This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 10.22 22:09:04.57 +61:10:20.7
104.59649 4.22095 galactic Cep Second-epoch detections are separated by 0.2" and 3.4 pix
The object was found in VSX 1" ASASSN-V J220904.56+611021.5
Type: SR
# Max. Min./Amp. JD0 Period
11.450 V 12.030 V 2458326.31080 88.951569200000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:09:04.57 +61:10:20.7: 11.24 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:09:04.57 +61:10:20.7: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220904.56+611021.5,2461186.7241,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220904.56+611021.5 20260526.2241 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 10.50 22:33:37.32 +63:35:08.5
108.30495 4.69849 galactic Cep Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX 1" V0686 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
11.500 V 12.000 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:33:37.32 +63:35:08.5: 11.46 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:33:37.32 +63:35:08.5: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0686 Cep,2461186.7241,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0686 Cep 20260526.2241 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 10.45 22:37:17.45 +63:57:16.3
108.84219 4.81562 galactic Cep Second-epoch detections are separated by 0.6" and 3.2 pix
The object was found in VSX 2" V1235 Cep
Type: SRB
# Max. Min./Amp. JD0 Period
12.000 V 12.780 V 50.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:37:17.45 +63:57:16.3: 11.49 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:37:17.45 +63:57:16.3: 11.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1235 Cep,2461186.7241,10.45,0.05,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
V1235 Cep 20260526.2241 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 10.46 22:12:56.08 +59:46:48.9
104.18506 2.80838 galactic Cep Second-epoch detections are separated by 0.7" and 3.5 pix
The object was found in VSX 1" V0651 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
11.300 V 12.300 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:12:56.08 +59:46:48.9: 11.49 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:12:56.08 +59:46:48.9: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0651 Cep,2461186.7241,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0651 Cep 20260526.2241 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 10.35 22:05:57.91 +60:59:53.5
104.18848 4.29977 galactic Cep Second-epoch detections are separated by 0.5" and 3.5 pix
The object was found in VSX 1" V0640 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
11.800 V 12.900 V 293.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:05:57.91 +60:59:53.5: 11.61 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:05:57.91 +60:59:53.5: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0640 Cep,2461186.7241,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0640 Cep 20260526.2241 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.26 21:55:24.77 +59:38:37.7
102.32439 4.01171 galactic Cep Second-epoch detections are separated by 2.0" and 3.7 pix
The object was found in VSX 1" Gaia DR3 2202731225377480064
Type: L
# Max. Min./Amp. JD0 Period
12.170 G 13.020 G M
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:55:24.77 +59:38:37.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:55:24.77 +59:38:37.7: 13.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2202731225377480064,2461186.7241,12.26,0.05,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 2202731225377480064 20260526.2241 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.40 21:59:39.48 +60:23:13.2
103.20161 4.27269 galactic Cep Second-epoch detections are separated by 3.7" and 3.6 pix
The object was found in VSX 2" ZTF J215939.53+602314.7
Type: SR
# Max. Min./Amp. JD0 Period
12.731 r Y 0.094 r 2458332.87080 28.756454800000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:59:39.48 +60:23:13.2: 13.47 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:59:39.48 +60:23:13.2: 13.31 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J215939.53+602314.7,2461186.7241,12.40,0.05,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
ZTF J215939.53+602314.7 20260526.2241 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.47 22:01:44.63 +60:21:40.2
103.39174 4.09617 galactic Cep Second-epoch detections are separated by 2.0" and 3.5 pix
The object was found in VSX 0" V1177 Cep
Type: SRB
# Max. Min./Amp. JD0 Period
14.470 V 15.820 V 139.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:01:44.63 +60:21:40.2: 13.92 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:01:44.63 +60:21:40.2: 13.94 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.93 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1177 Cep,2461186.7241,12.47,0.05,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
V1177 Cep 20260526.2241 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.58 22:32:31.53 +63:34:54.0
108.19742 4.75684 galactic Cep Second-epoch detections are separated by 2.0" and 3.6 pix
The object was found in VSX 3" ASASSN-V J223231.62+633457.4
Type: SR
# Max. Min./Amp. JD0 Period
14.100 V 14.300 V 2457263.94600 33.550000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:32:31.53 +63:34:54.0: 13.66 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:32:31.53 +63:34:54.0: 13.42 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J223231.62+633457.4,2461186.7241,12.58,0.05,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
ASASSN-V J223231.62+633457.4 20260526.2241 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.22 22:47:21.63 +64:15:53.9
109.96007 4.56429 galactic Cep Second-epoch detections are separated by 0.9" and 3.2 pix
The object was found in VSX 2" ASASSN-V J224721.83+641555.0
Type: SR
# Max. Min./Amp. JD0 Period
13.710 V 13.890 V 2457988.99500 51.490000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:47:21.63 +64:15:53.9: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:47:21.63 +64:15:53.9: 13.29 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J224721.83+641555.0,2461186.7241,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J224721.83+641555.0 20260526.2241 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.53 22:18:00.45 +62:36:55.8
106.28663 4.81200 galactic Cep Second-epoch detections are separated by 1.3" and 3.2 pix
The object was found in VSX 1" V0657 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
12.500 V 13.200 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:18:00.45 +62:36:55.8: 12.59 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:18:00.45 +62:36:55.8: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0657 Cep,2461186.7241,11.53,0.05,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
V0657 Cep 20260526.2241 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 05 26.2241 2461186.7241 11.58 22:11:18.94 +60:13:25.6
104.27221 3.28806 galactic Cep Second-epoch detections are separated by 0.7" and 3.4 pix
The object was found in VSX 2" ASASSN-V J221119.02+601327.9
Type: SRS
# Max. Min./Amp. JD0 Period
14.010 g Y 0.240 g 2459427.81100 28.776000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:11:18.94 +60:13:25.6: 12.58 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:11:18.94 +60:13:25.6: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221119.02+601327.9,2461186.7241,11.58,0.05,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
ASASSN-V J221119.02+601327.9 20260526.2241 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.29 22:36:20.36 +65:08:49.5
109.34641 5.90218 galactic Cep Second-epoch detections are separated by 0.8" and 2.9 pix
The object was found in VSX 2" NSVS 3506924
Type: L
# Max. Min./Amp. JD0 Period
11.400 R1 11.700 R1
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:36:20.36 +65:08:49.5: 13.51 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:36:20.36 +65:08:49.5: 13.45 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3506924,2461186.7241,12.29,0.05,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
NSVS 3506924 20260526.2241 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.48 22:15:20.50 +60:25:22.1
104.79632 3.16924 galactic Cep Second-epoch detections are separated by 0.8" and 3.6 pix
The object was found in VSX 2" ASASSN-V J221520.49+602523.6
Type: SRS
# Max. Min./Amp. JD0 Period
14.110 V 14.220 V 2457164.08600 14.716000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:15:20.50 +60:25:22.1: 13.55 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:15:20.50 +60:25:22.1: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221520.49+602523.6,2461186.7241,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221520.49+602523.6 20260526.2241 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.72 22:18:21.42 +60:49:19.4
105.32662 3.29503 galactic Cep Second-epoch detections are separated by 1.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:18:21.42 +60:49:19.4 (user input) | T | P | (position from user input) J-Ks=1.433+/-0.038 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:18:21.42 +60:49:19.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:18:21.42 +60:49:19.4: 13.61 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461186.7241,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260526.2241 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.24 22:06:46.19 +57:31:20.7
102.22589 1.42745 galactic Cep Second-epoch detections are separated by 0.8" and 3.8 pix
The object was found in VSX 1" ASASSN-V J220646.22+573121.6
Type: SR
# Max. Min./Amp. JD0 Period
14.850 g Y 0.260 g 2459200.66600 71.660000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:06:46.19 +57:31:20.7: 13.25 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:06:46.19 +57:31:20.7: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220646.22+573121.6,2461186.7241,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220646.22+573121.6 20260526.2241 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.38 21:33:16.40 +63:57:12.3
103.16187 8.97973 galactic Cep Second-epoch detections are separated by 0.9" and 3.2 pix
The object was found in VSX 5" NSVS J2133166+635717
Type: L:
# Max. Min./Amp. JD0 Period
10.994 R1 Y 0.795 R1 228.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:33:16.40 +63:57:12.3: 13.39 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:33:16.40 +63:57:12.3: 13.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2133166+635717,2461186.7241,12.38,0.05,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
NSVS J2133166+635717 20260526.2241 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.21 21:58:25.50 +60:17:16.9
103.01985 4.28727 galactic Cep Second-epoch detections are separated by 0.8" and 3.7 pix
The object was found in VSX 5" V0620 Cep
Type: SRS:
# Max. Min./Amp. JD0 Period
12.600 V 13.300 V 29.800000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:58:25.50 +60:17:16.9: 12.32 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:58:25.50 +60:17:16.9: 12.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0620 Cep,2461186.7241,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0620 Cep 20260526.2241 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.45 22:05:04.48 +59:50:31.7
103.41501 3.43200 galactic Cep Second-epoch detections are separated by 0.7" and 3.6 pix
The object was found in VSX 3" ASASSN-V J220504.60+595034.4
Type: SR
# Max. Min./Amp. JD0 Period
13.840 V 14.730 V 2458384.38650 169.003465400000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:05:04.48 +59:50:31.7: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:05:04.48 +59:50:31.7: 13.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220504.60+595034.4,2461186.7241,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220504.60+595034.4 20260526.2241 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.29 22:31:29.28 +62:26:42.0
107.51444 3.83922 galactic Cep Second-epoch detections are separated by 0.6" and 3.4 pix
The object was found in VSX 2" ASASSN-V J223129.24+622643.7
Type: SR
# Max. Min./Amp. JD0 Period
13.960 V 14.340 V 2458489.14140 227.689905400000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:31:29.28 +62:26:42.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:31:29.28 +62:26:42.0: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J223129.24+622643.7,2461186.7241,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J223129.24+622643.7 20260526.2241 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.42 22:14:31.15 +60:01:13.2
104.48509 2.89389 galactic Cep Second-epoch detections are separated by 0.9" and 3.7 pix
The object was found in VSX 2" ASASSN-V J221431.28+600114.9
Type: SRS
# Max. Min./Amp. JD0 Period
13.800 V 13.910 V 2457139.11800 22.326000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:14:31.15 +60:01:13.2: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:14:31.15 +60:01:13.2: 13.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221431.28+600114.9,2461186.7241,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221431.28+600114.9 20260526.2241 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.68 22:51:04.01 +64:16:22.2
110.32321 4.38873 galactic Cep Second-epoch detections are separated by 3.5" and 3.2 pix
The object was found in VSX 2" ASASSN-V J225104.13+641623.5
Type: L:
# Max. Min./Amp. JD0 Period
14.020 V 14.650 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:51:04.01 +64:16:22.2: 14.01 +/- 0.07 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:51:04.01 +64:16:22.2: 13.88 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J225104.13+641623.5,2461186.7241,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J225104.13+641623.5 20260526.2241 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.16 22:37:40.37 +65:03:02.7
109.42104 5.74898 galactic Cep Second-epoch detections are separated by 0.5" and 3.1 pix
The object was found in VSX 2" ASASSN-V J223740.43+650304.2
Type: SR
# Max. Min./Amp. JD0 Period
13.530 V 14.700 V 2457012.70000 422.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:37:40.37 +65:03:02.7: 13.05 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:37:40.37 +65:03:02.7: 13.32 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J223740.43+650304.2,2461186.7241,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J223740.43+650304.2 20260526.2241 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.01 22:24:21.64 +62:02:45.3
106.59639 3.93283 galactic Cep Second-epoch detections are separated by 0.7" 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 2204704986186576256 | 22:24:21.60 +62:02:47.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.533+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:24:21.64 +62:02:45.3: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:24:21.64 +62:02:45.3: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2204704986186576256,2461186.7241,12.01,0.05,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
Large-amplitude variable Gaia DR2 2204704986186576256 20260526.2241 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.35 22:05:12.92 +58:20:37.8
102.54255 2.21301 galactic Cep Second-epoch detections are separated by 0.5" and 3.8 pix
The object was found in VSX 1" ZTF J220512.96+582038.4
Type: SR
# Max. Min./Amp. JD0 Period
12.970 r Y 0.159 r 2458637.00230 34.812889600000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:05:12.92 +58:20:37.8: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:05:12.92 +58:20:37.8: 13.42 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.59 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220512.96+582038.4,2461186.7241,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J220512.96+582038.4 20260526.2241 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.30 22:00:38.03 +58:07:05.2
101.92363 2.39231 galactic Cep Second-epoch detections are separated by 1.4" and 3.6 pix
The object was found in VSX 2" NSVS J2200379+580703
Type: SR
# Max. Min./Amp. JD0 Period
13.483 r Y 0.452 r 2458369.99090 156.969430600000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:00:38.03 +58:07:05.2: 13.72 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:00:38.03 +58:07:05.2: 13.53 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2200379+580703,2461186.7241,12.30,0.05,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
NSVS J2200379+580703 20260526.2241 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.40 22:40:33.48 +63:24:37.2
108.89293 4.16393 galactic Cep Second-epoch detections are separated by 0.6" and 3.2 pix
The object was found in VSX 1" ASASSN-V J224033.47+632438.1
Type: SRS
# Max. Min./Amp. JD0 Period
14.950 g Y 0.300 g 2459362.01000 28.199000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:40:33.48 +63:24:37.2: 13.48 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:40:33.48 +63:24:37.2: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J224033.47+632438.1,2461186.7241,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J224033.47+632438.1 20260526.2241 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.45 22:07:11.97 +62:00:37.4
104.90542 5.03162 galactic Cep Second-epoch detections are separated by 2.1" and 3.4 pix
The object was found in VSX14" Gaia DR3 2204887745644472320
Type: YSO
# Max. Min./Amp. JD0 Period
16.560 G 16.810 G M
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:07:11.97 +62:00:37.4: 13.47 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:07:11.97 +62:00:37.4: 13.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2204887745644472320,2461186.7241,12.45,0.05,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 2204887745644472320 20260526.2241 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.22 22:02:46.47 +58:09:24.7
102.17292 2.25350 galactic Cep Second-epoch detections are separated by 1.1" and 3.8 pix
The object was found in VSX 1" ASASSN-V J220246.54+580924.4
Type: SR
# Max. Min./Amp. JD0 Period
14.260 V 14.970 V 2458421.31940 301.151128500000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:02:46.47 +58:09:24.7: 13.43 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:02:46.47 +58:09:24.7: 13.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.41 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220246.54+580924.4,2461186.7241,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220246.54+580924.4 20260526.2241 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.31 22:21:24.90 +61:21:31.7
