29.80 +59:24:31.9
01:35:09.77 +60:17:10.9
02:18:22.64 +58:47:11.0
02:18:24.74 +58:37:27.8
01:41:47.05 +59:03:48.5
01:09:37.99 +59:05:15.2
02:03:07.39 +57:18:15.1
02:35:19.15 +56:39:41.2
01:33:46.78 +58:39:46.2
02:48:41.14 +63:58:46.1
02:49:57.11 +63:51:37.9
02:27:17.51 +56:07:13.9
02:09:55.23 +56:59:24.0
02:34:46.49 +56:12:07.0
02:33:23.74 +64:25:00.4
00:42:54.80 +62:48:25.7
02:46:03.81 +63:32:43.4
01:22:27.49 +65:23:26.6
02:47:29.79 +65:31:27.8
00:44:01.60 +58:23:35.1
02:26:23.38 +56:29:19.8
02:00:42.05 +61:18:04.8
01:29:16.07 +60:15:48.3
02:41:51.08 +62:00:32.2
01:04:16.84 +62:17:14.4
01:08:25.44 +59:48:04.0
02:52:58.74 +63:23:24.0
01:37:41.97 +59:27:45.8
02:41:58.35 +60:23:19.7
00:59:30.61 +62:53:54.5
02:38:12.38 +59:36:40.8
01:02:45.81 +63:46:48.9
01:55:53.64 +64:36:21.5
00:52:45.42 +63:28:59.5
00:39:51.75 +62:45:29.3
00:59:24.06 +57:51:42.7
01:15:35.37 +59:15:09.5
00:46:28.44 +58:20:30.0
01:54:24.92 +59:00:13.7
01:49:30.14 +57:16:28.7
01:52:49.00 +56:57:10.2
01:21:38.69 +59:26:15.1
00:44:53.41 +58:45:49.8
01:48:02.36 +60:59:06.6
01:10:11.71 +59:17:24.9
02:15:24.05 +59:54:56.8
01:11:44.76 +61:13:57.4
02:33:58.68 +56:29:45.2
00:52:38.68 +58:02:49.1
02:04:54.31 +64:12:10.2
01:39:23.91 +58:23:02.3
00:45:11.09 +57:46:43.2
00:54:31.19 +59:24:00.6
02:30:17.42 +57:10:05.2
00:44:13.57 +56:48:03.6
00:56:47.69 +60:38:48.5
00:55:30.17 +62:23:46.1
01:40:55.79 +57:55:16.6
01:02:08.11 +60:49:21.2
00:52:55.15 +58:28:52.4
01:12:40.87 +61:20:38.1
02:07:04.56 +58:31:27.6
00:36:55.09 +62:40:47.3
00:52:16.25 +59:42:58.7
00:52:30.72 +59:43:27.2
01:03:22.65 +60:32:13.7
01:29:32.92 +61:46:25.9
01:20:56.88 +62:03:30.3
00:36:55.70 +62:32:56.0
01:03:35.55 +60:28:10.7
01:22:23.86 +61:13:51.7
00:52:12.56 +64:57:22.2
00:45:37.79 +56:46:42.5
02:10:23.90 +60:01:13.3
01:59:33.44 +60:01:44.9
01:29:32.90 +63:19:35.9
02:22:13.26 +59:08:19.8
00:38:04.03 +62:29:01.6
01:19:41.77 +62:51:04.8
01:18:36.92 +58:41:37.9
01:03:24.22 +61:12:24.3
02:02:54.01 +60:15:41.7
01:18:48.42 +64:12:22.2
02:19:57.66 +59:32:25.7
01:34:42.46 +58:42:14.7
00:54:25.57 +60:12:30.4
01:09:51.36 +57:04:44.5
01:38:08.14 +61:01:39.6
02:00:32.97 +59:40:07.0
02:02:50.62 +60:13:57.8
01:29:49.78 +58:44:46.4
01:43:03.65 +58:57:14.1
01:51:09.55 +64:52:45.9
02:02:24.51 +64:38:24.6
00:44:39.75 +62:06:29.5
01:14:21.78 +59:59:49.2
00:50:25.40 +60:08:08.8
01:23:46.01 +60:53:25.2
01:11:56.69 +58:41:05.6
01:31:48.55 +64:22:28.2
01:25:19.00 +62:14:40.2
01:05:51.59 +60:27:36.2
01:02:13.99 +59:56:04.8
01:55:53.02 +64:15:25.6
02:39:11.03 +63:43:56.9
02:01:21.95 +66:30:18.0
01:20:34.92 +64:02:26.7
01:06:55.38 +59:18:56.7
01:08:11.42 +62:14:22.3
01:07:44.51 +59:03:02.7
01:17:07.44 +62:50:32.4
01:49:47.63 +65:03:22.0
01:39:32.59 +64:53:04.2
01:20:18.28 +64:28:06.2
02:44:05.83 +62:19:56.7
02:06:50.44 +63:27:21.8
02:13:47.76 +63:11:27.0
02:48:49.50 +61:53:28.2
02:15:26.79 +62:47:46.4
02:48:30.05 +61:37:04.3
01:45:35.83 +63:07:08.5
01:58:48.47 +62:43:32.2
02:07:46.81 +62:11:12.5
01:32:51.46 +62:40:37.1
########### Completed Cas-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:16:28.89 +60:14:00.6
01:56:38.08 +59:15:34.3
02:21:40.70 +60:54:42.3
02:00:42.05 +61:18:04.8
01:29:16.07 +60:15:48.3
02:41:51.08 +62:00:32.2
01:04:16.84 +62:17:14.4
01:08:25.44 +59:48:04.0
02:52:58.74 +63:23:24.0
01:37:41.97 +59:27:45.8
02:41:58.35 +60:23:19.7
00:59:30.61 +62:53:54.5
02:38:12.38 +59:36:40.8
01:02:45.81 +63:46:48.9
01:55:53.64 +64:36:21.5
00:52:45.42 +63:28:59.5
00:39:51.75 +62:45:29.3
00:59:24.06 +57:51:42.7
01:15:35.37 +59:15:09.5
00:46:28.44 +58:20:30.0
01:54:24.92 +59:00:13.7
01:49:30.14 +57:16:28.7
01:52:49.00 +56:57:10.2
01:21:38.69 +59:26:15.1
00:44:53.41 +58:45:49.8
01:48:02.36 +60:59:06.6
01:10:11.71 +59:17:24.9
02:15:24.05 +59:54:56.8
01:11:44.76 +61:13:57.4
02:33:58.68 +56:29:45.2
00:52:38.68 +58:02:49.1
02:04:54.31 +64:12:10.2
01:39:23.91 +58:23:02.3
00:45:11.09 +57:46:43.2
00:54:31.19 +59:24:00.6
02:30:17.42 +57:10:05.2
00:44:13.57 +56:48:03.6
00:56:47.69 +60:38:48.5
00:55:30.17 +62:23:46.1
01:40:55.79 +57:55:16.6
01:02:08.11 +60:49:21.2
00:52:55.15 +58:28:52.4
01:12:40.87 +61:20:38.1
02:07:04.56 +58:31:27.6
00:36:55.09 +62:40:47.3
00:52:16.25 +59:42:58.7
00:52:30.72 +59:43:27.2
01:03:22.65 +60:32:13.7
01:29:32.92 +61:46:25.9
01:20:56.88 +62:03:30.3
00:36:55.70 +62:32:56.0
01:03:35.55 +60:28:10.7
01:22:23.86 +61:13:51.7
00:52:12.56 +64:57:22.2
00:45:37.79 +56:46:42.5
02:10:23.90 +60:01:13.3
01:59:33.44 +60:01:44.9
01:29:32.90 +63:19:35.9
02:22:13.26 +59:08:19.8
00:38:04.03 +62:29:01.6
01:19:41.77 +62:51:04.8
01:18:36.92 +58:41:37.9
01:03:24.22 +61:12:24.3
02:02:54.01 +60:15:41.7
01:18:48.42 +64:12:22.2
02:19:57.66 +59:32:25.7
01:34:42.46 +58:42:14.7
00:54:25.57 +60:12:30.4
01:09:51.36 +57:04:44.5
01:38:08.14 +61:01:39.6
02:00:32.97 +59:40:07.0
02:02:50.62 +60:13:57.8
01:29:49.78 +58:44:46.4
