This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y
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 08 13.3646 2461265.8646 10.71 19:36:24.38 +65:10:26.4
96.95156 19.93753 galactic Dra Second-epoch detections are separated by 0.2" and 6.8 pix
The object was found in VSX 2" ASASSN-V J193624.05+651027.5
Type: SR
# Max. Min./Amp. JD0 Period
11.750 V 12.320 V 2458656.11690 69.201095800000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:36:24.38 +65:10:26.4: 11.68 +/- 0.01 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:36:24.38 +65:10:26.4: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J193624.05+651027.5,2461265.8646,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193624.05+651027.5 20260813.3646 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.77 20:56:50.52 +60:47:43.6
97.90779 9.90928 galactic Cep Second-epoch detections are separated by 0.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:50.52 +60:47:43.6 (user input) | T | P | (position from user input) J-Ks=0.701+/-0.031 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:56:50.52 +60:47:43.6: 13.68 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:56:50.52 +60:47:43.6: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461265.8646,12.77,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.69 20:57:02.38 +61:18:01.7
98.31906 10.21200 galactic Cep Second-epoch detections are separated by 0.7" and 6.0 pix
The object was found in VSX 1" ASASSN-V J205702.38+611802.4
Type: L
# Max. Min./Amp. JD0 Period
13.950 V 14.120 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:57:02.38 +61:18:01.7: 13.73 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:57:02.38 +61:18:01.7: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 J205702.38+611802.4,2461265.8646,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205702.38+611802.4 20260813.3646 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.86 21:23:22.05 +59:48:19.9
99.40157 6.81426 galactic Cep Second-epoch detections are separated by 2.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:23:22.05 +59:48:19.9 (user input) | T | P | (position from user input) J-Ks=0.479+/-0.029 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:23:22.05 +59:48:19.9: 13.74 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:23:22.05 +59:48:19.9: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 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
target,2461265.8646,12.86,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.79 21:23:15.30 +59:49:21.6
99.40369 6.83638 galactic Cep Second-epoch detections are separated by 0.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:23:15.30 +59:49:21.6 (user input) | T | P | (position from user input) J-Ks=0.925+/-0.025 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:23:15.30 +59:49:21.6: 13.79 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:23:15.30 +59:49:21.6: 13.74 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.87 21:25:57.61 +59:36:56.1
99.50116 6.44934 galactic Cep Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:25:57.61 +59:36:56.1 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.028 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:25:57.61 +59:36:56.1: 13.79 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:25:57.61 +59:36:56.1: 13.89 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.83 +/- 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
target,2461265.8646,12.87,0.05,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
target 20260813.3646 12.87CV 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 08 13.3646 2461265.8646 12.85 20:59:44.23 +60:32:31.4
97.94068 9.47470 galactic Cep Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:44.23 +60:32:31.4 (user input) | T | P | (position from user input) J-Ks=1.464+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:59:44.23 +60:32:31.4: 13.79 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:59:44.23 +60:32:31.4: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 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
target,2461265.8646,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.82 21:24:27.49 +59:09:56.6
99.04656 6.26279 galactic Cep Second-epoch detections are separated by 0.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.1261+59.1620 | 21:24:27.49 +59:09:56.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.173+/-0.029 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:24:27.49 +59:09:56.6: 13.83 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:24:27.49 +59:09:56.6: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J321.1261+59.1620,2461265.8646,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.1261+59.1620 20260813.3646 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.84 20:55:59.56 +60:28:49.1
97.59364 9.78948 galactic Cep Second-epoch detections are separated by 0.9" and 6.3 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 | 20:55:59.56 +60:28:49.1 (user input) | T | P | (position from user input) J-Ks=0.485+/-0.033 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:55:59.56 +60:28:49.1: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:55:59.56 +60:28:49.1: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.84 21:03:27.39 +59:10:26.3
97.19678 8.22999 galactic Cep Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:27.39 +59:10:26.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:03:27.39 +59:10:26.3: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:03:27.39 +59:10:26.3: 13.79 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.90 21:30:03.89 +59:39:40.9