105.93083 3.54181 galactic Cep Second-epoch detections are separated by 1.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2201656654620000640 | 22:21:25.02 +61:21:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.612+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:21:24.90 +61:21:31.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:21:24.90 +61:21:31.7: 13.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.25 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2201656654620000640,2461186.7241,12.31,0.05,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 2201656654620000640 20260526.2241 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.40 22:09:28.28 +59:37:57.4
103.74204 2.93791 galactic Cep Second-epoch detections are separated by 7.8" and 4.2 pix
The object was found in VSX 9" ZTF J220928.77+593805.0
Type: SR
# Max. Min./Amp. JD0 Period
15.388 g Y 0.232 g 2458307.57200 91.389549900000 C
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:09:28.28 +59:37:57.4: 13.61 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:09:28.28 +59:37:57.4: 13.60 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.61 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220928.77+593805.0,2461186.7241,12.40,0.05,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
ZTF J220928.77+593805.0 20260526.2241 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.64 22:21:01.21 +60:27:28.3
105.40023 2.81152 galactic Cep Second-epoch detections are separated by 0.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.2559+60.4583 | 22:21:01.40 +60:27:29.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.767+/-0.046 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:21:01.21 +60:27:28.3: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:21:01.21 +60:27:28.3: 13.76 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.87 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J335.2559+60.4583,2461186.7241,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.2559+60.4583 20260526.2241 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.28 21:54:36.75 +66:45:22.7
106.72593 9.62519 galactic Cep Second-epoch detections are separated by 2.9" and 2.9 pix
The object was found in VSX 2" V0602 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
13.600 V 14.300 V 213.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:54:36.75 +66:45:22.7: 13.45 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:54:36.75 +66:45:22.7: 13.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0602 Cep,2461186.7241,12.28,0.05,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
V0602 Cep 20260526.2241 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.45 22:20:03.44 +62:14:56.1
106.28258 4.37541 galactic Cep Second-epoch detections are separated by 1.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2204777618375529216 | 22:20:03.47 +62:14:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.853+/-0.047 (Very red!)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:20:03.44 +62:14:56.1: 13.60 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:20:03.44 +62:14:56.1: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.59 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2204777618375529216,2461186.7241,12.45,0.05,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 2204777618375529216 20260526.2241 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.47 22:01:58.12 +60:50:05.0
103.69960 4.45779 galactic Cep Second-epoch detections are separated by 1.3" and 3.7 pix
The object was found in VSX 3" V1179 Cep
Type: SRB
# Max. Min./Amp. JD0 Period
14.600 g 15.130 g 2457139.12000 37.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:01:58.12 +60:50:05.0: 13.60 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:01:58.12 +60:50:05.0: 13.44 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1179 Cep,2461186.7241,12.47,0.05,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
V1179 Cep 20260526.2241 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.28 21:57:04.34 +59:06:16.8
102.15750 3.45709 galactic Cep Second-epoch detections are separated by 0.7" and 3.6 pix
The object was found in VSX 1" NSVS J2157042+590615
Type: SR
# Max. Min./Amp. JD0 Period
12.207 r Y 0.418 r 2458246.95780 85.866663800000 M6
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:57:04.34 +59:06:16.8: 12.42 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:57:04.34 +59:06:16.8: 12.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2157042+590615,2461186.7241,11.28,0.05,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
NSVS J2157042+590615 20260526.2241 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 05 26.2241 2461186.7241 12.65 22:19:07.84 +60:55:50.0
105.46519 3.33371 galactic Cep Second-epoch detections are separated by 1.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:07.84 +60:55:50.0 (user input) | T | P | (position from user input) J-Ks=1.483+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:19:07.84 +60:55:50.0: 13.75 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:19:07.84 +60:55:50.0: 13.56 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461186.7241,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260526.2241 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.42 22:25:24.93 +61:18:04.5
106.30549 3.23577 galactic Cep Second-epoch detections are separated by 1.9" and 3.5 pix
The object was found in VSX16" Gaia DR3 2201619619126733568
Type: YSO
# Max. Min./Amp. JD0 Period
15.570 G 15.600 G G
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:25:24.93 +61:18:04.5: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:25:24.93 +61:18:04.5: 13.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2201619619126733568,2461186.7241,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2201619619126733568 20260526.2241 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.35 21:35:41.80 +57:48:44.3
99.18152 4.27058 galactic Cep Second-epoch detections are separated by 3.1" and 4.4 pix
The object was found in VSX 4" NSVS J2135411+574839
Type: SR
# Max. Min./Amp. JD0 Period
16.973 g Y 0.320 g 2458435.15630 227.729570400000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:35:41.80 +57:48:44.3: 13.44 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:35:41.80 +57:48:44.3: 13.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.41 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2135411+574839,2461186.7241,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2135411+574839 20260526.2241 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.91 21:46:57.24 +59:34:47.8
101.45242 4.63805 galactic Cep Second-epoch detections are separated by 1.2" and 3.6 pix
The object was found in VSX 1" V0590 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
13.600 V 14.200 V 140.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:46:57.24 +59:34:47.8: 13.00 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:46:57.24 +59:34:47.8: 12.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0590 Cep,2461186.7241,11.91,0.05,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
V0590 Cep 20260526.2241 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.61 21:55:19.04 +60:10:45.0
102.64788 4.43912 galactic Cep Second-epoch detections are separated by 2.0" and 3.5 pix
The object was found in VSX 1" V1145 Cep
Type: SRB
# Max. Min./Amp. JD0 Period
14.740 g 16.290 g 65.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:55:19.04 +60:10:45.0: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:55:19.04 +60:10:45.0: 13.67 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.80 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1145 Cep,2461186.7241,12.61,0.05,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
V1145 Cep 20260526.2241 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.71 22:07:55.35 +61:54:25.6
104.91383 4.89814 galactic Cep Second-epoch detections are separated by 0.8" and 3.2 pix
The object was found in VSX 2" ASASSN-V J220755.22+615427.6
Type: SRS
# Max. Min./Amp. JD0 Period
15.580 g Y 0.370 g 2459479.73800 27.124000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:07:55.35 +61:54:25.6: 14.14 +/- 0.06 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:07:55.35 +61:54:25.6: 14.04 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.12 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220755.22+615427.6,2461186.7241,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220755.22+615427.6 20260526.2241 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.73 22:37:48.63 +63:15:40.3
108.55017 4.18372 galactic Cep Second-epoch detections are separated by 0.3" and 3.2 pix
The object was found in VSX 1" V0692 Cep
Type: SRB:
# Max. Min./Amp. JD0 Period
12.800 V 13.700 V 78.700000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:37:48.63 +63:15:40.3: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:37:48.63 +63:15:40.3: 12.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0692 Cep,2461186.7241,11.73,0.05,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
V0692 Cep 20260526.2241 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.35 22:09:47.47 +61:09:35.2
104.65958 4.16069 galactic Cep Second-epoch detections are separated by 0.2" and 3.4 pix
The object was found in VSX 1" V0649 Cep
Type: SR
# Max. Min./Amp. JD0 Period
12.400 V 13.200 V 2451438.00000 75.900000000000 MS
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:09:47.47 +61:09:35.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:09:47.47 +61:09:35.2: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0649 Cep,2461186.7241,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0649 Cep 20260526.2241 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.41 21:45:11.06 +57:48:03.6
100.12523 3.42775 galactic Cep Second-epoch detections are separated by 1.0" and 3.7 pix
The object was found in VSX 1" V0581 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
12.700 V 13.400 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:45:11.06 +57:48:03.6: 12.36 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:45:11.06 +57:48:03.6: 12.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0581 Cep,2461186.7241,11.41,0.05,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
V0581 Cep 20260526.2241 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 05 26.2241 2461186.7241 11.87 23:08:21.84 +65:45:41.0
112.61162 4.97642 galactic Cep Second-epoch detections are separated by 1.6" and 3.3 pix
The object was found in VSX 3" NSVS J2308218+654557
Type: SR
# Max. Min./Amp. JD0 Period
13.107 r Y 0.394 r 2458324.97380 129.762802300000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 23:08:21.84 +65:45:41.0: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 23:08:21.84 +65:45:41.0: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.36 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2308218+654557,2461186.7241,11.87,0.05,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 J2308218+654557 20260526.2241 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.10 22:45:34.10 +64:14:38.4
109.77728 4.63583 galactic Cep Second-epoch detections are separated by 0.8" and 3.0 pix
The object was found in VSX 3" ASASSN-V J224534.15+641441.3
Type: SR
# Max. Min./Amp. JD0 Period
13.770 V 13.970 V 2457513.00000 366.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:45:34.10 +64:14:38.4: 13.24 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:45:34.10 +64:14:38.4: 13.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J224534.15+641441.3,2461186.7241,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J224534.15+641441.3 20260526.2241 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.35 22:01:13.94 +60:31:19.0
103.43844 4.26248 galactic Cep Second-epoch detections are separated by 3.4" and 3.9 pix
The object was found in VSX 3" V1174 Cep
Type: SRB
# Max. Min./Amp. JD0 Period
13.960 V 14.780 V 53.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:01:13.94 +60:31:19.0: 13.57 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:01:13.94 +60:31:19.0: 13.48 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1174 Cep,2461186.7241,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1174 Cep 20260526.2241 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.52 22:12:30.98 +59:33:40.8
104.01690 2.65838 galactic Cep Second-epoch detections are separated by 1.2" and 3.5 pix
The object was found in VSX 2" ASASSN-V J221230.99+593343.1
Type: L
# Max. Min./Amp. JD0 Period
14.150 V 14.290 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:12:30.98 +59:33:40.8: 13.60 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:12:30.98 +59:33:40.8: 13.43 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221230.99+593343.1,2461186.7241,12.52,0.05,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
ASASSN-V J221230.99+593343.1 20260526.2241 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.33 21:42:26.21 +57:22:28.6
99.56721 3.34380 galactic Cep Second-epoch detections are separated by 1.8" and 3.7 pix
The object was found in VSX 1" NSVS 3411613
Type: SR
# Max. Min./Amp. JD0 Period
13.394 r Y 0.400 R1 2458273.96940 67.457684800000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:42:26.21 +57:22:28.6: 13.58 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:42:26.21 +57:22:28.6: 13.52 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3411613,2461186.7241,12.33,0.05,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
NSVS 3411613 20260526.2241 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.59 22:29:50.20 +65:19:21.9
108.84628 6.39950 galactic Cep Second-epoch detections are separated by 1.1" and 2.8 pix
The object was found in VSX 1" V0680 Cep
Type: SR
# Max. Min./Amp. JD0 Period
13.400 V 14.700 V 2451344.00000 118.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:29:50.20 +65:19:21.9: 13.76 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:29:50.20 +65:19:21.9: 13.70 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0680 Cep,2461186.7241,12.59,0.05,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
V0680 Cep 20260526.2241 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.90 22:33:25.13 +63:13:00.9
108.09829 4.39177 galactic Cep Second-epoch detections are separated by 0.9" and 3.2 pix
The object was found in VSX 1" ASASSN-V J223325.19+631301.8
Type: SR
# Max. Min./Amp. JD0 Period
14.700 g Y 0.180 g 2458597.11100 124.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:33:25.13 +63:13:00.9: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:33:25.13 +63:13:00.9: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J223325.19+631301.8,2461186.7241,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J223325.19+631301.8 20260526.2241 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.86 22:17:40.07 +60:49:17.2
105.25619 3.34099 galactic Cep Second-epoch detections are separated by 2.2" and 3.5 pix
The object was found in VSX 4" ZTF J221740.15+604920.9
Type: SR
# Max. Min./Amp. JD0 Period
13.285 r Y 0.227 r 2458382.82740 50.600484000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:17:40.07 +60:49:17.2: 14.01 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:17:40.07 +60:49:17.2: 14.11 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.02 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221740.15+604920.9,2461186.7241,12.86,0.05,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 J221740.15+604920.9 20260526.2241 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.54 22:19:14.01 +61:22:38.1
105.72160 3.70003 galactic Cep Second-epoch detections are separated by 1.3" and 3.2 pix
The object was found in VSX 2" ASASSN-V J221914.07+612239.7
Type: SR
# Max. Min./Amp. JD0 Period
13.250 V 13.610 V 2458426.79620 66.555437200000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:19:14.01 +61:22:38.1: 12.71 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:19:14.01 +61:22:38.1: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221914.07+612239.7,2461186.7241,11.54,0.05,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
ASASSN-V J221914.07+612239.7 20260526.2241 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 05 26.2241 2461186.7241 12.51 22:14:03.95 +59:56:21.5
104.39244 2.85899 galactic Cep Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.5152+59.9368 | 22:14:03.95 +59:56:21.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:14:03.95 +59:56:21.5: 13.60 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:14:03.95 +59:56:21.5: 13.45 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.57 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J333.5152+59.9368,2461186.7241,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.5152+59.9368 20260526.2241 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.89 22:01:47.83 +61:17:28.4
103.95869 4.83480 galactic Cep Second-epoch detections are separated by 0.6" and 3.4 pix
The object was found in VSX 3" V0633 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
13.800 V 14.500 V 2451530.00000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:01:47.83 +61:17:28.4: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:01:47.83 +61:17:28.4: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0633 Cep,2461186.7241,11.89,0.05,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
V0633 Cep 20260526.2241 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.24 22:15:00.76 +61:24:10.8
105.31511 4.00248 galactic Cep Second-epoch detections are separated by 1.8" and 3.5 pix
The object was found in VSX 3" ASASSN-V J221500.78+612413.5
Type: L
# Max. Min./Amp. JD0 Period
13.990 V 14.150 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:15:00.76 +61:24:10.8: 13.20 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:15:00.76 +61:24:10.8: 13.34 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221500.78+612413.5,2461186.7241,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221500.78+612413.5 20260526.2241 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.45 21:42:33.40 +58:35:41.5
100.38006 4.25564 galactic Cep Second-epoch detections are separated by 1.3" and 3.8 pix
The object was found in VSX 2" ASASSN-V J214233.17+583542.4
Type: SR