01:43:03.65 +58:57:14.1
01:51:09.55 +64:52:45.9
02:02:24.51 +64:38:24.6
00:44:39.75 +62:06:29.5
01:14:21.78 +59:59:49.2
00:50:25.40 +60:08:08.8
01:23:46.01 +60:53:25.2
01:11:56.69 +58:41:05.6
01:31:48.55 +64:22:28.2
01:25:19.00 +62:14:40.2
01:05:51.59 +60:27:36.2
01:02:13.99 +59:56:04.8
01:55:53.02 +64:15:25.6
02:39:11.03 +63:43:56.9
02:01:21.95 +66:30:18.0
01:20:34.92 +64:02:26.7
01:06:55.38 +59:18:56.7
01:08:11.42 +62:14:22.3
01:07:44.51 +59:03:02.7
01:17:07.44 +62:50:32.4
01:58:48.47 +62:43:32.2
02:47:29.79 +65:31:27.8
02:26:23.38 +56:29:19.8
02:44:05.83 +62:19:56.7
01:41:47.05 +59:03:48.5
02:10:17.83 +60:58:59.7
01:21:54.89 +61:20:56.5
02:48:41.14 +63:58:46.1
02:24:29.80 +59:24:31.9
01:33:46.78 +58:39:46.2
01:32:51.46 +62:40:37.1
01:45:35.83 +63:07:08.5
02:34:46.49 +56:12:07.0
02:19:16.61 +59:42:22.6
01:39:32.59 +64:53:04.2
02:07:46.81 +62:11:12.5
02:06:50.44 +63:27:21.8
02:27:17.51 +56:07:13.9
02:15:26.79 +62:47:46.4
02:48:49.50 +61:53:28.2
01:32:28.17 +61:03:28.1
02:35:19.15 +56:39:41.2
02:18:24.74 +58:37:27.8
00:44:01.60 +58:23:35.1
01:20:18.28 +64:28:06.2
01:22:27.49 +65:23:26.6
02:46:03.81 +63:32:43.4
01:49:47.63 +65:03:22.0
02:09:55.23 +56:59:24.0
00:42:54.80 +62:48:25.7
01:09:37.99 +59:05:15.2
01:33:44.42 +60:46:19.9
02:33:23.74 +64:25:00.4
02:03:07.39 +57:18:15.1
02:48:30.05 +61:37:04.3
02:13:47.76 +63:11:27.0
02:49:57.11 +63:51:37.9
02:40:38.88 +60:07:58.7
02:18:22.64 +58:47:11.0
01:35:09.77 +60:17:10.9
###################################################################################
01:16:28.89 +60:14:00.6 -- not an asteroid (will add it to exclusion list)
01:56:38.08 +59:15:34.3 -- not an asteroid (will add it to exclusion list)
02:21:40.70 +60:54:42.3 -- not an asteroid (will add it to exclusion list)
02:00:42.05 +61:18:04.8 -- not an asteroid (will add it to exclusion list)
01:29:16.07 +60:15:48.3 -- not an asteroid (will add it to exclusion list)
02:41:51.08 +62:00:32.2 -- not an asteroid (will add it to exclusion list)
01:04:16.84 +62:17:14.4 -- not an asteroid (will add it to exclusion list)
01:08:25.44 +59:48:04.0 -- not an asteroid (will add it to exclusion list)
02:52:58.74 +63:23:24.0 -- not an asteroid (will add it to exclusion list)
01:37:41.97 +59:27:45.8 -- not an asteroid (will add it to exclusion list)
02:41:58.35 +60:23:19.7 -- not an asteroid (will add it to exclusion list)
00:59:30.61 +62:53:54.5 -- not an asteroid (will add it to exclusion list)
02:38:12.38 +59:36:40.8 -- not an asteroid (will add it to exclusion list)
01:02:45.81 +63:46:48.9 -- not an asteroid (will add it to exclusion list)
01:55:53.64 +64:36:21.5 -- not an asteroid (will add it to exclusion list)
00:52:45.42 +63:28:59.5 -- not an asteroid (will add it to exclusion list)
00:39:51.75 +62:45:29.3 -- not an asteroid (will add it to exclusion list)
00:59:24.06 +57:51:42.7 -- not an asteroid (will add it to exclusion list)
01:15:35.37 +59:15:09.5 -- not an asteroid (will add it to exclusion list)
00:46:28.44 +58:20:30.0 -- not an asteroid (will add it to exclusion list)
01:54:24.92 +59:00:13.7 -- not an asteroid (will add it to exclusion list)
01:49:30.14 +57:16:28.7 -- not an asteroid (will add it to exclusion list)
01:52:49.00 +56:57:10.2 -- not an asteroid (will add it to exclusion list)
01:21:38.69 +59:26:15.1 -- not an asteroid (will add it to exclusion list)
00:44:53.41 +58:45:49.8 -- not an asteroid (will add it to exclusion list)
01:48:02.36 +60:59:06.6 -- not an asteroid (will add it to exclusion list)
01:10:11.71 +59:17:24.9 -- not an asteroid (will add it to exclusion list)
02:15:24.05 +59:54:56.8 -- not an asteroid (will add it to exclusion list)
01:11:44.76 +61:13:57.4 -- not an asteroid (will add it to exclusion list)
02:33:58.68 +56:29:45.2 -- not an asteroid (will add it to exclusion list)
00:52:38.68 +58:02:49.1 -- not an asteroid (will add it to exclusion list)
02:04:54.31 +64:12:10.2 -- not an asteroid (will add it to exclusion list)
01:39:23.91 +58:23:02.3 -- not an asteroid (will add it to exclusion list)
00:45:11.09 +57:46:43.2 -- not an asteroid (will add it to exclusion list)
00:54:31.19 +59:24:00.6 -- not an asteroid (will add it to exclusion list)
02:30:17.42 +57:10:05.2 -- not an asteroid (will add it to exclusion list)
00:44:13.57 +56:48:03.6 -- not an asteroid (will add it to exclusion list)
00:56:47.69 +60:38:48.5 -- not an asteroid (will add it to exclusion list)
00:55:30.17 +62:23:46.1 -- not an asteroid (will add it to exclusion list)
01:40:55.79 +57:55:16.6 -- not an asteroid (will add it to exclusion list)
01:02:08.11 +60:49:21.2 -- not an asteroid (will add it to exclusion list)
00:52:55.15 +58:28:52.4 -- not an asteroid (will add it to exclusion list)
01:12:40.87 +61:20:38.1 -- not an asteroid (will add it to exclusion list)
02:07:04.56 +58:31:27.6 -- not an asteroid (will add it to exclusion list)