99.90863 6.12211 galactic Cep Second-epoch detections are separated by 2.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:03.89 +59:39:40.9 (user input) | T | P | (position from user input) J-Ks=1.356+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:30:03.89 +59:39:40.9: 13.84 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:30:03.89 +59:39:40.9: 13.89 +/- 0.07 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
target,2461265.8646,12.90,0.05,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
target 20260813.3646 12.90CV 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 08 13.3646 2461265.8646 12.95 20:55:44.69 +60:44:23.8
97.77793 9.97756 galactic Cep Second-epoch detections are separated by 0.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:44.69 +60:44:23.8 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.035 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:55:44.69 +60:44:23.8: 13.81 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:55:44.69 +60:44:23.8: 13.94 +/- 0.06 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
target,2461265.8646,12.95,0.05,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
target 20260813.3646 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.86 21:26:17.42 +59:27:42.6
99.42310 6.31016 galactic Cep Second-epoch detections are separated by 2.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:26:17.42 +59:27:42.6 (user input) | T | P | (position from user input) J-Ks=1.296+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:26:17.42 +59:27:42.6: 13.85 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:26:17.42 +59:27:42.6: 13.89 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.87 +/- 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
target,2461265.8646,12.86,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.88 21:09:25.31 +58:40:42.5
97.33988 7.32564 galactic Cep Second-epoch detections are separated by 2.0" and 6.3 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 | 21:09:25.31 +58:40:42.5 (user input) | T | P | (position from user input) J-Ks=1.076+/-0.033 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:09:25.31 +58:40:42.5: 13.85 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:09:25.31 +58:40:42.5: 13.98 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.94 21:01:46.36 +59:34:54.4
97.36679 8.65894 galactic Cep Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2190903710079310592 | 21:01:40.39 +59:34:54.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A3 1958TrRig...7...33A Cl Trumpler 37 1365 J-Ks=0.968+/-0.033 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:01:46.36 +59:34:54.4: 13.87 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:01:46.36 +59:34:54.4: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 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
Gaia DR3 2190903710079310592,2461265.8646,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2190903710079310592 20260813.3646 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.96 20:56:25.11 +61:00:21.8
98.03971 10.08286 galactic Cep Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:25.11 +61:00:21.8 (user input) | T | P | (position from user input) J-Ks=0.646+/-0.032 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:56:25.11 +61:00:21.8: 13.88 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:56:25.11 +61:00:21.8: 13.86 +/- 0.05 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
target,2461265.8646,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.00 21:00:17.49 +59:12:01.0
96.94962 8.55430 galactic Cep Second-epoch detections are separated by 6.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0773+59.2009 | 21:00:17.49 +59:12:01.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.941+/-0.032 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:00:17.49 +59:12:01.0: 14.05 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:00:17.49 +59:12:01.0: 14.02 +/- 0.07 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
ATO J315.0773+59.2009,2461265.8646,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0773+59.2009 20260813.3646 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.15 21:01:23.16 +59:16:47.5
97.10272 8.49960 galactic Cep Second-epoch detections are separated by 1.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:23.16 +59:16:47.5 (user input) | T | P | (position from user input) J-Ks=1.095+/-0.031 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:01:23.16 +59:16:47.5: 14.18 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:01:23.16 +59:16:47.5: 14.26 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.22 +/- 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
target,2461265.8646,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.15CV 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 08 13.3646 2461265.8646 12.22 21:01:45.02 +59:00:58.6
96.93141 8.29240 galactic Cep Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2190677240745430912 | 21:01:44.98 +59:00:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.300+/-0.036 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:01:45.02 +59:00:58.6: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:01:45.02 +59:00:58.6: 13.16 +/- 0.03 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
Gaia DR3 2190677240745430912,2461265.8646,12.22,0.05,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
Gaia DR3 2190677240745430912 20260813.3646 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 08 13.3646 2461265.8646 12.17 20:56:22.53 +60:33:25.7
97.68423 9.80187 galactic Cep Second-epoch detections are separated by 0.5" and 6.1 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 2194017630087138048 | 20:56:22.53 +60:33:26.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.609+/-0.038 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:56:22.53 +60:33:25.7: 13.20 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:56:22.53 +60:33:25.7: 13.19 +/- 0.03 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