# Max. Min./Amp. JD0 Period
14.320 V 14.650 V 2458367.83250 36.236868300000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:42:33.40 +58:35:41.5: 13.60 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:42:33.40 +58:35:41.5: 13.22 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J214233.17+583542.4,2461186.7241,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214233.17+583542.4 20260526.2241 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.45 22:16:55.71 +60:42:41.9
105.11991 3.29981 galactic Cep Second-epoch detections are separated by 1.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2201529145630918784 | 22:16:55.75 +60:42:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.583+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:16:55.71 +60:42:41.9: 13.58 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:16:55.71 +60:42:41.9: 13.60 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2201529145630918784,2461186.7241,12.45,0.05,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 2201529145630918784 20260526.2241 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.59 22:19:28.29 +62:36:52.6
106.42701 4.71833 galactic Cep Second-epoch detections are separated by 1.4" and 3.1 pix
The object was found in VSX 2" ASASSN-V J221928.40+623654.4
Type: SR
# Max. Min./Amp. JD0 Period
14.580 V 15.150 V 2458304.98650 86.145419800000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:19:28.29 +62:36:52.6: 13.76 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:19:28.29 +62:36:52.6: 13.72 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221928.40+623654.4,2461186.7241,12.59,0.05,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
ASASSN-V J221928.40+623654.4 20260526.2241 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.73 22:05:07.34 +60:24:12.0
103.75267 3.88081 galactic Cep Second-epoch detections are separated by 2.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2203043001350161920 | 22:05:07.49 +60:24:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:05:07.34 +60:24:12.0: 13.89 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:05:07.34 +60:24:12.0: 13.77 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.86 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2203043001350161920,2461186.7241,12.73,0.05,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 2203043001350161920 20260526.2241 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.48 22:00:43.14 +65:03:47.0
106.16004 7.90992 galactic Cep Second-epoch detections are separated by 1.7" and 2.9 pix
The object was found in VSX 2" V0631 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
13.900 V 14.500 V 72.300000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:00:43.14 +65:03:47.0: 13.36 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:00:43.14 +65:03:47.0: 13.58 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.39 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0631 Cep,2461186.7241,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0631 Cep 20260526.2241 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.23 22:14:56.09 +60:11:44.1
104.62674 3.00957 galactic Cep Second-epoch detections are separated by 0.7" and 3.7 pix
The object was found in VSX 2" ASASSN-V J221456.19+601145.7
Type: SRS
# Max. Min./Amp. JD0 Period
14.740 g Y 0.240 g 2458720.60600 24.975000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:14:56.09 +60:11:44.1: 13.19 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:14:56.09 +60:11:44.1: 13.06 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221456.19+601145.7,2461186.7241,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221456.19+601145.7 20260526.2241 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.12 22:03:52.81 +58:10:46.3
102.30357 2.18476 galactic Cep Second-epoch detections are separated by 0.6" and 3.8 pix
The object was found in VSX 1" ASASSN-V J220352.87+581047.0
Type: SRS
# Max. Min./Amp. JD0 Period
12.650 V 12.840 V 2457578.90000 28.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:03:52.81 +58:10:46.3: 12.21 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:03:52.81 +58:10:46.3: 11.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220352.87+581047.0,2461186.7241,11.12,0.05,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
ASASSN-V J220352.87+581047.0 20260526.2241 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 05 26.2241 2461186.7241 11.64 22:07:49.36 +60:47:25.6
104.24956 3.99898 galactic Cep Second-epoch detections are separated by 1.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2203089696228125056 | 22:07:49.40 +60:47:27.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.548+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:07:49.36 +60:47:25.6: 12.65 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:07:49.36 +60:47:25.6: 12.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2203089696228125056,2461186.7241,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2203089696228125056 20260526.2241 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.68 22:24:56.51 +61:38:33.6
106.43914 3.55509 galactic Cep Second-epoch detections are separated by 1.7" and 3.1 pix
The object was found in VSX 3" ASASSN-V J222456.55+613836.7
Type: SRS
# Max. Min./Amp. JD0 Period
14.150 V 14.250 V 2458062.84700 19.943000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:24:56.51 +61:38:33.6: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:24:56.51 +61:38:33.6: 13.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J222456.55+613836.7,2461186.7241,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J222456.55+613836.7 20260526.2241 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.60 22:18:41.17 +59:42:11.4
104.74300 2.33911 galactic Cep Second-epoch detections are separated by 1.0" and 3.6 pix
The object was found in VSX 2" ASASSN-V J221841.13+594213.5
Type: SRS:
# Max. Min./Amp. JD0 Period
15.420 g Y 0.410 g 2458874.55300 5.949600000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:18:41.17 +59:42:11.4: 13.69 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:18:41.17 +59:42:11.4: 13.66 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.68 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221841.13+594213.5,2461186.7241,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221841.13+594213.5 20260526.2241 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.27 22:02:27.88 +60:31:33.8
103.56232 4.17455 galactic Cep Second-epoch detections are separated by 0.7" and 3.6 pix
The object was found in VSX 3" ASASSN-V J220228.05+603136.0
Type: SR
# Max. Min./Amp. JD0 Period
14.650 g Y 0.230 g 2458318.91400 597.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:02:27.88 +60:31:33.8: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:02:27.88 +60:31:33.8: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220228.05+603136.0,2461186.7241,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220228.05+603136.0 20260526.2241 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.55 22:02:12.28 +59:04:10.5
102.66064 3.02887 galactic Cep Second-epoch detections are separated by 1.7" and 3.6 pix
The object was found in VSX 3" ZTF J220212.22+590413.0
Type: SR
# Max. Min./Amp. JD0 Period
12.820 r Y 0.096 r 2458345.76010 410.879509500000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:02:12.28 +59:04:10.5: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:02:12.28 +59:04:10.5: 13.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220212.22+590413.0,2461186.7241,12.55,0.05,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
ZTF J220212.22+590413.0 20260526.2241 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.61 21:58:55.88 +58:19:46.6
101.87369 2.69641 galactic Cep Second-epoch detections are separated by 0.5" and 3.6 pix
The object was found in VSX 1" V0622 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
13.000 V 13.500 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:58:55.88 +58:19:46.6: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:58:55.88 +58:19:46.6: 12.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0622 Cep,2461186.7241,11.61,0.05,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
V0622 Cep 20260526.2241 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.18 21:33:08.41 +61:46:29.1
101.64432 7.40152 galactic Cep Second-epoch detections are separated by 0.3" and 3.4 pix
The object was found in VSX 1" V0486 Cep
Type: SRA
# Max. Min./Amp. JD0 Period
11.800 V 14.300 V 2450200.00000 248.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:33:08.41 +61:46:29.1: 12.16 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:33:08.41 +61:46:29.1: 11.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0486 Cep,2461186.7241,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0486 Cep 20260526.2241 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.19 22:03:43.61 +59:02:25.8
102.80033 2.88860 galactic Cep Second-epoch detections are separated by 0.7" and 3.6 pix
The object was found in VSX 1" V1102 Cep
Type: SRB
# Max. Min./Amp. JD0 Period
12.420 V 13.220 V 76.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:03:43.61 +59:02:25.8: 12.16 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:03:43.61 +59:02:25.8: 11.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1102 Cep,2461186.7241,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1102 Cep 20260526.2241 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.05 21:46:38.92 +58:36:51.9
100.79906 3.92440 galactic Cep Second-epoch detections are separated by 0.7" and 3.7 pix
The object was found in VSX 1" ASASSN-V J214638.86+583652.5
Type: SR
# Max. Min./Amp. JD0 Period
13.850 V 14.210 V 2458371.10690 199.897832800000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:46:38.92 +58:36:51.9: 13.24 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:46:38.92 +58:36:51.9: 13.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J214638.86+583652.5,2461186.7241,12.05,0.05,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
ASASSN-V J214638.86+583652.5 20260526.2241 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.51 21:51:10.35 +58:56:54.9
101.46519 3.80803 galactic Cep Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J327.7925+58.9494 | 21:51:10.21 +58:56:57.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:51:10.35 +58:56:54.9: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:51:10.35 +58:56:54.9: 13.26 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J327.7925+58.9494,2461186.7241,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J327.7925+58.9494 20260526.2241 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.68 22:08:21.81 +59:41:52.1
103.66586 3.07218 galactic Cep Second-epoch detections are separated by 4.3" and 3.0 pix
The object was found in VSX 2" ASASSN-V J220821.73+594153.6
Type: SRS
# Max. Min./Amp. JD0 Period
14.340 V 14.440 V 2457586.91000 25.405000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:08:21.81 +59:41:52.1: 13.93 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:08:21.81 +59:41:52.1: 13.66 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220821.73+594153.6,2461186.7241,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220821.73+594153.6 20260526.2241 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.55 22:16:22.62 +62:16:39.9
105.94080 4.63638 galactic Cep Second-epoch detections are separated by 1.9" and 3.6 pix
The object was found in VSX 3" NSVS J2216224+621645
Type: SR
# Max. Min./Amp. JD0 Period
15.532 g Y 0.526 g 2458635.02910 228.186410600000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:16:22.62 +62:16:39.9: 13.85 +/- 0.06 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:16:22.62 +62:16:39.9: 13.83 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2216224+621645,2461186.7241,12.55,0.05,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
NSVS J2216224+621645 20260526.2241 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.14 22:31:26.46 +62:54:57.0
107.75131 4.24651 galactic Cep Second-epoch detections are separated by 0.2" and 3.2 pix
The object was found in VSX 2" ASASSN-V J223126.53+625458.8
Type: SR
# Max. Min./Amp. JD0 Period
13.910 g Y 0.220 g 2459032.92500 35.670000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:31:26.46 +62:54:57.0: 12.11 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:31:26.46 +62:54:57.0: 11.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J223126.53+625458.8,2461186.7241,11.14,0.05,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
ASASSN-V J223126.53+625458.8 20260526.2241 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 05 26.2241 2461186.7241 12.29 21:55:24.82 +63:53:20.2
104.97596 7.33754 galactic Cep Second-epoch detections are separated by 0.8" and 3.2 pix
The object was found in VSX 2" V0606 Cep
Type: SR
# Max. Min./Amp. JD0 Period
13.000 V 13.700 V 2451323.00000 159.000000000000 C4/6
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:55:24.82 +63:53:20.2: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:55:24.82 +63:53:20.2: 13.25 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0606 Cep,2461186.7241,12.29,0.05,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
V0606 Cep 20260526.2241 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.39 22:21:29.15 +60:43:09.5
105.59046 3.00000 galactic Cep Second-epoch detections are separated by 0.8" and 3.6 pix
The object was found in VSX 3" V0662 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
13.100 V 13.800 V S
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:21:29.15 +60:43:09.5: 12.58 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:21:29.15 +60:43:09.5: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0662 Cep,2461186.7241,11.39,0.05,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
V0662 Cep 20260526.2241 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.89 22:02:22.60 +61:09:41.9
103.93638 4.68933 galactic Cep Second-epoch detections are separated by 0.0" and 3.5 pix
The object was found in VSX 2" ASASSN-V J220222.68+610943.8
Type: SR
# Max. Min./Amp. JD0 Period
14.470 g Y 0.140 g 2459333.06200
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:02:22.60 +61:09:41.9: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:02:22.60 +61:09:41.9: 12.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220222.68+610943.8,2461186.7241,11.89,0.05,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
ASASSN-V J220222.68+610943.8 20260526.2241 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.77 21:53:45.42 +59:05:56.7
101.81928 3.71638 galactic Cep Second-epoch detections are separated by 1.2" and 3.6 pix
The object was found in VSX 1" V1063 Cep
Type: LB
# Max. Min./Amp. JD0 Period
12.200 CR 12.550 CR
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:53:45.42 +59:05:56.7: 14.20 +/- 0.07 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:53:45.42 +59:05:56.7: 14.03 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.16 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1063 Cep,2461186.7241,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1063 Cep 20260526.2241 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.63 22:23:27.33 +61:46:07.8
106.35751 3.75584 galactic Cep Second-epoch detections are separated by 1.2" and 3.6 pix
The object was found in VSX 3" ASASSN-V J222327.53+614610.4
Type: SR
# Max. Min./Amp. JD0 Period
14.460 V 14.760 V 2457233.82800 71.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:23:27.33 +61:46:07.8: 13.94 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:23:27.33 +61:46:07.8: 13.78 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.90 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J222327.53+614610.4,2461186.7241,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J222327.53+614610.4 20260526.2241 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.92 22:45:34.16 +63:37:04.4
109.48481 4.08179 galactic Cep Second-epoch detections are separated by 0.4" and 3.1 pix
The object was found in VSX 3" ASASSN-V J224534.01+633706.8
Type: SR
# Max. Min./Amp. JD0 Period
15.174 g Y 0.599 g 2458276.98190 77.986648000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:45:34.16 +63:37:04.4: 13.16 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:45:34.16 +63:37:04.4: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J224534.01+633706.8,2461186.7241,11.92,0.05,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
ASASSN-V J224534.01+633706.8 20260526.2241 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.31 22:07:19.44 +60:19:26.7
103.92640 3.65651 galactic Cep Second-epoch detections are separated by 2.3" and 3.9 pix
The object was found in VSX 2" ZTF J220719.48+601928.3
Type: SR
# Max. Min./Amp. JD0 Period
12.854 r Y 0.304 r 2458344.05580 203.664821000000 C
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:07:19.44 +60:19:26.7: 13.32 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:07:19.44 +60:19:26.7: 13.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.31 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220719.48+601928.3,2461186.7241,12.31,0.05,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
ZTF J220719.48+601928.3 20260526.2241 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.98 23:29:30.89 +64:51:22.8
114.36750 3.35563 galactic Cep Second-epoch detections are separated by 0.6" and 3.1 pix
The object was found in VSX 6" NSVS 3539281
Type: SR
# Max. Min./Amp. JD0 Period
12.609 r Y 0.350 R1 2458374.81950 54.629055300000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 23:29:30.89 +64:51:22.8: 13.14 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 23:29:30.89 +64:51:22.8: 12.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3539281,2461186.7241,11.98,0.05,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
NSVS 3539281 20260526.2241 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 05 26.2241 2461186.7241 12.47 22:14:44.65 +60:55:33.5
105.01912 3.62648 galactic Cep Second-epoch detections are separated by 5.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2204528411499989504 | 22:14:42.67 +60:56:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:14:44.65 +60:55:33.5: 13.46 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:14:44.65 +60:55:33.5: 13.37 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2204528411499989504,2461186.7241,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2204528411499989504 20260526.2241 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.29 22:21:01.27 +59:55:03.8