00:36:55.09 +62:40:47.3 -- not an asteroid (will add it to exclusion list)
00:52:16.25 +59:42:58.7 -- not an asteroid (will add it to exclusion list)
00:52:30.72 +59:43:27.2 -- not an asteroid (will add it to exclusion list)
01:03:22.65 +60:32:13.7 -- not an asteroid (will add it to exclusion list)
01:29:32.92 +61:46:25.9 -- not an asteroid (will add it to exclusion list)
01:20:56.88 +62:03:30.3 -- not an asteroid (will add it to exclusion list)
00:36:55.70 +62:32:56.0 -- not an asteroid (will add it to exclusion list)
01:03:35.55 +60:28:10.7 -- not an asteroid (will add it to exclusion list)
01:22:23.86 +61:13:51.7 -- not an asteroid (will add it to exclusion list)
00:52:12.56 +64:57:22.2 -- not an asteroid (will add it to exclusion list)
00:45:37.79 +56:46:42.5 -- not an asteroid (will add it to exclusion list)
02:10:23.90 +60:01:13.3 -- not an asteroid (will add it to exclusion list)
01:59:33.44 +60:01:44.9 -- not an asteroid (will add it to exclusion list)
01:29:32.90 +63:19:35.9 -- not an asteroid (will add it to exclusion list)
02:22:13.26 +59:08:19.8 -- not an asteroid (will add it to exclusion list)
00:38:04.03 +62:29:01.6 -- not an asteroid (will add it to exclusion list)
01:19:41.77 +62:51:04.8 -- not an asteroid (will add it to exclusion list)
01:18:36.92 +58:41:37.9 -- not an asteroid (will add it to exclusion list)
01:03:24.22 +61:12:24.3 -- not an asteroid (will add it to exclusion list)
02:02:54.01 +60:15:41.7 -- not an asteroid (will add it to exclusion list)
01:18:48.42 +64:12:22.2 -- not an asteroid (will add it to exclusion list)
02:19:57.66 +59:32:25.7 -- not an asteroid (will add it to exclusion list)
01:34:42.46 +58:42:14.7 -- not an asteroid (will add it to exclusion list)
00:54:25.57 +60:12:30.4 -- not an asteroid (will add it to exclusion list)
01:09:51.36 +57:04:44.5 -- not an asteroid (will add it to exclusion list)
01:38:08.14 +61:01:39.6 -- not an asteroid (will add it to exclusion list)
02:00:32.97 +59:40:07.0 -- not an asteroid (will add it to exclusion list)
02:02:50.62 +60:13:57.8 -- not an asteroid (will add it to exclusion list)
01:29:49.78 +58:44:46.4 -- not an asteroid (will add it to exclusion list)
01:43:03.65 +58:57:14.1 -- not an asteroid (will add it to exclusion list)
01:51:09.55 +64:52:45.9 -- not an asteroid (will add it to exclusion list)
02:02:24.51 +64:38:24.6 -- not an asteroid (will add it to exclusion list)
00:44:39.75 +62:06:29.5 -- not an asteroid (will add it to exclusion list)
01:14:21.78 +59:59:49.2 -- not an asteroid (will add it to exclusion list)
00:50:25.40 +60:08:08.8 -- not an asteroid (will add it to exclusion list)
01:23:46.01 +60:53:25.2 -- not an asteroid (will add it to exclusion list)
01:11:56.69 +58:41:05.6 -- not an asteroid (will add it to exclusion list)
01:31:48.55 +64:22:28.2 -- not an asteroid (will add it to exclusion list)
01:25:19.00 +62:14:40.2 -- not an asteroid (will add it to exclusion list)
01:05:51.59 +60:27:36.2 -- not an asteroid (will add it to exclusion list)
01:02:13.99 +59:56:04.8 -- not an asteroid (will add it to exclusion list)
01:55:53.02 +64:15:25.6 -- not an asteroid (will add it to exclusion list)
02:39:11.03 +63:43:56.9 -- not an asteroid (will add it to exclusion list)
02:01:21.95 +66:30:18.0 -- not an asteroid (will add it to exclusion list)
01:20:34.92 +64:02:26.7 -- not an asteroid (will add it to exclusion list)
01:06:55.38 +59:18:56.7 -- not an asteroid (will add it to exclusion list)
01:08:11.42 +62:14:22.3 -- not an asteroid (will add it to exclusion list)
01:07:44.51 +59:03:02.7 -- not an asteroid (will add it to exclusion list)
01:17:07.44 +62:50:32.4 -- not an asteroid (will add it to exclusion list)
01:58:48.47 +62:43:32.2 -- not an asteroid (will add it to exclusion list)
02:47:29.79 +65:31:27.8 -- not an asteroid (will add it to exclusion list)
02:26:23.38 +56:29:19.8 -- not an asteroid (will add it to exclusion list)
02:44:05.83 +62:19:56.7 -- not an asteroid (will add it to exclusion list)
01:41:47.05 +59:03:48.5 -- not an asteroid (will add it to exclusion list)
02:10:17.83 +60:58:59.7 -- not an asteroid (will add it to exclusion list)
01:21:54.89 +61:20:56.5 -- not an asteroid (will add it to exclusion list)
02:48:41.14 +63:58:46.1 -- not an asteroid (will add it to exclusion list)
02:24:29.80 +59:24:31.9 -- not an asteroid (will add it to exclusion list)
01:33:46.78 +58:39:46.2 -- not an asteroid (will add it to exclusion list)
01:32:51.46 +62:40:37.1 -- not an asteroid (will add it to exclusion list)
01:45:35.83 +63:07:08.5 -- not an asteroid (will add it to exclusion list)
02:34:46.49 +56:12:07.0 -- not an asteroid (will add it to exclusion list)
02:19:16.61 +59:42:22.6 -- not an asteroid (will add it to exclusion list)
01:39:32.59 +64:53:04.2 -- not an asteroid (will add it to exclusion list)