Gaia DR3 2194017630087138048,2461265.8646,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2194017630087138048 20260813.3646 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.55 21:11:21.74 +58:49:49.2
97.62414 7.24269 galactic Cep Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.8412+58.8307 | 21:11:21.74 +58:49:49.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.418+/-0.074 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:11:21.74 +58:49:49.2: 13.38 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:11:21.74 +58:49:49.2: 13.49 +/- 0.05 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
ATO J317.8412+58.8307,2461265.8646,12.55,0.05,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
ATO J317.8412+58.8307 20260813.3646 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 08 13.3646 2461265.8646 12.46 21:24:37.01 +59:20:33.2
99.18614 6.37430 galactic Cep Second-epoch detections are separated by 1.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.1620+59.3491 | 21:24:37.01 +59:20:33.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.918+/-0.030 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:24:37.01 +59:20:33.2: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:24:37.01 +59:20:33.2: 13.40 +/- 0.04 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
ATO J321.1620+59.3491,2461265.8646,12.46,0.05,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
ATO J321.1620+59.3491 20260813.3646 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 08 13.3646 2461265.8646 12.51 19:43:58.65 +66:37:08.8
98.68494 19.77226 galactic Dra Second-epoch detections are separated by 4.4" and 6.0 pix
The object was found in VSX 1" Gaia DR3 2248663048749267200
Type: ROT
# Max. Min./Amp. JD0 Period
13.390 G 13.440 G 5.731400000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:43:58.65 +66:37:08.8: 13.50 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:43:58.65 +66:37:08.8: 13.48 +/- 0.04 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
Gaia DR3 2248663048749267200,2461265.8646,12.51,0.05,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
Gaia DR3 2248663048749267200 20260813.3646 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 08 13.3646 2461265.8646 12.49 19:38:26.91 +65:58:47.8
97.83112 20.04184 galactic Dra Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:38:26.91 +65:58:47.8 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.040 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:38:26.91 +65:58:47.8: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:38:26.91 +65:58:47.8: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461265.8646,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.73 21:00:50.07 +58:35:50.2
96.53219 8.10939 galactic Cep Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2044+58.5963 | 21:00:50.07 +58:35:50.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.001+/-0.034 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:00:50.07 +58:35:50.2: 13.64 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:00:50.07 +58:35:50.2: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J315.2044+58.5963,2461265.8646,12.73,0.05,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
ATO J315.2044+58.5963 20260813.3646 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 08 13.3646 2461265.8646 12.70 21:10:39.35 +58:55:53.9
97.63700 7.37846 galactic Cep Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:10:39.35 +58:55:53.9 (user input) | T | P | (position from user input) J-Ks=0.868+/-0.036 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:10:39.35 +58:55:53.9: 13.64 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:10:39.35 +58:55:53.9: 13.75 +/- 0.06 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
target,2461265.8646,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.74 21:09:22.48 +58:51:24.7
97.46879 7.45021 galactic Cep Second-epoch detections are separated by 2.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.3444+58.8502 | 21:09:22.48 +58:51:24.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:09:22.48 +58:51:24.7: 13.62 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:09:22.48 +58:51:24.7: 13.74 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J317.3444+58.8502,2461265.8646,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.3444+58.8502 20260813.3646 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.72 21:25:59.43 +59:39:01.8
99.52850 6.47161 galactic Cep Second-epoch detections are separated by 3.4" and 5.5 pix
The object was found in VSX 1" ASASSN-V J212559.49+593901.1
Type: SRS
# Max. Min./Amp. JD0 Period
14.960 g Y 0.320 g 2459480.80700 23.508000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:25:59.43 +59:39:01.8: 13.64 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:25:59.43 +59:39:01.8: 13.72 +/- 0.07 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 J212559.49+593901.1,2461265.8646,12.72,0.05,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
ASASSN-V J212559.49+593901.1 20260813.3646 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 08 13.3646 2461265.8646 12.51 21:24:08.16 +61:40:56.4
100.80592 8.07609 galactic Cep Second-epoch detections are separated by 0.8" and 5.7 pix
The object was found in VSX 3" NSVS J2124088+614059
Type: SR
# Max. Min./Amp. JD0 Period
15.562 g Y 0.368 g 2458206.02890 78.544830600000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:24:08.16 +61:40:56.4: 13.67 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:24:08.16 +61:40:56.4: 13.60 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2124088+614059,2461265.8646,12.51,0.05,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