105.10640 2.35810 galactic Cep Second-epoch detections are separated by 1.5" and 3.5 pix
The object was found in VSX 3" ASASSN-V J222101.21+595506.3
Type: SR
# Max. Min./Amp. JD0 Period
14.040 V 14.370 V 2457533.05000 73.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:21:01.27 +59:55:03.8: 13.48 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:21:01.27 +59:55:03.8: 13.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J222101.21+595506.3,2461186.7241,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J222101.21+595506.3 20260526.2241 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.40 22:06:33.76 +60:27:01.7
103.92436 3.81404 galactic Cep Second-epoch detections are separated by 2.1" and 3.5 pix
The object was found in VSX 2" ASASSN-V J220633.66+602703.6
Type: SR
# Max. Min./Amp. JD0 Period
14.100 V 14.560 V 2458347.84430 67.303028500000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:06:33.76 +60:27:01.7: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:06:33.76 +60:27:01.7: 13.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.48 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220633.66+602703.6,2461186.7241,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220633.66+602703.6 20260526.2241 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.59 21:57:24.82 +60:24:06.0
102.99060 4.45374 galactic Cep Second-epoch detections are separated by 6.6" and 3.2 pix
The object was found in VSX19" ZTF J215725.57+602424.0
Type: EW
# Max. Min./Amp. JD0 Period
20.214 r Y 0.564 r 2458382.81390 0.356370400000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:57:24.82 +60:24:06.0: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:57:24.82 +60:24:06.0: 13.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.54 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J215725.57+602424.0,2461186.7241,12.59,0.05,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 J215725.57+602424.0 20260526.2241 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.47 22:31:11.72 +62:18:44.1
107.41713 3.74255 galactic Cep Second-epoch detections are separated by 3.7" and 3.7 pix
The object was found in VSX23" ZTF J223114.28+621829.7
Type: EB:
# Max. Min./Amp. JD0 Period
15.352 r Y 0.111 r 2458271.94750 2.975253000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:31:11.72 +62:18:44.1: 13.53 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:31:11.72 +62:18:44.1: 13.43 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J223114.28+621829.7,2461186.7241,12.47,0.05,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
ZTF J223114.28+621829.7 20260526.2241 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.15 22:41:05.32 +64:16:04.3
109.35872 4.88723 galactic Cep 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 | Gaia DR3 2211353114528140672 | 22:41:05.48 +64:16:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.487+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:41:05.32 +64:16:04.3: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:41:05.32 +64:16:04.3: 13.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211353114528140672,2461186.7241,12.15,0.05,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 2211353114528140672 20260526.2241 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.72 21:52:39.15 +59:33:19.7
101.99551 4.16048 galactic Cep Second-epoch detections are separated by 2.0" and 3.2 pix
The object was found in VSX 3" ZTF J215238.90+593322.3
Type: SR
# Max. Min./Amp. JD0 Period
16.837 g Y 0.524 g 2458435.73690 232.158278300000 C:
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:52:39.15 +59:33:19.7: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:52:39.15 +59:33:19.7: 13.84 +/- 0.10 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J215238.90+593322.3,2461186.7241,12.72,0.05,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
ZTF J215238.90+593322.3 20260526.2241 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.55 22:14:47.28 +62:41:01.1
106.01719 5.07529 galactic Cep Second-epoch detections are separated by 1.1" and 3.4 pix
The object was found in VSX 2" ASASSN-V J221447.12+624102.3
Type: SR
# Max. Min./Amp. JD0 Period
14.480 V 15.210 V 2457945.00000 441.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:14:47.28 +62:41:01.1: 14.03 +/- 0.05 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:14:47.28 +62:41:01.1: 14.07 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.04 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221447.12+624102.3,2461186.7241,12.55,0.05,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 J221447.12+624102.3 20260526.2241 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.46 21:47:35.69 +58:56:18.4
101.10198 4.09387 galactic Cep Second-epoch detections are separated by 0.6" and 3.8 pix
The object was found in VSX 1" ASASSN-V J214735.64+585619.1
Type: SR
# Max. Min./Amp. JD0 Period
13.800 V 14.090 V 2457133.10000 45.120000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:47:35.69 +58:56:18.4: 13.47 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:47:35.69 +58:56:18.4: 13.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J214735.64+585619.1,2461186.7241,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214735.64+585619.1 20260526.2241 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.73 22:16:19.48 +63:14:09.8
106.47407 5.43401 galactic Cep Second-epoch detections are separated by 2.1" and 3.5 pix
The object was found in VSX 2" ASASSN-V J221619.56+631412.1
Type: SR
# Max. Min./Amp. JD0 Period
14.310 V 14.600 V 2457614.00000 523.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:16:19.48 +63:14:09.8: 13.83 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:16:19.48 +63:14:09.8: 13.81 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221619.56+631412.1,2461186.7241,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J221619.56+631412.1 20260526.2241 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.10 22:27:22.59 +64:29:07.1
108.18259 5.82169 galactic Cep Second-epoch detections are separated by 2.1" and 3.0 pix
The object was found in VSX 2" V0670 Cep
Type: SR
# Max. Min./Amp. JD0 Period
13.500 V 14.100 V 72.800000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:27:22.59 +64:29:07.1: 13.17 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:27:22.59 +64:29:07.1: 12.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0670 Cep,2461186.7241,12.10,0.05,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
V0670 Cep 20260526.2241 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.41 21:27:27.26 +62:53:20.7
101.94082 8.66288 galactic Cep Second-epoch detections are separated by 2.0" and 3.7 pix
The object was found in VSX 3" V0484 Cep
Type: SRA
# Max. Min./Amp. JD0 Period
13.200 V 15.000 V 2450273.00000 246.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:27:27.26 +62:53:20.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:27:27.26 +62:53:20.7: 13.57 +/- 0.08 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0484 Cep,2461186.7241,12.41,0.05,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
V0484 Cep 20260526.2241 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.59 21:58:14.62 +59:37:47.3
102.59827 3.78040 galactic Cep Second-epoch detections are separated by 1.0" and 3.8 pix
The object was found in VSX 1" V1161 Cep
Type: SRB
# Max. Min./Amp. JD0 Period
15.430 g 16.420 g 150.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:58:14.62 +59:37:47.3: 13.94 +/- 0.06 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:58:14.62 +59:37:47.3: 13.68 +/- 0.09 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1161 Cep,2461186.7241,12.59,0.05,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
V1161 Cep 20260526.2241 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.55 22:11:21.81 +62:35:59.7
105.64461 5.23053 galactic Cep Second-epoch detections are separated by 2.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2205683169280219264 | 22:11:25.47 +62:35:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:11:21.81 +62:35:59.7: 13.58 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:11:21.81 +62:35:59.7: 13.40 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2205683169280219264,2461186.7241,12.55,0.05,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 2205683169280219264 20260526.2241 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.71 21:45:50.55 +58:06:27.6
100.39062 3.60524 galactic Cep Second-epoch detections are separated by 0.3" and 3.8 pix
The object was found in VSX 1" NSVS 3296011
Type: SR
# Max. Min./Amp. JD0 Period
15.514 g Y 1.061 g 2458268.22780 140.307300500000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:45:50.55 +58:06:27.6: 12.83 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:45:50.55 +58:06:27.6: 12.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3296011,2461186.7241,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3296011 20260526.2241 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.25 22:28:25.51 +62:26:43.0
107.21054 4.02237 galactic Cep Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2205114824848370432 | 22:28:25.59 +62:26:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:28:25.51 +62:26:43.0: 13.28 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:28:25.51 +62:26:43.0: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2205114824848370432,2461186.7241,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2205114824848370432 20260526.2241 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.90 21:56:41.34 +58:53:08.2
101.98351 3.31477 galactic Cep Second-epoch detections are separated by 1.3" and 3.9 pix
The object was found in VSX 2" ZTF J215641.26+585309.6
Type: SR
# Max. Min./Amp. JD0 Period
15.008 g Y 0.301 g 2458635.98600 33.479495400000 M7
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:56:41.34 +58:53:08.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:56:41.34 +58:53:08.2: 12.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J215641.26+585309.6,2461186.7241,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J215641.26+585309.6 20260526.2241 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.44 21:53:12.66 +60:13:42.4
102.47347 4.64079 galactic Cep Second-epoch detections are separated by 1.3" and 3.7 pix
The object was found in VSX 3" ASASSN-V J215312.72+601345.6
Type: L:
# Max. Min./Amp. JD0 Period
14.170 V 14.640 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 21:53:12.66 +60:13:42.4: 13.68 +/- 0.04 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 21:53:12.66 +60:13:42.4: 13.71 +/- 0.09 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J215312.72+601345.6,2461186.7241,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J215312.72+601345.6 20260526.2241 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.10 22:06:02.22 +60:44:56.8
104.04829 4.09344 galactic Cep Second-epoch detections are separated by 2.2" and 3.6 pix
The object was found in VSX 5" ASASSN-V J220602.41+604501.5
Type: SR
# Max. Min./Amp. JD0 Period
12.639 r Y 0.435 r 2458318.69740 97.030685100000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:06:02.22 +60:44:56.8: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:06:02.22 +60:44:56.8: 12.98 +/- 0.04 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J220602.41+604501.5,2461186.7241,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J220602.41+604501.5 20260526.2241 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 12.19 22:12:26.58 +59:18:44.6
103.86730 2.45907 galactic Cep Second-epoch detections are separated by 1.7" and 3.7 pix
The object was found in VSX 2" ZTF J221226.62+591846.0
Type: SR
# Max. Min./Amp. JD0 Period
12.610 r Y 0.142 r 2458387.65350 53.139360100000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:12:26.58 +59:18:44.6: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:12:26.58 +59:18:44.6: 13.30 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J221226.62+591846.0,2461186.7241,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J221226.62+591846.0 20260526.2241 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2241 2461186.7241 11.95 22:42:39.13 +63:01:33.8
108.91612 3.71361 galactic Cep Second-epoch detections are separated by 0.8" and 3.2 pix
The object was found in VSX 3" NSVS 3511915
Type: SR
# Max. Min./Amp. JD0 Period
14.688 g Y 0.300 R1 2458382.80080 82.756884700000
The object was not found in astcheck.
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:42:39.13 +63:01:33.8: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:42:39.13 +63:01:33.8: 13.18 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.26 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3511915,2461186.7241,11.95,0.05,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 3511915 20260526.2241 11.95CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.62570392 23.12.2025 03:00:50.819 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
First image: 2461032.62570392 23.12.2025 03:00:50.819 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Last image: 2461186.72440697 26.05.2026 05:22:58.762 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 32
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
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: 5 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): 13615
Objects passed selection criteria: 13594
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 12249
Average stars matched: 12178.2 (99.4224 %)
Memory usage VmPeak: 124192 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 26 00:33:31 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: 2461032.62570392 23.12.2025 03:00:50.819 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
First image: 2461032.62570392 23.12.2025 03:00:50.819 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Last image: 2461186.72440697 26.05.2026 05:22:58.762 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 290
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.43
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: 28 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): 112818
Objects passed selection criteria: 112583
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 90250.5
Average stars matched: 89399 (99.0565 %)
Memory usage VmPeak: 1905564 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 26 00:37:16 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/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
SExtractor catalog cache: saved Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat to cache
SExtractor catalog cache: saved Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.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/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.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: 2461186.72386322
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_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits exists and is non-empty
Saving wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits to local_wcs_cache/
'wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits' -> 'local_wcs_cache/wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits'
wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits exists and is non-empty
Saving wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits to local_wcs_cache/
'wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits' -> 'local_wcs_cache/wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits'
wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits exists and is non-empty
Saving wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits to local_wcs_cache/
'wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits' -> 'local_wcs_cache/wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits'
wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits exists and is non-empty
Saving wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits to local_wcs_cache/
'wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits' -> 'local_wcs_cache/wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits (1st reference image)
verification OK: wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Image size: 941.6'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:13.968 +61:59:38.42 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits (1st new image)
verification OK: wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:56.093 +62:00:16.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:13.968 +61:59:38.42
Second-epoch image center 22:16:56.093 +62:00:16.92
Angular distance between the image centers 0.0366 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits (2nd new image)
verification OK: wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:58.934 +62:00:16.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:13.968 +61:59:38.42
Second-epoch image center 22:16:58.934 +62:00:16.90
Angular distance between the image centers 0.0313 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:16:56.093 +62:00:16.92
Second-epoch second image center 22:16:58.934 +62:00:16.90
Angular distance between the image centers 0.00556 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits &> /tmp/tmp.e0QFh50L47
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits &> /tmp/tmp.NqqZ4Og9N8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits &> /tmp/tmp.3c0RWQA7eZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits &> /tmp/tmp.Y7v6dqET9l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.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_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
Found non-empty wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits and wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
The reference image (wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits) and catalog (wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat) found
'wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat' -> 'wcsmag.cat'
Read 26505 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 315.7073 to 354.1451 deg, Dec +55.3424 to +67.4078 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 315.7073 to 354.1451 deg, Dec 55.3424 to 67.4078 deg
Loaded 22030 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): 12349 out of 13829 total matches.