02:07:46.81 +62:11:12.5 -- not an asteroid (will add it to exclusion list)
02:06:50.44 +63:27:21.8 -- not an asteroid (will add it to exclusion list)
02:27:17.51 +56:07:13.9 -- not an asteroid (will add it to exclusion list)
02:15:26.79 +62:47:46.4 -- not an asteroid (will add it to exclusion list)
02:48:49.50 +61:53:28.2 -- not an asteroid (will add it to exclusion list)
01:32:28.17 +61:03:28.1 -- not an asteroid (will add it to exclusion list)
02:35:19.15 +56:39:41.2 -- not an asteroid (will add it to exclusion list)
02:18:24.74 +58:37:27.8 -- not an asteroid (will add it to exclusion list)
00:44:01.60 +58:23:35.1 -- not an asteroid (will add it to exclusion list)
01:20:18.28 +64:28:06.2 -- not an asteroid (will add it to exclusion list)
01:22:27.49 +65:23:26.6 -- not an asteroid (will add it to exclusion list)
02:46:03.81 +63:32:43.4 -- not an asteroid (will add it to exclusion list)
01:49:47.63 +65:03:22.0 -- not an asteroid (will add it to exclusion list)
02:09:55.23 +56:59:24.0 -- not an asteroid (will add it to exclusion list)
00:42:54.80 +62:48:25.7 -- not an asteroid (will add it to exclusion list)
01:09:37.99 +59:05:15.2 -- not an asteroid (will add it to exclusion list)
01:33:44.42 +60:46:19.9 -- not an asteroid (will add it to exclusion list)
02:33:23.74 +64:25:00.4 -- not an asteroid (will add it to exclusion list)
02:03:07.39 +57:18:15.1 -- not an asteroid (will add it to exclusion list)
02:48:30.05 +61:37:04.3 -- not an asteroid (will add it to exclusion list)
02:13:47.76 +63:11:27.0 -- not an asteroid (will add it to exclusion list)
02:49:57.11 +63:51:37.9 -- not an asteroid (will add it to exclusion list)
02:40:38.88 +60:07:58.7 -- not an asteroid (will add it to exclusion list)
02:18:22.64 +58:47:11.0 -- not an asteroid (will add it to exclusion list)
01:35:09.77 +60:17:10.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:36:55.09 +62:40:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:55.70 +62:32:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:04.03 +62:29:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:51.75 +62:45:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:54.80 +62:48:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:01.60 +58:23:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:13.57 +56:48:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:39.75 +62:06:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:53.41 +58:45:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:11.09 +57:46:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:37.79 +56:46:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:28.44 +58:20:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:25.40 +60:08:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:12.56 +64:57:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:16.25 +59:42:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:30.72 +59:43:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:38.68 +58:02:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:45.42 +63:28:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:55.15 +58:28:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:25.57 +60:12:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:31.19 +59:24:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:30.17 +62:23:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:47.69 +60:38:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:24.06 +57:51:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:30.61 +62:53:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:08.11 +60:49:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:13.99 +59:56:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:45.81 +63:46:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:22.65 +60:32:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:24.22 +61:12:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:35.55 +60:28:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:04:16.84 +62:17:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:51.59 +60:27:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.38 +59:18:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:44.51 +59:03:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:11.42 +62:14:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:25.44 +59:48:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:37.99 +59:05:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:51.36 +57:04:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:11.71 +59:17:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:44.76 +61:13:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:56.69 +58:41:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:40.87 +61:20:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:21.78 +59:59:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:35.37 +59:15:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:28.89 +60:14:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:07.44 +62:50:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:36.92 +58:41:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:48.42 +64:12:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:41.77 +62:51:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:18.28 +64:28:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:34.92 +64:02:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:56.88 +62:03:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:38.69 +59:26:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:54.89 +61:20:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:23.86 +61:13:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:27.49 +65:23:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:46.01 +60:53:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:19.00 +62:14:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:16.07 +60:15:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.90 +63:19:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.92 +61:46:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:49.78 +58:44:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.55 +64:22:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:28.17 +61:03:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:51.46 +62:40:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:44.42 +60:46:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:46.78 +58:39:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:42.46 +58:42:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:09.77 +60:17:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:41.97 +59:27:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:08.14 +61:01:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:23.91 +58:23:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:32.59 +64:53:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:55.79 +57:55:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:47.05 +59:03:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.65 +58:57:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:35.83 +63:07:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:02.36 +60:59:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:30.14 +57:16:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:47.63 +65:03:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:09.55 +64:52:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:49.00 +56:57:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:24.92 +59:00:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:53.02 +64:15:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:53.64 +64:36:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.08 +59:15:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:48.47 +62:43:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:33.44 +60:01:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.97 +59:40:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:42.05 +61:18:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:21.95 +66:30:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:24.51 +64:38:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:50.62 +60:13:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:54.01 +60:15:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:07.39 +57:18:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:54.31 +64:12:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:50.44 +63:27:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:04.56 +58:31:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:46.81 +62:11:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:55.23 +56:59:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:17.83 +60:58:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:23.90 +60:01:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.76 +63:11:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:24.05 +59:54:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:26.79 +62:47:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:22.64 +58:47:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:24.74 +58:37:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:16.61 +59:42:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:57.66 +59:32:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:40.70 +60:54:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:13.26 +59:08:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:29.80 +59:24:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:23.38 +56:29:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:17.51 +56:07:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:17.42 +57:10:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:23.74 +64:25:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:58.68 +56:29:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:46.49 +56:12:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:19.15 +56:39:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:12.38 +59:36:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:11.03 +63:43:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:40:38.88 +60:07:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:51.08 +62:00:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:41:58.35 +60:23:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:44:05.83 +62:19:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:46:03.81 +63:32:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:47:29.79 +65:31:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:30.05 +61:37:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:41.14 +63:58:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:49.50 +61:53:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:57.11 +63:51:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:58.74 +63:23:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:36:55.09 +62:40:47.3 -- not a known variable star
00:36:55.70 +62:32:56.0 -- not a known variable star
00:38:04.03 +62:29:01.6 -- not a known variable star
00:39:51.75 +62:45:29.3 -- not a known variable star
00:42:54.80 +62:48:25.7 -- a known variable star
00:44:01.60 +58:23:35.1 -- not a known variable star
00:44:13.57 +56:48:03.6 -- a known variable star
00:44:39.75 +62:06:29.5 -- not a known variable star
00:44:53.41 +58:45:49.8 -- not a known variable star
00:45:11.09 +57:46:43.2 -- a known variable star
00:45:37.79 +56:46:42.5 -- not a known variable star
00:46:28.44 +58:20:30.0 -- not a known variable star
00:50:25.40 +60:08:08.8 -- not a known variable star
00:52:12.56 +64:57:22.2 -- not a known variable star
00:52:16.25 +59:42:58.7 -- a known variable star
00:52:30.72 +59:43:27.2 -- not a known variable star
00:52:38.68 +58:02:49.1 -- not a known variable star
00:52:45.42 +63:28:59.5 -- not a known variable star
00:52:55.15 +58:28:52.4 -- not a known variable star
00:54:25.57 +60:12:30.4 -- not a known variable star
00:54:31.19 +59:24:00.6 -- a known variable star
00:55:30.17 +62:23:46.1 -- not a known variable star
00:56:47.69 +60:38:48.5 -- not a known variable star
00:59:24.06 +57:51:42.7 -- not a known variable star
00:59:30.61 +62:53:54.5 -- not a known variable star
01:02:08.11 +60:49:21.2 -- not a known variable star
01:02:13.99 +59:56:04.8 -- not a known variable star
01:02:45.81 +63:46:48.9 -- not a known variable star
01:03:22.65 +60:32:13.7 -- not a known variable star
01:03:24.22 +61:12:24.3 -- not a known variable star
01:03:35.55 +60:28:10.7 -- not a known variable star
01:04:16.84 +62:17:14.4 -- not a known variable star
01:05:51.59 +60:27:36.2 -- a known variable star
01:06:55.38 +59:18:56.7 -- not a known variable star
01:07:44.51 +59:03:02.7 -- a known variable star
01:08:11.42 +62:14:22.3 -- a known variable star
01:08:25.44 +59:48:04.0 -- not a known variable star
01:09:37.99 +59:05:15.2 -- a known variable star
01:09:51.36 +57:04:44.5 -- a known variable star
01:10:11.71 +59:17:24.9 -- not a known variable star
01:11:44.76 +61:13:57.4 -- a known variable star
01:11:56.69 +58:41:05.6 -- not a known variable star
01:12:40.87 +61:20:38.1 -- not a known variable star
01:14:21.78 +59:59:49.2 -- not a known variable star
01:15:35.37 +59:15:09.5 -- not a known variable star
01:16:28.89 +60:14:00.6 -- a known variable star
01:17:07.44 +62:50:32.4 -- a known variable star
01:18:36.92 +58:41:37.9 -- a known variable star
01:18:48.42 +64:12:22.2 -- not a known variable star
01:19:41.77 +62:51:04.8 -- not a known variable star
01:20:18.28 +64:28:06.2 -- a known variable star
01:20:34.92 +64:02:26.7 -- not a known variable star
01:20:56.88 +62:03:30.3 -- not a known variable star
01:21:38.69 +59:26:15.1 -- not a known variable star
01:21:54.89 +61:20:56.5 -- a known variable star
01:22:23.86 +61:13:51.7 -- a known variable star
01:22:27.49 +65:23:26.6 -- not a known variable star
01:23:46.01 +60:53:25.2 -- not a known variable star
01:25:19.00 +62:14:40.2 -- not a known variable star
01:29:16.07 +60:15:48.3 -- not a known variable star
01:29:32.90 +63:19:35.9 -- a known variable star
01:29:32.92 +61:46:25.9 -- not a known variable star
01:29:49.78 +58:44:46.4 -- not a known variable star
01:31:48.55 +64:22:28.2 -- not a known variable star
01:32:28.17 +61:03:28.1 -- not a known variable star
01:32:51.46 +62:40:37.1 -- a known variable star
01:33:44.42 +60:46:19.9 -- not a known variable star
01:33:46.78 +58:39:46.2 -- a known variable star
01:34:42.46 +58:42:14.7 -- not a known variable star
01:35:09.77 +60:17:10.9 -- a known variable star