NSVS J2124088+614059 20260813.3646 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 08 13.3646 2461265.8646 12.77 21:14:23.70 +58:51:51.9
97.91879 6.97906 galactic Cep Second-epoch detections are separated by 2.5" and 6.4 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 | 21:14:23.70 +58:51:51.9 (user input) | T | P | (position from user input) J-Ks=0.853+/-0.025 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:14:23.70 +58:51:51.9: 13.63 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:14:23.70 +58:51:51.9: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.77,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.75 20:59:34.78 +59:31:00.7
97.13445 8.82829 galactic Cep Second-epoch detections are separated by 0.8" and 6.3 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 | 20:59:34.78 +59:31:00.7 (user input) | T | P | (position from user input) J-Ks=0.966+/-0.033 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:59:34.78 +59:31:00.7: 13.62 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:59:34.78 +59:31:00.7: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461265.8646,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.45 19:24:13.08 +65:17:39.4
96.59523 21.17534 galactic Dra Second-epoch detections are separated by 3.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:24:13.08 +65:17:39.4 (user input) | T | P | (position from user input) J-Ks=0.629+/-0.027 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:24:13.08 +65:17:39.4: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:24:13.08 +65:17:39.4: 13.31 +/- 0.04 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
target,2461265.8646,12.45,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.71 20:59:57.54 +59:09:21.8
96.88765 8.55810 galactic Cep Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:57.54 +59:09:21.8 (user input) | T | P | (position from user input) J-Ks=0.496+/-0.033 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:59:57.54 +59:09:21.8: 13.63 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:59:57.54 +59:09:21.8: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.71,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.62 21:30:27.51 +59:37:56.0
99.92472 6.06673 galactic Cep Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.6189+59.6434 | 21:30:27.51 +59:37:56.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.962+/-0.030 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:30:27.51 +59:37:56.0: 13.64 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:30:27.51 +59:37:56.0: 13.52 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J322.6189+59.6434,2461265.8646,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.6189+59.6434 20260813.3646 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.61 20:00:13.62 +66:53:49.9
99.65927 18.43116 galactic Dra Second-epoch detections are separated by 2.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:13.62 +66:53:49.9 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.039 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:00:13.62 +66:53:49.9: 13.56 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:00:13.62 +66:53:49.9: 13.55 +/- 0.04 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
target,2461265.8646,12.61,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.62 21:08:53.44 +58:28:55.7
97.14647 7.24482 galactic Cep Second-epoch detections are separated by 1.0" and 6.3 pix
The object was found in VSX22" ZTF J210854.39+582916.9
Type: EW
# Max. Min./Amp. JD0 Period
16.365 r Y 0.205 r 2458582.94080 0.546603200000
ATTENTION: measured mag 12.62 is 3.5 mag brighter than the VSX record maximum brightness 16.16 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:08:53.44 +58:28:55.7: 13.54 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:08:53.44 +58:28:55.7: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J210854.39+582916.9,2461265.8646,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210854.39+582916.9 20260813.3646 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.60 21:13:29.33 +58:09:45.0
97.32220 6.58442 galactic Cep Second-epoch detections are separated by 2.3" and 5.8 pix
The object was found in VSX 0" ASASSN-V J211329.34+580945.2
Type: SR
# Max. Min./Amp. JD0 Period
13.810 V 14.170 V 2458277.66920 91.695806900000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:13:29.33 +58:09:45.0: 13.58 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:13:29.33 +58:09:45.0: 13.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 J211329.34+580945.2,2461265.8646,12.60,0.05,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 J211329.34+580945.2 20260813.3646 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 08 13.3646 2461265.8646 12.62 21:11:45.27 +59:06:01.3
97.85874 7.38873 galactic Cep Second-epoch detections are separated by 0.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.9387+59.1003 | 21:11:45.27 +59:06:01.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.178+/-0.033 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:11:45.27 +59:06:01.3: 13.56 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:11:45.27 +59:06:01.3: 13.55 +/- 0.05 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
ATO J317.9387+59.1003,2461265.8646,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.9387+59.1003 20260813.3646 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.59 20:59:11.34 +59:56:10.5
97.42679 9.13639 galactic Cep Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:11.34 +59:56:10.5 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.035 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:59:11.34 +59:56:10.5: 13.57 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:59:11.34 +59:56:10.5: 13.62 +/- 0.05 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