Matched with Tycho-2 13829 out of 26505 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.942700
a=0.000000 b=1.000000 c=22.942700
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 26505 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 315.7073 to 354.1451 deg, Dec +55.3424 to +67.4078 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 315.7073 to 354.1451 deg, Dec 55.3424 to 67.4078 deg
Loaded 22030 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): 12349 out of 13829 total matches.
Matched with Tycho-2 13829 out of 26505 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits:
Forced-photometry filter: calibrated wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits -> calib.txt_param_ref_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits (aperture=6.0)
Read 13833 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 315.3774 to 354.0209 deg, Dec +55.5200 to +67.3681 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 315.3774 to 354.0209 deg, Dec 55.5200 to 67.3681 deg
Loaded 21406 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): 9846 out of 10295 total matches.
Matched with Tycho-2 10295 out of 13833 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits:
Forced-photometry filter: calibrated wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits -> calib.txt_param_ref_wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 28 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
2.2 pix Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
3.8 pix fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
3.9 pix fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
2.1 pix wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
2.2 pix wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
Limiting magnitude estimates:
15.2 mag. Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
14.4 mag. Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
12.3 mag. fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
12.3 mag. fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
All-image limiting magnitude estimate: 12.3 (SNR ) 10.5 (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.e0QFh50L47 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits' -> 'wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS-calibrated image found: wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
Checking if the catalog wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits
WCS catalog name: wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3069, passed=26505
Got 26505 stars (including 23407 good ones) from the SExtractor catalog wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 26505 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 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(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 24985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 24985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 24984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits N_match=972 sigma_overall_arcsec=0.424 sigma_q1_arcsec=0.482 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.394 n_q1=174 n_q2=263 n_q3=248 n_q4=287 worst_quadrant_to_overall_ratio=1.136
The image catalog is written to wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits -region wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NqqZ4Og9N8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits' -> 'wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
WCS_IMAGE_NAME=wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
WCS-calibrated image found: wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
Checking if the catalog wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat corresponding to the image wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits alredy exist and is non-empty...
Catalog wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat corresponding to the image wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits
WCS catalog name: wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1104, passed=13833
Got 13833 stars (including 12711 good ones) from the SExtractor catalog wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat
util/solve_plate_with_UCAC5 got 13833 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.8'
Seting catalog search parameters based on the expected field of view 942.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013094 (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 0.010476 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 13654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 13656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 13656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits N_match=966 sigma_overall_arcsec=0.432 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.425 sigma_q4_arcsec=0.445 n_q1=256 n_q2=218 n_q3=273 n_q4=219 worst_quadrant_to_overall_ratio=1.029
The image catalog is written to wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits -region wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3c0RWQA7eZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
WCS_IMAGE_NAME=wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
WCS-calibrated image found: wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
Checking if the catalog wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat corresponding to the image wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat corresponding to the image wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
WCS catalog name: wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=202, passed=4482
Got 4482 stars (including 4280 good ones) from the SExtractor catalog wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat
util/solve_plate_with_UCAC5 got 4482 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010473 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 4279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 4278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 4278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits N_match=961 sigma_overall_arcsec=0.535 sigma_q1_arcsec=0.613 sigma_q2_arcsec=0.615 sigma_q3_arcsec=0.521 sigma_q4_arcsec=0.499 n_q1=367 n_q2=74 n_q3=275 n_q4=245 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits -region wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Y7v6dqET9l (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
WCS_IMAGE_NAME=wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
WCS-calibrated image found: wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
Checking if the catalog wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat corresponding to the image wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat corresponding to the image wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
WCS catalog name: wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=206, passed=4488
Got 4488 stars (including 4281 good ones) from the SExtractor catalog wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat
util/solve_plate_with_UCAC5 got 4488 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010473 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 4285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 4285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 4284 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits N_match=960 sigma_overall_arcsec=0.551 sigma_q1_arcsec=0.643 sigma_q2_arcsec=0.517 sigma_q3_arcsec=0.501 sigma_q4_arcsec=0.524 n_q1=361 n_q2=89 n_q3=258 n_q4=252 worst_quadrant_to_overall_ratio=1.167
The image catalog is written to wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits -region wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits sigma_overall=0.424 worst_q_ratio=1.136
ref2=Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits sigma_overall=0.432 worst_q_ratio=1.029
new1=fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits sigma_overall=0.535 worst_q_ratio=1.149
new2=fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits sigma_overall=0.551 worst_q_ratio=1.167
reference average sigma_overall=0.428 worst_q_ratio=1.0825
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082_astrometric_residuals.png (972 matched stars from wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211_astrometric_residuals.png (966 matched stars from wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112_astrometric_residuals.png (961 matched stars from wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113_astrometric_residuals.png (960 matched stars from wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-11_20.00sec_-0.00C_LIGHTs_0112.fits'
Saving fully-calibrated image wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Cep-06-Q1b1x1_002453_TTUQ1b1x1_2676351_XkqJrg8R/wcs_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113.fits'
Preparing the HTML report for the field Cep-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:09:04.57 +61:10:20.7: 11.24 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:56:21.09 +64:47:22.0: 10.28 +/- 0.00 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:33:37.32 +63:35:08.5: 11.46 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:37:17.45 +63:57:16.3: 11.49 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:05:57.91 +60:59:53.5: 11.61 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits at 22:12:56.08 +59:46:48.9: 11.49 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:09:04.57 +61:10:20.7: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Forced photometry filter KEPT candidate at 22:09:04.57 +61:10:20.7: ref_mag=11.25 +/- 0.01 new_mean_mag=10.2150 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:33:37.32 +63:35:08.5: 11.38 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:56:21.09 +64:47:22.0: 10.37 +/- 0.00 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:37:17.45 +63:57:16.3: 11.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.29 +/- 0.00
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Forced photometry filter KEPT candidate at 22:33:37.32 +63:35:08.5: ref_mag=11.44 +/- 0.01 new_mean_mag=10.5003 delta=0.94 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:56:21.09 +64:47:22.0: ref_mag=10.29 +/- 0.00 new_mean_mag=10.0181 delta=0.27 (need > 0.90)
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Forced photometry filter KEPT candidate at 22:37:17.45 +63:57:16.3: ref_mag=11.46 +/- 0.01 new_mean_mag=10.4491 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:05:57.91 +60:59:53.5: 11.25 +/- 0.01 detection
Forced photometry on wcs_Cep-06-Q1b1x1_2026-04-17_03-02-46_20.00sec_-4.90C_LIGHTs_0211.fits at 22:12:56.08 +59:46:48.9: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.01
Forced photometry filter KEPT candidate at 22:05:57.91 +60:59:53.5: ref_mag=11.48 +/- 0.01 new_mean_mag=10.3435 delta=1.14 (need > 0.90)
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Forced photometry filter KEPT candidate at 22:12:56.08 +59:46:48.9: ref_mag=11.45 +/- 0.01 new_mean_mag=10.4511 delta=1.00 (need > 0.90)
Adding exclusion_list_local.txt__out05887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16472.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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: 3s
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Considering the candidate 30237_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30237_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:54:17.34 +56:19:59.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30238_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30238_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:10:09.49 +57:26:54.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30239_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30239_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:04:55.96 +56:41:26.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30241_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30241_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:04:24.97 +56:27:28.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30243_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30243_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:52:35.42 +56:31:14.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30244_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30244_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:10:07.60 +56:50:54.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30245_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30245_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:08:23.62 +57:10:48.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30246_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30246_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:56:11.00 +56:27:00.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30247_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30247_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:57:02.79 +56:29:24.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30250_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30250_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:10:29.11 +57:01:48.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30253_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30253_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:14:06.51 +57:57:13.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30254_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30254_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:08:35.66 +56:54:07.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30256_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30256_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:08:15.60 +56:18:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30257_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30257_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:57:25.59 +57:00:46.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30260_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30260_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 30261_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30261_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 30262_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30262_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 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 30264_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30264_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:13:05.42 +57:27:32.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30271_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30271_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 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 13008_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 13008_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 03446_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 03446_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 30005_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 30005_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:09:09.66 +57:31:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06781_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 06781_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 10639_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 10639_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:13:50.27 +61:51:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10212_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 10212_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 201227_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201227_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 201234_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201234_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 201236_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201236_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:29:09.30 +58:24:17.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 201240_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201240_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:54:17.32 +56:19:59.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201242_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201242_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:10:09.48 +57:26:54.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201243_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201243_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:04:55.97 +56:41:26.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201244_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201244_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:04:24.96 +56:27:28.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201247_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201247_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:10:07.59 +56:50:54.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201249_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201249_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:08:23.61 +57:10:48.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201252_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201252_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 201253_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201253_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:56:11.00 +56:27:00.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201254_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201254_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:57:02.78 +56:29:24.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201255_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201255_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:10:29.10 +57:01:48.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201257_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201257_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:08:35.65 +56:54:07.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201258_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201258_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:14:06.50 +57:57:13.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201259_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201259_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 201263_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201263_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:08:15.59 +56:18:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201264_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201264_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 201265_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201265_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:13:05.42 +57:27:32.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201266_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201266_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 201269_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201269_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 201272_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201272_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:43:48.85 +58:48:33.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 201275_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201275_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 201277_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201277_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:58:16.27 +56:58:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201281_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201281_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:00:31.73 +56:34:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201282_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201282_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:11:44.89 +57:06:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201286_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201286_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:06:20.21 +57:32:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201289_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201289_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:05:01.63 +55:54:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201290_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201290_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 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 201293_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201293_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:08:58.63 +56:22:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201296_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201296_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:59:11.86 +56:52:08.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201301_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201301_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:03:23.41 +57:33:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201304_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201304_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:56:53.08 +56:19:04.