01:37:41.97 +59:27:45.8 -- not a known variable star
01:38:08.14 +61:01:39.6 -- not a known variable star
01:39:23.91 +58:23:02.3 -- not a known variable star
01:39:32.59 +64:53:04.2 -- a known variable star
01:40:55.79 +57:55:16.6 -- not a known variable star
01:41:47.05 +59:03:48.5 -- a known variable star
01:43:03.65 +58:57:14.1 -- not a known variable star
01:45:35.83 +63:07:08.5 -- a known variable star
01:48:02.36 +60:59:06.6 -- a known variable star
01:49:30.14 +57:16:28.7 -- not a known variable star
01:49:47.63 +65:03:22.0 -- a known variable star
01:51:09.55 +64:52:45.9 -- a known variable star
01:52:49.00 +56:57:10.2 -- a known variable star
01:54:24.92 +59:00:13.7 -- not a known variable star
01:55:53.02 +64:15:25.6 -- not a known variable star
01:55:53.64 +64:36:21.5 -- a known variable star
01:56:38.08 +59:15:34.3 -- a known variable star
01:58:48.47 +62:43:32.2 -- a known variable star
01:59:33.44 +60:01:44.9 -- a known variable star
02:00:32.97 +59:40:07.0 -- a known variable star
02:00:42.05 +61:18:04.8 -- not a known variable star
02:01:21.95 +66:30:18.0 -- not a known variable star
02:02:24.51 +64:38:24.6 -- a known variable star
02:02:50.62 +60:13:57.8 -- a known variable star
02:02:54.01 +60:15:41.7 -- not a known variable star
02:03:07.39 +57:18:15.1 -- a known variable star
02:04:54.31 +64:12:10.2 -- not a known variable star
02:06:50.44 +63:27:21.8 -- a known variable star
02:07:04.56 +58:31:27.6 -- not a known variable star
02:07:46.81 +62:11:12.5 -- a known variable star
02:09:55.23 +56:59:24.0 -- a known variable star
02:10:17.83 +60:58:59.7 -- a known variable star
02:10:23.90 +60:01:13.3 -- not a known variable star
02:13:47.76 +63:11:27.0 -- a known variable star
02:15:24.05 +59:54:56.8 -- not a known variable star
02:15:26.79 +62:47:46.4 -- a known variable star
02:18:22.64 +58:47:11.0 -- a known variable star
02:18:24.74 +58:37:27.8 -- a known variable star
02:19:16.61 +59:42:22.6 -- a known variable star
02:19:57.66 +59:32:25.7 -- not a known variable star
02:21:40.70 +60:54:42.3 -- a known variable star
02:22:13.26 +59:08:19.8 -- not a known variable star
02:24:29.80 +59:24:31.9 -- a known variable star
02:26:23.38 +56:29:19.8 -- not a known variable star
02:27:17.51 +56:07:13.9 -- not a known variable star
02:30:17.42 +57:10:05.2 -- a known variable star
02:33:23.74 +64:25:00.4 -- a known variable star
02:33:58.68 +56:29:45.2 -- not a known variable star
02:34:46.49 +56:12:07.0 -- not a known variable star
02:35:19.15 +56:39:41.2 -- a known variable star
02:38:12.38 +59:36:40.8 -- a known variable star
02:39:11.03 +63:43:56.9 -- not a known variable star
02:40:38.88 +60:07:58.7 -- a known variable star
02:41:51.08 +62:00:32.2 -- a known variable star
02:41:58.35 +60:23:19.7 -- not a known variable star
02:44:05.83 +62:19:56.7 -- not a known variable star
02:46:03.81 +63:32:43.4 -- not a known variable star
02:47:29.79 +65:31:27.8 -- not a known variable star
02:48:30.05 +61:37:04.3 -- not a known variable star
02:48:41.14 +63:58:46.1 -- not a known variable star
02:48:49.50 +61:53:28.2 -- not a known variable star
02:49:57.11 +63:51:37.9 -- not a known variable star
02:52:58.74 +63:23:24.0 -- not a known variable star
Found 80 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
133 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 133 (excluding asteroids and hot pixels, 80 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)2461202.92271319 -observatory V36
07:01:51.86 +24:18:51.0 Mercury (0.3mag)
07:59:00.62 +22:41:47.0 Venus (-4.0mag)
02:59:00.78 +16:25:44.2 Mars (1.3mag)
07:51:08.82 +21:24:33.7 Jupiter (-1.9mag)
00:50:16.24 +02:53:31.8 Saturn (0.8mag)
04:00:58.33 +20:27:39.3 Uranus (5.8mag)
00:16:19.35 +00:17:47.6 Neptune (7.8mag)
20:33:10.21 -23:05:46.8 Pluto (14.5mag)
01:42:09.86 +14:16:10.7 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 361 Jun 11 06:00 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461202.92271319:
07:51:03.97 +21:24:49.8 Io (6.0mag)
07:51:03.56 +21:24:51.9 Europa (6.2mag)
07:51:25.60 +21:23:44.8 Ganymede (5.6mag)
07:50:53.24 +21:25:15.5 Callisto (6.7mag)
07:51:14.54 +21:01:08.3 Himalia (15.6mag)
07:51:10.63 +21:24:29.1 Thebe (16.5mag)
07:51:08.60 +21:15:10.4 Elara (17.5mag)
07:53:29.40 +21:34:29.8 Pasiphae (17.7mag)
07:57:35.29 +21:26:31.2 Carme (18.9mag)
00:50:19.21 +02:53:07.8 Titan (8.6mag)
00:50:20.74 +02:53:37.1 Rhea (9.9mag)
00:50:45.92 +02:55:56.9 Iapetus (11.3mag)
00:50:24.11 +02:53:01.8 Hyperion (14.6mag)
00:50:54.50 +02:55:00.3 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 11 06:00 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461202.92271319:
17:26:30.94 -35:28:32.7 JWST
16:44:56.40 +45:12:19.1 Chandra
09:57:40.17 -56:18:08.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 11 06:00 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461202.92271319 -observatory V36