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201308_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201308_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 201314_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201314_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:12:28.53 +57:29:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201318_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201318_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:07:18.63 +56:15:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201320_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201320_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 201321_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201321_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:11:02.63 +57:09:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201322_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201322_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 201323_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201323_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:24:56.66 +62:18:49.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201324_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201324_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:57:13.62 +56:28:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201325_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201325_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:07:36.41 +56:28:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201330_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201330_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:56:54.99 +56:33:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201332_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201332_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 201334_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201334_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 201336_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201336_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:52:03.47 +56:40:08.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 201341_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201341_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:06:54.70 +56:42:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201346_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201346_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:54:44.12 +56:39:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201347_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201347_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:52:46.45 +56:14:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201350_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201350_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:10:09.76 +56:33:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201353_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201353_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:07:45.30 +57:57:34.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201355_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201355_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201359_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201359_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:17:30.30 +58:11:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 2.428 2191059428420371072 319.37505819338 +58.18689395604 12.4142 10.2591 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201361_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201361_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:57:31.99 +66:09:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201364_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201364_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 201366_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201366_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:18:34.46 +61:12:41.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201367_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201367_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 201368_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201368_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:53:57.91 +62:37:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201369_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201369_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:09:02.53 +56:59:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201370_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201370_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:17:59.99 +63:08:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201372_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201372_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:45:11.72 +61:08:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201373_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201373_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:52:27.15 +56:26:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201377_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201377_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:56:09.39 +56:51:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201379_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201379_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:55:21.67 +65:19:50.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201380_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201380_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:55:55.11 +56:33:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201381_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201381_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:08:20.26 +56:43:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201383_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201383_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:54:50.46 +56:37:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201384_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201384_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:55:24.74 +56:14:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201385_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201385_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 201387_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201387_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:04:21.40 +55:56:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201389_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201389_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:07:39.71 +56:06:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201390_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201390_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 201392_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201392_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 201394_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201394_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:07:08.84 +56:25:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201397_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201397_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 201402_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201402_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:53:40.52 +62:35:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201403_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201403_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:18:10.36 +62:46:23.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201406_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201406_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:23:32.20 +65:02:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201408_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201408_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:10:42.75 +57:15:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201409_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201409_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:06:18.50 +57:19:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201410_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201410_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:04:56.47 +56:05:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201413_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201413_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:11:37.31 +60:05:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201414_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201414_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:25:24.89 +60:37:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201416_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201416_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:58:31.15 +56:44:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201417_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201417_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 201422_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201422_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:11:01.31 +56:57:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201423_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201423_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:18:54.66 +62:37:14.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 201424_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201424_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:07:57.13 +56:17:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201425_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201425_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:06:27.02 +57:33:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201430_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201430_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:11:05.51 +57:16:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201431_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201431_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:18:07.44 +62:46:43.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201433_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201433_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 201434_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201434_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:58:55.04 +59:05:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201437_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201437_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:42:47.69 +58:57:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201445_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201445_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:05:45.34 +56:07:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201452_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201452_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 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 201453_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201453_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 201454_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201454_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 201455_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201455_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:11:58.22 +59:06:34.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201460_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201460_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 201463_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201463_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:09:27.87 +56:54:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201468_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201468_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:04:32.51 +61:22:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201473_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201473_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:58:00.75 +56:16:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201475_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201475_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201480_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201480_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:55:08.62 +56:22:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201481_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201481_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:06:54.70 +57:47:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201482_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201482_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:07:43.02 +56:17:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201483_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201483_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:53:39.16 +56:22:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201496_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201496_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 201500_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201500_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 201501_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201501_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:01:48.09 +56:58:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201505_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201505_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 201507_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201507_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 201518_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 201518_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 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 127244_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 127244_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 112797_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 112797_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 112957_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 112957_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 96873_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 96873_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:09:04.59 +61:10:20.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 48932_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 48932_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 137257_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 137257_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:01:37.47 +59:07:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34071_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 34071_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 124449_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 124449_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:03:42.83 +59:45:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68069_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 68069_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 114920_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 114920_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 140686_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 140686_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:58:58.40 +58:28:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24766_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 24766_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 110557_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 110557_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 100979_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 100979_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 166979_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 166979_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 47789_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 47789_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 04348_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 04348_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:06:21.89 +65:58:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114931_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 114931_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 122630_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 122630_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 67092_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 67092_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 117605_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 117605_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 32533_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 32533_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 172483_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 172483_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:03:10.67 +57:47:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25805_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 25805_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 76322_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 76322_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 183628_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 183628_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 138772_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 138772_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 49247_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 49247_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 80245_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 80245_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 139103_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 139103_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106151_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 106151_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:07:26.84 +60:41:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89637_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 89637_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 125966_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 125966_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 107743_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 107743_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08193_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 08193_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 73776_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 73776_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 103709_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 103709_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15017_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 15017_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:00:47.36 +65:15:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36181_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 36181_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:33:48.44 +64:42:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138168_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 138168_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 98741_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 98741_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89660_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 89660_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199169_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 199169_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:47:43.67 +63:52:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173389_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 173389_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120728_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 120728_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:16:55.97 +59:49:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198564_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 198564_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:13:43.88 +63:03:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128770_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 128770_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116916_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 116916_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 81900_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 81900_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144435_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 144435_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:56:19.06 +58:48:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.691 2202454938718802304 329.07911966112 +58.80642022365 10.5413 8.9060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83887_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 83887_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:03:09.04 +61:50:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52603_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 52603_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96661_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 96661_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 171976_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 171976_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 05842_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 05842_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 35146_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 35146_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 42724_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 42724_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:11:26.48 +62:58:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109979_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 109979_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 126730_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 126730_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 162033_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 162033_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 23821_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 23821_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 54695_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 54695_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101166_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 101166_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 90136_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 90136_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 119280_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 119280_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 94931_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 94931_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 69283_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 69283_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:29:30.18 +62:20:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.851 2202107974089476608 337.37550792710 +62.34677943813 12.3300 10.8542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90481_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 90481_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187058_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 187058_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103676_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 103676_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67462_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 67462_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 112044_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 112044_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 05449_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 05449_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:40:37.07 +66:30:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59464_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 59464_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:05:49.57 +62:01:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31786_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 31786_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 102325_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 102325_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:05:57.95 +60:59:53.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 05940_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 05940_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:29:24.50 +64:59:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114231_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 114231_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 13438_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 13438_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 23:05:20.48 +65:14:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89584_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 89584_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:08:37.61 +61:29:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43087_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 43087_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 139371_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 139371_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 32151_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 32151_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:57:34.68 +65:02:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104021_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 104021_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 83294_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 83294_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 62978_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 62978_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:16:27.75 +62:54:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122538_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 122538_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 109872_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 109872_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 137924_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 137924_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 139990_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 139990_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 127982_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 127982_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:40:06.13 +59:35:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84881_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 84881_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 150126_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 150126_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 186981_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 186981_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 76639_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 76639_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:20:08.38 +62:10:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147111_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 147111_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 124795_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 124795_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 73872_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 73872_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 59976_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 59976_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 49899_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 49899_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 103698_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 103698_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 97335_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 97335_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 44350_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 44350_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:30:42.50 +63:56:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137780_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 137780_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 174474_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 174474_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:44:45.65 +57:54:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108588_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 108588_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 51052_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 51052_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:44:02.73 +63:12:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81381_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 81381_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 79153_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 79153_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:13:50.37 +61:51:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44702_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 44702_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 113126_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 113126_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 07078_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 07078_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 01883_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 01883_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:32:59.58 +66:54:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99875_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 99875_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 118100_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 118100_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 110809_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 110809_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 112643_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 112643_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 69573_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 69573_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 108223_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 108223_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:44:39.84 +60:37:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.344 2203814003818638592 326.16549182139 +60.63274046351 11.5284 9.9283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162034_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 162034_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 21:48:36.04 +57:23:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36207_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 36207_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 29133_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 29133_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:51:14.20 +64:30:28.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
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Considering the candidate 129021_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 129021_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 67021_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 67021_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 146929_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 146929_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 57970_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 57970_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 36857_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 36857_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 63441_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 63441_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 103470_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 103470_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 127295_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 127295_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 69069_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 69069_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 178383_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 178383_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 144882_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 144882_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:06:02.34 +58:47:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68053_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 68053_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 145785_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 145785_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 18346_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 18346_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
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Considering the candidate 116254_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 116254_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 105439_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 105439_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 131576_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 131576_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
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Considering the candidate 28970_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
The candidate 28970_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113 did not pass the final checks
**** FOUND 22:53:17.85 +64:29:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54612_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
Preparing report for the candidate 54612_fd_Cep-06-Q1b1x1_2026-05-26_00-22-58_20.00sec_-0.00C_LIGHTs_0113
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 110s
Prepared the HTML report for the field Cep-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:37:17.45 +63:57:16.3
22:33:37.32 +63:35:08.5
22:09:04.57 +61:10:20.7
22:05:57.91 +60:59:53.5
22:12:56.08 +59:46:48.9
23:08:21.84 +65:45:41.0
23:29:30.89 +64:51:22.8
21:54:36.75 +66:45:22.7
22:18:21.42 +60:49:19.4
22:17:40.07 +60:49:17.2
22:16:55.71 +60:42:41.9
22:21:29.15 +60:43:09.5
22:01:58.12 +60:50:05.0
22:07:49.36 +60:47:25.6
22:06:02.22 +60:44:56.8
22:21:01.21 +60:27:28.3
22:02:27.88 +60:31:33.8
22:01:13.94 +60:31:19.0
22:15:20.50 +60:25:22.1
22:06:33.76 +60:27:01.7
22:05:07.34 +60:24:12.0
21:57:24.82 +60:24:06.0
21:59:39.48 +60:23:13.2
22:01:44.63 +60:21:40.2
22:07:19.44 +60:19:26.7
22:14:56.09 +60:11:44.1
22:11:18.94 +60:13:25.6
21:58:25.50 +60:17:16.9
21:53:12.66 +60:13:42.4
21:55:19.04 +60:10:45.0
22:14:31.15 +60:01:13.2
22:21:01.27 +59:55:03.8
22:14:03.95 +59:56:21.5
22:18:41.17 +59:42:11.4
22:05:04.48 +59:50:31.7
22:08:21.81 +59:41:52.1
22:09:28.28 +59:37:57.4
22:12:30.98 +59:33:40.8
21:55:24.77 +59:38:37.7
21:58:14.62 +59:37:47.3
21:46:57.24 +59:34:47.8
21:52:39.15 +59:33:19.7
22:12:26.58 +59:18:44.6
21:53:45.42 +59:05:56.7
22:02:12.28 +59:04:10.5
21:57:04.34 +59:06:16.8
22:00:38.03 +58:07:05.2
22:02:46.47 +58:09:24.7
22:03:52.81 +58:10:46.3
21:58:55.88 +58:19:46.6
21:56:41.34 +58:53:08.2
21:47:35.69 +58:56:18.4
21:51:10.35 +58:56:54.9
22:03:43.61 +59:02:25.8
21:42:26.21 +57:22:28.6
22:06:46.19 +57:31:20.7
21:45:11.06 +57:48:03.6
21:35:41.80 +57:48:44.3
21:45:50.55 +58:06:27.6
22:05:12.92 +58:20:37.8
21:46:38.92 +58:36:51.9
21:42:33.40 +58:35:41.5
22:29:50.20 +65:19:21.9
22:36:20.36 +65:08:49.5
22:37:40.37 +65:03:02.7
22:00:43.14 +65:03:47.0
22:51:04.01 +64:16:22.2
22:47:21.63 +64:15:53.9
22:45:34.10 +64:14:38.4
22:41:05.32 +64:16:04.3
22:27:22.59 +64:29:07.1
22:45:34.16 +63:37:04.4
21:33:16.40 +63:57:12.3
22:32:31.53 +63:34:54.0
22:40:33.48 +63:24:37.2
21:55:24.82 +63:53:20.2
22:37:48.63 +63:15:40.3
22:42:39.13 +63:01:33.8
22:33:25.13 +63:13:00.9
22:16:19.48 +63:14:09.8
22:31:26.46 +62:54:57.0
21:27:27.26 +62:53:20.7
22:14:47.28 +62:41:01.1
22:31:29.28 +62:26:42.0
22:19:28.29 +62:36:52.6
22:28:25.51 +62:26:43.0
22:18:00.45 +62:36:55.8
22:11:21.81 +62:35:59.7
22:31:11.72 +62:18:44.1
22:20:03.44 +62:14:56.1
22:16:22.62 +62:16:39.9
22:24:21.64 +62:02:45.3
22:07:11.97 +62:00:37.4
22:23:27.33 +61:46:07.8
22:07:55.35 +61:54:25.6
22:24:56.51 +61:38:33.6
21:33:08.41 +61:46:29.1
22:21:24.90 +61:21:31.7
22:25:24.93 +61:18:04.5
22:19:14.01 +61:22:38.1
22:15:00.76 +61:24:10.8
22:01:47.83 +61:17:28.4
22:09:47.47 +61:09:35.2
22:02:22.60 +61:09:41.9
22:19:07.84 +60:55:50.0
22:14:44.65 +60:55:33.5
########### Completed Cep-06-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 ####
22:09:04.57 +61:10:20.7
22:33:37.32 +63:35:08.5
22:37:17.45 +63:57:16.3
22:12:56.08 +59:46:48.9
22:05:57.91 +60:59:53.5
21:55:24.77 +59:38:37.7
21:59:39.48 +60:23:13.2
22:01:44.63 +60:21:40.2
22:32:31.53 +63:34:54.0
22:47:21.63 +64:15:53.9
22:18:00.45 +62:36:55.8
22:11:18.94 +60:13:25.6
22:36:20.36 +65:08:49.5
22:15:20.50 +60:25:22.1
22:18:21.42 +60:49:19.4
22:06:46.19 +57:31:20.7
21:33:16.40 +63:57:12.3
21:58:25.50 +60:17:16.9
22:05:04.48 +59:50:31.7
22:31:29.28 +62:26:42.0
22:14:31.15 +60:01:13.2
22:51:04.01 +64:16:22.2
22:37:40.37 +65:03:02.7
22:24:21.64 +62:02:45.3
22:05:12.92 +58:20:37.8
22:00:38.03 +58:07:05.2
22:40:33.48 +63:24:37.2
22:07:11.97 +62:00:37.4
22:02:46.47 +58:09:24.7
22:21:24.90 +61:21:31.7
22:09:28.28 +59:37:57.4
22:21:01.21 +60:27:28.3
21:54:36.75 +66:45:22.7
22:20:03.44 +62:14:56.1
22:01:58.12 +60:50:05.0
21:57:04.34 +59:06:16.8
22:19:07.84 +60:55:50.0
22:25:24.93 +61:18:04.5
21:35:41.80 +57:48:44.3
21:46:57.24 +59:34:47.8
21:55:19.04 +60:10:45.0
22:07:55.35 +61:54:25.6
22:37:48.63 +63:15:40.3
22:09:47.47 +61:09:35.2
21:45:11.06 +57:48:03.6
23:08:21.84 +65:45:41.0
22:45:34.10 +64:14:38.4
22:01:13.94 +60:31:19.0
22:12:30.98 +59:33:40.8
21:42:26.21 +57:22:28.6
22:29:50.20 +65:19:21.9
22:33:25.13 +63:13:00.9
22:17:40.07 +60:49:17.2
22:19:14.01 +61:22:38.1
22:14:03.95 +59:56:21.5
22:01:47.83 +61:17:28.4
22:15:00.76 +61:24:10.8
21:42:33.40 +58:35:41.5
22:16:55.71 +60:42:41.9
22:19:28.29 +62:36:52.6
22:05:07.34 +60:24:12.0
22:00:43.14 +65:03:47.0
22:14:56.09 +60:11:44.1
22:03:52.81 +58:10:46.3
22:07:49.36 +60:47:25.6
22:24:56.51 +61:38:33.6
22:18:41.17 +59:42:11.4
22:02:27.88 +60:31:33.8
22:02:12.28 +59:04:10.5
21:58:55.88 +58:19:46.6
21:33:08.41 +61:46:29.1
22:03:43.61 +59:02:25.8
21:46:38.92 +58:36:51.9
21:51:10.35 +58:56:54.9
22:08:21.81 +59:41:52.1
22:16:22.62 +62:16:39.9
22:31:26.46 +62:54:57.0
21:55:24.82 +63:53:20.2
22:21:29.15 +60:43:09.5
22:02:22.60 +61:09:41.9
21:53:45.42 +59:05:56.7
22:23:27.33 +61:46:07.8
22:45:34.16 +63:37:04.4
22:07:19.44 +60:19:26.7
23:29:30.89 +64:51:22.8
22:14:44.65 +60:55:33.5
22:21:01.27 +59:55:03.8
22:06:33.76 +60:27:01.7
21:57:24.82 +60:24:06.0
22:31:11.72 +62:18:44.1
22:41:05.32 +64:16:04.3
21:52:39.15 +59:33:19.7
22:14:47.28 +62:41:01.1
21:47:35.69 +58:56:18.4
22:16:19.48 +63:14:09.8
22:27:22.59 +64:29:07.1
21:27:27.26 +62:53:20.7
21:58:14.62 +59:37:47.3
22:11:21.81 +62:35:59.7
21:45:50.55 +58:06:27.6
22:28:25.51 +62:26:43.0
21:56:41.34 +58:53:08.2
21:53:12.66 +60:13:42.4
22:06:02.22 +60:44:56.8
22:12:26.58 +59:18:44.6
22:42:39.13 +63:01:33.8
###################################################################################
22:09:04.57 +61:10:20.7 -- not an asteroid (will add it to exclusion list)
22:33:37.32 +63:35:08.5 -- not an asteroid (will add it to exclusion list)
22:37:17.45 +63:57:16.3 -- not an asteroid (will add it to exclusion list)
22:12:56.08 +59:46:48.9 -- not an asteroid (will add it to exclusion list)
22:05:57.91 +60:59:53.5 -- not an asteroid (will add it to exclusion list)
21:55:24.77 +59:38:37.7 -- not an asteroid (will add it to exclusion list)
21:59:39.48 +60:23:13.2 -- not an asteroid (will add it to exclusion list)
22:01:44.63 +60:21:40.2 -- not an asteroid (will add it to exclusion list)
22:32:31.53 +63:34:54.0 -- not an asteroid (will add it to exclusion list)
22:47:21.63 +64:15:53.9 -- not an asteroid (will add it to exclusion list)
22:18:00.45 +62:36:55.8 -- not an asteroid (will add it to exclusion list)
22:11:18.94 +60:13:25.6 -- not an asteroid (will add it to exclusion list)
22:36:20.36 +65:08:49.5 -- not an asteroid (will add it to exclusion list)
22:15:20.50 +60:25:22.1 -- not an asteroid (will add it to exclusion list)
22:18:21.42 +60:49:19.4 -- not an asteroid (will add it to exclusion list)
22:06:46.19 +57:31:20.7 -- not an asteroid (will add it to exclusion list)
21:33:16.40 +63:57:12.3 -- not an asteroid (will add it to exclusion list)
21:58:25.50 +60:17:16.9 -- not an asteroid (will add it to exclusion list)
22:05:04.48 +59:50:31.7 -- not an asteroid (will add it to exclusion list)
22:31:29.28 +62:26:42.0 -- not an asteroid (will add it to exclusion list)
22:14:31.15 +60:01:13.2 -- not an asteroid (will add it to exclusion list)
22:51:04.01 +64:16:22.2 -- not an asteroid (will add it to exclusion list)
22:37:40.37 +65:03:02.7 -- not an asteroid (will add it to exclusion list)
22:24:21.64 +62:02:45.3 -- not an asteroid (will add it to exclusion list)
22:05:12.92 +58:20:37.8 -- not an asteroid (will add it to exclusion list)
22:00:38.03 +58:07:05.2 -- not an asteroid (will add it to exclusion list)
22:40:33.48 +63:24:37.2 -- not an asteroid (will add it to exclusion list)
22:07:11.97 +62:00:37.4 -- not an asteroid (will add it to exclusion list)
22:02:46.47 +58:09:24.7 -- not an asteroid (will add it to exclusion list)
22:21:24.90 +61:21:31.7 -- not an asteroid (will add it to exclusion list)
22:09:28.28 +59:37:57.4 -- not an asteroid (will add it to exclusion list)
22:21:01.21 +60:27:28.3 -- not an asteroid (will add it to exclusion list)
21:54:36.75 +66:45:22.7 -- not an asteroid (will add it to exclusion list)
22:20:03.44 +62:14:56.1 -- not an asteroid (will add it to exclusion list)
22:01:58.12 +60:50:05.0 -- not an asteroid (will add it to exclusion list)
21:57:04.34 +59:06:16.8 -- not an asteroid (will add it to exclusion list)
22:19:07.84 +60:55:50.0 -- not an asteroid (will add it to exclusion list)
22:25:24.93 +61:18:04.5 -- not an asteroid (will add it to exclusion list)
21:35:41.80 +57:48:44.3 -- not an asteroid (will add it to exclusion list)
21:46:57.24 +59:34:47.8 -- not an asteroid (will add it to exclusion list)
21:55:19.04 +60:10:45.0 -- not an asteroid (will add it to exclusion list)
22:07:55.35 +61:54:25.6 -- not an asteroid (will add it to exclusion list)
22:37:48.63 +63:15:40.3 -- not an asteroid (will add it to exclusion list)
22:09:47.47 +61:09:35.2 -- not an asteroid (will add it to exclusion list)
21:45:11.06 +57:48:03.6 -- not an asteroid (will add it to exclusion list)
23:08:21.84 +65:45:41.0 -- not an asteroid (will add it to exclusion list)
22:45:34.10 +64:14:38.4 -- not an asteroid (will add it to exclusion list)
22:01:13.94 +60:31:19.0 -- not an asteroid (will add it to exclusion list)
22:12:30.98 +59:33:40.8 -- not an asteroid (will add it to exclusion list)
21:42:26.21 +57:22:28.6 -- not an asteroid (will add it to exclusion list)
22:29:50.20 +65:19:21.9 -- not an asteroid (will add it to exclusion list)
22:33:25.13 +63:13:00.9 -- not an asteroid (will add it to exclusion list)
22:17:40.07 +60:49:17.2 -- not an asteroid (will add it to exclusion list)
22:19:14.01 +61:22:38.1 -- not an asteroid (will add it to exclusion list)
22:14:03.95 +59:56:21.5 -- not an asteroid (will add it to exclusion list)
22:01:47.83 +61:17:28.4 -- not an asteroid (will add it to exclusion list)
22:15:00.76 +61:24:10.8 -- not an asteroid (will add it to exclusion list)
21:42:33.40 +58:35:41.5 -- not an asteroid (will add it to exclusion list)
22:16:55.71 +60:42:41.9 -- not an asteroid (will add it to exclusion list)
22:19:28.29 +62:36:52.6 -- not an asteroid (will add it to exclusion list)
22:05:07.34 +60:24:12.0 -- not an asteroid (will add it to exclusion list)
22:00:43.14 +65:03:47.0 -- not an asteroid (will add it to exclusion list)