18:41:13.45 -32:53:07.3 13.6mag P/2010 H2 (Vales)
05:56:39.63 -68:02:02.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:50:15.10 +32:00:38.3 17.5mag C/2017 K2 (PANSTARRS)
17:13:26.22 +15:30:16.9 17.8mag C/2021 G2 (ATLAS)
21:42:55.21 -47:27:55.6 16.6mag P/2021 N1 (ZTF)
23:11:51.94 +31:42:42.5 17.2mag C/2022 E2 (ATLAS)
05:37:59.90 +26:59:31.7 16.5mag C/2022 N2 (PANSTARRS)
09:32:04.75 +30:58:03.9 16.7mag C/2022 QE78 (ATLAS)
08:52:17.93 +04:04:55.3 17.7mag C/2022 R6 (PANSTARRS)
18:26:06.27 +21:39:19.4 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:18:14.49 -11:00:58.6 17.6mag P/2023 B1 (PANSTARRS)
22:13:13.76 +66:43:17.1 17.8mag C/2023 H5 (Lemmon)
17:38:22.52 -07:00:32.6 13.7mag C/2023 R1 (PANSTARRS)
13:16:53.87 +82:15:07.1 18.0mag C/2023 X2 (Lemmon)
07:14:57.34 +64:25:13.3 17.7mag C/2024 A1 (ATLAS)
06:52:08.79 +28:06:55.5 13.7mag C/2024 E1 (Wierzchos)
15:34:47.15 +13:47:56.8 17.4mag C/2024 G6 (ATLAS)
20:10:48.28 +32:05:22.8 14.0mag C/2024 J3 (ATLAS)
04:21:15.89 -15:40:25.9 16.0mag C/2024 T5 (ATLAS)
06:08:55.20 +33:55:56.4 17.9mag C/2025 J1 (Borisov)
11:33:34.27 +52:33:33.7 17.5mag C/2025 L1 (ATLAS)
06:48:45.46 -11:01:06.5 14.4mag C/2025 R3 (PANSTARRS)
09:26:51.62 +23:17:34.2 17.9mag C/2025 V2 (Rankin)
12:39:40.54 +04:40:26.1 17.2mag C/2025 Y1 (ATLAS)
18:07:24.97 +75:48:31.3 17.8mag C/2026 A2 (Bok)
02:06:11.74 +43:38:28.2 16.1mag C/2026 B2 (Sun-Gao)
11:12:03.45 -02:37:41.6 16.5mag A/2026 E1
20:29:29.36 -08:49:53.4 8.6mag 10P/Tempel
11:02:48.08 -01:01:06.1 16.0mag 29P/Schwassmann-Wachmann
03:16:42.89 +26:04:28.1 17.7mag 47P/Ashbrook-Jackson
09:06:52.18 +22:50:27.2 16.9mag 63P/Wild
00:29:39.12 -06:09:59.6 15.7mag 65P/Gunn
06:53:55.52 +33:43:50.8 17.0mag 76P/West-Kohoutek-Ikemura
03:16:59.93 +17:37:09.1 13.8mag 78P/Gehrels
01:27:42.18 +05:32:26.2 15.6mag 88P/Howell
05:05:02.40 +30:31:28.7 15.3mag 93P/Lovas
02:52:09.47 +28:07:53.0 17.5mag 114P/Wiseman-Skiff
06:58:16.30 +32:54:37.2 15.6mag 123P/West-Hartley
09:55:48.99 +13:15:25.8 16.5mag 124P/Mrkos
04:04:22.05 +19:27:40.1 16.3mag 128P/Shoemaker-Holt
04:39:59.01 +19:13:28.9 17.7mag 131P/Mueller
06:11:58.25 +18:16:08.6 15.1mag 141P/Machholz
06:14:47.31 +17:48:47.8 15.0mag 141P-A/Machholz
05:10:12.66 +16:34:44.2 11.9mag 141P-D/Machholz
02:59:56.27 -24:15:34.9 16.7mag 161P/Hartley-IRAS
03:52:13.51 +25:04:53.6 15.0mag 162P/SidingSpring
19:36:11.22 +02:42:17.8 16.7mag 169P/NEAT
00:27:00.67 +03:05:24.1 17.8mag 220P/McNaught
16:49:44.96 -08:19:56.4 16.4mag 235P/LINEAR
07:41:56.90 +35:20:54.2 17.6mag 240P/NEAT
00:40:50.65 -01:05:12.0 16.3mag 260P/McNaught
04:13:03.52 +33:03:21.5 17.5mag 295P/LINEAR
00:11:48.41 -05:44:36.9 17.7mag 320P/McNaught
15:13:49.75 +07:58:45.2 17.4mag 391P/Kowalski
08:09:43.80 +20:39:42.1 17.9mag 450P/LONEOS
07:05:14.46 +41:27:54.6 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 11 06:00 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
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -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
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -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
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
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 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
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
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
-rw-r--r-- 1 apache apache 5.6K Jun 11 06:00 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 11 06:00 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:40:17.448 +69:47:55.79 AT 2026oeo 2026-04-20.43 20.7564
16:51:55.641 +43:49:10.27 AT 2026oen 2026-06-01.32 20.1057
14:26:49.759 +08:51:50.81 AT 2026oem 2026-05-23.34 20.9956
16:33:33.092 +12:48:11.76 AT 2026oel 2026-05-24.31 20.322
14:42:53.361 +09:25:56.12 AT 2026oek 2026-05-31.21 19.7393
16:12:09.163 +29:54:51.29 AT 2026oej 2026-05-25.37 21.1198
16:32:31.727 +65:39:51.90 AT 2026oei 2026-05-23.32 20.7631
16:04:39.925 -21:36:56.05 AT 2026oeh 2026-05-21.40 20.1751
15:27:47.338 +38:55:13.31 AT 2026oeg 2026-05-21.97 19.64
14:51:39.615 +45:21:56.05 AT 2026oef 2026-05-28.95 19.09
10:32:49.111 +46:46:00.48 AT 2026oee 2026-06-03.89 19.348
17:25:39.755 +21:57:18.90 SN 2026oed 2026-05-31.37 19.4457
09:59:38.199 +00:31:00.31 AT 2026oec 2026-05-30.97 22.39
09:27:53.984 +22:21:00.63 AT 2026oeb 2026-06-01.17 18.66
09:22:28.890 +11:30:25.73 AT 2026oea 2026-06-04.18 19.4125
12:42:23.918 -13:22:38.30 AT 2026odz 2026-06-02.21 20.0149
09:58:40.601 +01:27:22.46 AT 2026ody 2026-05-29.04 21.94
14:57:09.055 +33:12:55.31 AT 2026odx 2026-05-28.93 19.3
13:30:34.211 +08:18:17.60 AT 2026odw 2026-06-02.93 19.81
22:05:04.941 -08:18:56.22 SN 2026odv 2026-06-03.15 18.492
-rw-r--r-- 1 apache apache 30K Jun 11 06:00 tns_transients_list.txt