22:14:56.09 +60:11:44.1 -- not an asteroid (will add it to exclusion list)
22:03:52.81 +58:10:46.3 -- not an asteroid (will add it to exclusion list)
22:07:49.36 +60:47:25.6 -- not an asteroid (will add it to exclusion list)
22:24:56.51 +61:38:33.6 -- not an asteroid (will add it to exclusion list)
22:18:41.17 +59:42:11.4 -- not an asteroid (will add it to exclusion list)
22:02:27.88 +60:31:33.8 -- not an asteroid (will add it to exclusion list)
22:02:12.28 +59:04:10.5 -- not an asteroid (will add it to exclusion list)
21:58:55.88 +58:19:46.6 -- not an asteroid (will add it to exclusion list)
21:33:08.41 +61:46:29.1 -- not an asteroid (will add it to exclusion list)
22:03:43.61 +59:02:25.8 -- not an asteroid (will add it to exclusion list)
21:46:38.92 +58:36:51.9 -- not an asteroid (will add it to exclusion list)
21:51:10.35 +58:56:54.9 -- not an asteroid (will add it to exclusion list)
22:08:21.81 +59:41:52.1 -- not an asteroid (will add it to exclusion list)
22:16:22.62 +62:16:39.9 -- not an asteroid (will add it to exclusion list)
22:31:26.46 +62:54:57.0 -- not an asteroid (will add it to exclusion list)
21:55:24.82 +63:53:20.2 -- not an asteroid (will add it to exclusion list)
22:21:29.15 +60:43:09.5 -- not an asteroid (will add it to exclusion list)
22:02:22.60 +61:09:41.9 -- not an asteroid (will add it to exclusion list)
21:53:45.42 +59:05:56.7 -- not an asteroid (will add it to exclusion list)
22:23:27.33 +61:46:07.8 -- not an asteroid (will add it to exclusion list)
22:45:34.16 +63:37:04.4 -- not an asteroid (will add it to exclusion list)
22:07:19.44 +60:19:26.7 -- not an asteroid (will add it to exclusion list)
23:29:30.89 +64:51:22.8 -- not an asteroid (will add it to exclusion list)
22:14:44.65 +60:55:33.5 -- not an asteroid (will add it to exclusion list)
22:21:01.27 +59:55:03.8 -- not an asteroid (will add it to exclusion list)
22:06:33.76 +60:27:01.7 -- not an asteroid (will add it to exclusion list)
21:57:24.82 +60:24:06.0 -- not an asteroid (will add it to exclusion list)
22:31:11.72 +62:18:44.1 -- not an asteroid (will add it to exclusion list)
22:41:05.32 +64:16:04.3 -- not an asteroid (will add it to exclusion list)
21:52:39.15 +59:33:19.7 -- not an asteroid (will add it to exclusion list)
22:14:47.28 +62:41:01.1 -- not an asteroid (will add it to exclusion list)
21:47:35.69 +58:56:18.4 -- not an asteroid (will add it to exclusion list)
22:16:19.48 +63:14:09.8 -- not an asteroid (will add it to exclusion list)
22:27:22.59 +64:29:07.1 -- not an asteroid (will add it to exclusion list)
21:27:27.26 +62:53:20.7 -- not an asteroid (will add it to exclusion list)
21:58:14.62 +59:37:47.3 -- not an asteroid (will add it to exclusion list)
22:11:21.81 +62:35:59.7 -- not an asteroid (will add it to exclusion list)
21:45:50.55 +58:06:27.6 -- not an asteroid (will add it to exclusion list)
22:28:25.51 +62:26:43.0 -- not an asteroid (will add it to exclusion list)
21:56:41.34 +58:53:08.2 -- not an asteroid (will add it to exclusion list)
21:53:12.66 +60:13:42.4 -- not an asteroid (will add it to exclusion list)
22:06:02.22 +60:44:56.8 -- not an asteroid (will add it to exclusion list)
22:12:26.58 +59:18:44.6 -- not an asteroid (will add it to exclusion list)
22:42:39.13 +63:01:33.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
21:27:27.26 +62:53:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:08.41 +61:46:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:16.40 +63:57:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:41.80 +57:48:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:26.21 +57:22:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:33.40 +58:35:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:11.06 +57:48:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:50.55 +58:06:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:38.92 +58:36:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:46:57.24 +59:34:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:47:35.69 +58:56:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:51:10.35 +58:56:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:52:39.15 +59:33:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:12.66 +60:13:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:53:45.42 +59:05:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:54:36.75 +66:45:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:19.04 +60:10:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:24.77 +59:38:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:55:24.82 +63:53:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:56:41.34 +58:53:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:04.34 +59:06:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:57:24.82 +60:24:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:14.62 +59:37:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:25.50 +60:17:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:58:55.88 +58:19:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:59:39.48 +60:23:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:38.03 +58:07:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:00:43.14 +65:03:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:13.94 +60:31:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:44.63 +60:21:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:47.83 +61:17:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:58.12 +60:50:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:12.28 +59:04:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:22.60 +61:09:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:27.88 +60:31:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:46.47 +58:09:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:43.61 +59:02:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:52.81 +58:10:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:04.48 +59:50:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:07.34 +60:24:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:12.92 +58:20:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:57.91 +60:59:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:02.22 +60:44:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:33.76 +60:27:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:46.19 +57:31:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:11.97 +62:00:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:19.44 +60:19:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:49.36 +60:47:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:55.35 +61:54:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:08:21.81 +59:41:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:04.57 +61:10:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:28.28 +59:37:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:47.47 +61:09:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:18.94 +60:13:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:21.81 +62:35:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:26.58 +59:18:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:30.98 +59:33:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:12:56.08 +59:46:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:03.95 +59:56:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:31.15 +60:01:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:44.65 +60:55:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:47.28 +62:41:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:56.09 +60:11:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:00.76 +61:24:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:20.50 +60:25:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:19.48 +63:14:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:22.62 +62:16:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:55.71 +60:42:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:40.07 +60:49:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:00.45 +62:36:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:21.42 +60:49:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:41.17 +59:42:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:07.84 +60:55:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:14.01 +61:22:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:28.29 +62:36:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:03.44 +62:14:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:01.21 +60:27:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:01.27 +59:55:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:24.90 +61:21:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:21:29.15 +60:43:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:23:27.33 +61:46:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:21.64 +62:02:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:24:56.51 +61:38:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:25:24.93 +61:18:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:27:22.59 +64:29:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:28:25.51 +62:26:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:29:50.20 +65:19:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:31:11.72 +62:18:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:31:26.46 +62:54:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:31:29.28 +62:26:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:32:31.53 +63:34:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:33:25.13 +63:13:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:33:37.32 +63:35:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:36:20.36 +65:08:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:37:17.45 +63:57:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:37:40.37 +65:03:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:37:48.63 +63:15:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:40:33.48 +63:24:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:41:05.32 +64:16:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:42:39.13 +63:01:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:45:34.10 +64:14:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:45:34.16 +63:37:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:47:21.63 +64:15:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:51:04.01 +64:16:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:08:21.84 +65:45:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:30.89 +64:51:22.8 -- 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)
21:27:27.26 +62:53:20.7 -- a known variable star
21:33:08.41 +61:46:29.1 -- a known variable star
21:33:16.40 +63:57:12.3 -- a known variable star
21:35:41.80 +57:48:44.3 -- a known variable star
21:42:26.21 +57:22:28.6 -- a known variable star
21:42:33.40 +58:35:41.5 -- a known variable star
21:45:11.06 +57:48:03.6 -- a known variable star
21:45:50.55 +58:06:27.6 -- a known variable star
21:46:38.92 +58:36:51.9 -- a known variable star
21:46:57.24 +59:34:47.8 -- a known variable star
21:47:35.69 +58:56:18.4 -- a known variable star
21:51:10.35 +58:56:54.9 -- not a known variable star
21:52:39.15 +59:33:19.7 -- a known variable star
21:53:12.66 +60:13:42.4 -- a known variable star
21:53:45.42 +59:05:56.7 -- a known variable star
21:54:36.75 +66:45:22.7 -- a known variable star
21:55:19.04 +60:10:45.0 -- a known variable star
21:55:24.77 +59:38:37.7 -- a known variable star
21:55:24.82 +63:53:20.2 -- a known variable star
21:56:41.34 +58:53:08.2 -- a known variable star
21:57:04.34 +59:06:16.8 -- a known variable star
21:57:24.82 +60:24:06.0 -- a known variable star
21:58:14.62 +59:37:47.3 -- a known variable star
21:58:25.50 +60:17:16.9 -- a known variable star
21:58:55.88 +58:19:46.6 -- a known variable star
21:59:39.48 +60:23:13.2 -- a known variable star
22:00:38.03 +58:07:05.2 -- a known variable star
22:00:43.14 +65:03:47.0 -- a known variable star
22:01:13.94 +60:31:19.0 -- a known variable star
22:01:44.63 +60:21:40.2 -- a known variable star
22:01:47.83 +61:17:28.4 -- a known variable star
22:01:58.12 +60:50:05.0 -- a known variable star
22:02:12.28 +59:04:10.5 -- a known variable star
22:02:22.60 +61:09:41.9 -- a known variable star
22:02:27.88 +60:31:33.8 -- a known variable star
22:02:46.47 +58:09:24.7 -- a known variable star
22:03:43.61 +59:02:25.8 -- a known variable star
22:03:52.81 +58:10:46.3 -- a known variable star
22:05:04.48 +59:50:31.7 -- a known variable star
22:05:07.34 +60:24:12.0 -- not a known variable star
22:05:12.92 +58:20:37.8 -- a known variable star
22:05:57.91 +60:59:53.5 -- a known variable star
22:06:02.22 +60:44:56.8 -- a known variable star
22:06:33.76 +60:27:01.7 -- a known variable star
22:06:46.19 +57:31:20.7 -- a known variable star
22:07:11.97 +62:00:37.4 -- a known variable star
22:07:19.44 +60:19:26.7 -- a known variable star
22:07:49.36 +60:47:25.6 -- not a known variable star
22:07:55.35 +61:54:25.6 -- a known variable star
22:08:21.81 +59:41:52.1 -- a known variable star
22:09:04.57 +61:10:20.7 -- a known variable star
22:09:28.28 +59:37:57.4 -- a known variable star
22:09:47.47 +61:09:35.2 -- a known variable star
22:11:18.94 +60:13:25.6 -- a known variable star
22:11:21.81 +62:35:59.7 -- not a known variable star
22:12:26.58 +59:18:44.6 -- a known variable star
22:12:30.98 +59:33:40.8 -- a known variable star
22:12:56.08 +59:46:48.9 -- a known variable star
22:14:03.95 +59:56:21.5 -- not a known variable star
22:14:31.15 +60:01:13.2 -- a known variable star
22:14:44.65 +60:55:33.5 -- not a known variable star
22:14:47.28 +62:41:01.1 -- a known variable star
22:14:56.09 +60:11:44.1 -- a known variable star
22:15:00.76 +61:24:10.8 -- a known variable star
22:15:20.50 +60:25:22.1 -- a known variable star
22:16:19.48 +63:14:09.8 -- a known variable star
22:16:22.62 +62:16:39.9 -- a known variable star
22:16:55.71 +60:42:41.9 -- not a known variable star
22:17:40.07 +60:49:17.2 -- a known variable star
22:18:00.45 +62:36:55.8 -- a known variable star
22:18:21.42 +60:49:19.4 -- not a known variable star
22:18:41.17 +59:42:11.4 -- a known variable star
22:19:07.84 +60:55:50.0 -- not a known variable star
22:19:14.01 +61:22:38.1 -- a known variable star
22:19:28.29 +62:36:52.6 -- a known variable star
22:20:03.44 +62:14:56.1 -- not a known variable star
22:21:01.21 +60:27:28.3 -- not a known variable star
22:21:01.27 +59:55:03.8 -- a known variable star
22:21:24.90 +61:21:31.7 -- not a known variable star
22:21:29.15 +60:43:09.5 -- a known variable star
22:23:27.33 +61:46:07.8 -- a known variable star
22:24:21.64 +62:02:45.3 -- not a known variable star
22:24:56.51 +61:38:33.6 -- a known variable star
22:25:24.93 +61:18:04.5 -- a known variable star
22:27:22.59 +64:29:07.1 -- a known variable star
22:28:25.51 +62:26:43.0 -- not a known variable star
22:29:50.20 +65:19:21.9 -- a known variable star
22:31:11.72 +62:18:44.1 -- a known variable star
22:31:26.46 +62:54:57.0 -- a known variable star
22:31:29.28 +62:26:42.0 -- a known variable star
22:32:31.53 +63:34:54.0 -- a known variable star
22:33:25.13 +63:13:00.9 -- a known variable star
22:33:37.32 +63:35:08.5 -- a known variable star
22:36:20.36 +65:08:49.5 -- a known variable star
22:37:17.45 +63:57:16.3 -- a known variable star
22:37:40.37 +65:03:02.7 -- a known variable star
22:37:48.63 +63:15:40.3 -- a known variable star
22:40:33.48 +63:24:37.2 -- a known variable star
22:41:05.32 +64:16:04.3 -- not a known variable star
22:42:39.13 +63:01:33.8 -- a known variable star
22:45:34.10 +64:14:38.4 -- a known variable star
22:45:34.16 +63:37:04.4 -- a known variable star
22:47:21.63 +64:15:53.9 -- a known variable star
22:51:04.01 +64:16:22.2 -- a known variable star
23:08:21.84 +65:45:41.0 -- a known variable star
23:29:30.89 +64:51:22.8 -- a known variable star
Found 15 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
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106 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 106 (excluding asteroids and hot pixels, 15 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461186.72386322 -observatory V36
05:07:33.33 +24:43:52.1 Mercury (-1.1mag)
06:36:06.97 +24:58:52.3 Venus (-3.9mag)
02:12:10.17 +12:34:29.6 Mars (1.3mag)
07:38:01.01 +21:56:21.4 Jupiter (-1.9mag)
00:45:18.87 +02:25:57.6 Saturn (0.9mag)
03:57:04.73 +20:16:20.5 Uranus (5.8mag)
00:15:13.92 +00:11:34.8 Neptune (7.8mag)
20:33:56.19 -23:00:04.6 Pluto (14.5mag)
12:20:52.92 -06:00:14.9 Moon (-11.2mag)
-rw-r--r-- 1 apache apache 363 May 26 00:33 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461186.72386322:
07:37:55.74 +21:56:34.9 Io (5.9mag)
07:38:11.22 +21:55:52.2 Europa (6.1mag)
07:37:54.39 +21:56:44.9 Ganymede (5.5mag)
07:37:38.98 +21:57:15.5 Callisto (6.7mag)
07:39:05.98 +21:32:41.8 Himalia (15.5mag)
07:38:02.56 +21:56:18.4 Thebe (16.5mag)
07:39:24.29 +21:53:56.2 Elara (17.5mag)
07:39:28.94 +22:15:05.3 Pasiphae (17.7mag)
07:45:08.04 +21:57:11.1 Carme (18.8mag)
00:45:21.17 +02:25:37.8 Titan (8.7mag)
00:45:14.86 +02:26:05.1 Rhea (10.0mag)
00:45:41.61 +02:26:04.9 Iapetus (11.4mag)
00:45:33.57 +02:26:00.8 Hyperion (14.7mag)
00:46:16.46 +02:29:44.3 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 26 00:33 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461186.72386322:
17:17:18.64 -33:21:49.5 JWST
16:08:16.20 +51:46:21.3 Chandra
08:27:19.78 -46:21:55.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 26 00:33 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461186.72386322 -observatory V36
13:20:44.78 -27:03:21.7 14.4mag D/1884 O1 (Barnard)
06:37:26.63 +30:40:15.3 15.7mag D/1886 K1 (Brooks)
15:26:15.37 +01:21:03.9 14.6mag D/1895 Q1 (Swift)
05:28:14.71 +24:38:59.7 17.2mag D/1918 W1 (Schorr)
09:31:39.49 +14:30:32.8 17.9mag P/2009 WX51 (Catalina)
18:50:59.92 -31:39:37.9 13.7mag P/2010 H2 (Vales)
05:40:55.39 -68:15:59.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:22.22 +31:48:31.7 17.4mag C/2017 K2 (PANSTARRS)
17:19:50.72 +14:33:07.4 17.7mag C/2021 G2 (ATLAS)
23:14:32.67 +31:02:56.1 17.2mag C/2022 E2 (ATLAS)
05:18:03.64 +26:51:30.2 16.4mag C/2022 N2 (PANSTARRS)
09:20:59.34 +31:29:31.9 16.5mag C/2022 QE78 (ATLAS)
08:44:02.25 +03:13:15.6 17.6mag C/2022 R6 (PANSTARRS)
18:36:20.23 +21:12:23.0 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:25.94 -11:02:15.5 17.5mag P/2023 B1 (PANSTARRS)
22:16:12.54 +65:39:56.2 17.7mag C/2023 H5 (Lemmon)
18:17:00.59 -05:32:21.2 13.7mag C/2023 R1 (PANSTARRS)
13:39:39.21 +85:47:32.1 17.9mag C/2023 X2 (Lemmon)
06:53:29.11 +63:55:45.8 17.6mag C/2024 A1 (ATLAS)
06:26:57.28 +26:29:11.3 13.1mag C/2024 E1 (Wierzchos)
15:47:50.88 +12:12:49.9 17.3mag C/2024 G6 (ATLAS)
20:19:46.96 +27:11:13.2 14.1mag C/2024 J3 (ATLAS)
04:05:01.47 -17:11:58.9 16.1mag C/2024 T5 (ATLAS)
05:53:41.98 +36:48:26.3 17.9mag C/2025 J1 (Borisov)
11:45:38.49 +53:20:08.2 16.9mag C/2025 L1 (ATLAS)
06:25:00.33 -10:11:28.1 12.7mag C/2025 R3 (PANSTARRS)
12:40:56.77 +04:37:01.3 17.2mag C/2025 Y1 (ATLAS)
01:36:24.06 +42:23:09.5 15.7mag C/2026 B2 (Sun-Gao)
11:10:26.30 -08:58:06.8 16.3mag A/2026 E1
19:59:44.84 -08:07:26.0 9.5mag 10P/Tempel
14:18:44.25 -02:35:48.0 17.6mag 24P/Schaumasse
10:59:43.44 -00:51:55.3 15.9mag 29P/Schwassmann-Wachmann
10:51:20.82 -02:34:28.9 17.8mag 43P/Wolf-Harrington
02:51:31.57 +23:50:31.6 17.6mag 47P/Ashbrook-Jackson
08:32:20.09 +27:21:25.4 16.9mag 63P/Wild
00:14:55.59 -07:19:07.8 15.7mag 65P/Gunn
06:01:46.58 +31:41:31.8 16.5mag 76P/West-Kohoutek-Ikemura
02:38:03.89 +15:23:48.1 13.9mag 78P/Gehrels
00:51:15.18 +01:49:48.3 15.3mag 88P/Howell
04:12:54.40 +28:57:00.6 15.1mag 93P/Lovas
02:07:31.64 +25:21:40.1 17.9mag 114P/Wiseman-Skiff
06:20:05.45 +33:19:26.1 15.7mag 123P/West-Hartley
09:28:01.63 +20:15:03.0 16.4mag 124P/Mrkos
03:37:40.33 +18:17:33.8 16.4mag 128P/Shoemaker-Holt
04:07:39.37 +18:21:04.1 17.7mag 131P/Mueller
04:58:54.40 +19:38:37.6 13.0mag 141P/Machholz
05:01:32.99 +16:23:17.8 13.0mag 141P-A/Machholz
03:46:44.46 +13:43:41.4 10.6mag 141P-D/Machholz
02:48:13.76 -26:38:48.7 17.3mag 161P/Hartley-IRAS
03:00:01.86 +18:15:05.7 14.9mag 162P/SidingSpring
19:34:45.77 -01:42:05.1 17.6mag 169P/NEAT
17:02:19.31 -09:21:19.8 16.2mag 235P/LINEAR
07:05:07.76 +35:51:50.2 17.3mag 240P/NEAT
23:58:39.72 -07:45:15.3 16.7mag 260P/McNaught
03:30:06.65 +29:55:53.5 17.7mag 295P/LINEAR
22:05:40.10 -27:27:15.9 17.7mag 320P/McNaught
15:21:43.38 +08:21:36.2 17.4mag 391P/Kowalski
07:57:14.99 +21:02:16.0 17.8mag 450P/LONEOS
06:38:49.57 +42:35:04.3 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 26 00:33 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
-rw-r--r-- 1 apache apache 5.6K May 26 00:33 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 26 00:33 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:51:00.147 -40:59:30.34 AT 2026myv 2026-05-04.40 19.85
23:01:42.557 -37:41:28.08 AT 2026myu 2026-05-14.36 20.03
17:40:41.796 +55:46:35.59 AT 2026myt 2026-05-13.08 19.76
11:57:21.623 +08:17:50.60 AT 2026mys 2026-05-17.92 20.12
18:08:09.175 +24:46:16.68 AT 2026myr 2026-05-16.11 19.59
19:44:08.720 +05:58:44.85 AT 2026myq 2026-05-18.09 19.96
22:15:03.694 +37:18:03.97 SN 2026myp 2026-05-17.58 17.878
13:28:54.990 -05:49:13.50 AT 2026myo 2026-05-17.76 18.69
13:35:39.060 +60:25:07.59 AT 2026myn 2026-05-17.79 18.94
15:11:37.375 +27:04:22.10 AT 2026mym 2026-05-17.80 19.01
15:45:32.128 +08:10:41.12 AT 2026myl 2026-05-17.84 19.27
16:38:47.743 +40:50:56.52 AT 2026myk 2026-05-17.88 18.14
13:21:16.033 -33:01:10.62 AT 2026myj 2026-05-10.44 20.34
14:04:07.440 +19:21:36.43 AT 2026myi 2026-05-16.96 20.28
12:09:08.262 +13:15:11.92 AT 2026myh 2026-05-05.92 20.33
17:37:21.286 +36:24:32.57 AT 2026myg 2026-05-12.55 19.89
14:40:52.425 +10:22:25.10 AT 2026myf 2026-05-14.32 20.45
21:41:13.013 +64:08:54.76 AT 2026mye 2026-05-17.15 19.242
17:07:33.400 +35:38:40.42 AT 2026myd 2026-05-17.43 20.44
20:38:48.864 -58:53:21.28 AT 2026myc 2026-05-13.27 19.093
-rw-r--r-- 1 apache apache 30K May 26 00:33 tns_transients_list.txt