target,2461265.8646,12.59,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.56 19:39:10.71 +64:46:34.5
96.67761 19.51604 galactic Dra Second-epoch detections are separated by 1.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:39:10.71 +64:46:34.5 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.032 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:39:10.71 +64:46:34.5: 13.55 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:39:10.71 +64:46:34.5: 13.46 +/- 0.04 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
target,2461265.8646,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.40 19:31:27.58 +65:54:59.2
97.49316 20.68269 galactic Dra Second-epoch detections are separated by 3.6" and 6.4 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 | 19:31:27.58 +65:54:59.2 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.032 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:31:27.58 +65:54:59.2: 13.63 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:31:27.58 +65:54:59.2: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461265.8646,12.40,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.39 19:27:50.79 +65:55:45.9
97.37078 21.03325 galactic Dra Second-epoch detections are separated by 2.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:27:50.79 +65:55:45.9 (user input) | T | P | (position from user input) J-Ks=0.623+/-0.030 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:27:50.79 +65:55:45.9: 13.58 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:27:50.79 +65:55:45.9: 13.40 +/- 0.04 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
target,2461265.8646,12.39,0.05,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
target 20260813.3646 12.39CV 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 08 13.3646 2461265.8646 12.21 19:29:30.80 +66:01:24.3
97.52717 20.90561 galactic Dra Second-epoch detections are separated by 1.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:29:30.80 +66:01:24.3 (user input) | T | P | (position from user input) J-Ks=0.706+/-0.029 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:29:30.80 +66:01:24.3: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:29:30.80 +66:01:24.3: 13.12 +/- 0.03 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
target,2461265.8646,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.21CV 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 08 13.3646 2461265.8646 12.49 20:57:55.84 +60:59:51.1
98.15152 9.93611 galactic Cep Second-epoch detections are separated by 1.2" and 6.0 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 2195578794860568448 | 20:57:55.82 +60:59:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.304+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:57:55.84 +60:59:51.1: 13.45 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:57:55.84 +60:59:51.1: 13.43 +/- 0.04 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 2195578794860568448,2461265.8646,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2195578794860568448 20260813.3646 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.21 19:27:30.14 +66:05:06.0
97.51523 21.11846 galactic Dra Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:27:30.14 +66:05:06.0 (user input) | T | P | (position from user input) J-Ks=0.688+/-0.030 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:27:30.14 +66:05:06.0: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:27:30.14 +66:05:06.0: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.21CV 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 08 13.3646 2461265.8646 12.60 21:09:32.55 +58:54:52.0
97.52646 7.47292 galactic Cep Second-epoch detections are separated by 2.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.3695+58.9211 | 21:09:32.55 +58:54:52.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.969+/-0.046 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:09:32.55 +58:54:52.0: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:09:32.55 +58:54:52.0: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J317.3695+58.9211,2461265.8646,12.60,0.05,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
ATO J317.3695+58.9211 20260813.3646 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 08 13.3646 2461265.8646 12.54 20:59:55.88 +59:11:31.6
96.91312 8.58414 galactic Cep Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:55.88 +59:11:31.6 (user input) | T | P | (position from user input) J-Ks=0.801+/-0.033 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:59:55.88 +59:11:31.6: 13.44 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:59:55.88 +59:11:31.6: 13.55 +/- 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
target,2461265.8646,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.54CV 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 08 13.3646 2461265.8646 12.40 19:29:26.70 +66:02:10.2
97.53745 20.91649 galactic Dra Second-epoch detections are separated by 7.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:29:26.70 +66:02:10.2 (user input) | T | P | (position from user input) J-Ks=0.508+/-0.030 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:29:26.70 +66:02:10.2: 13.49 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:29:26.70 +66:02:10.2: 13.37 +/- 0.04 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
target,2461265.8646,12.40,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.33 19:40:01.58 +66:22:20.4
98.28192 20.04151 galactic Dra Second-epoch detections are separated by 6.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:40:01.58 +66:22:20.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:40:01.58 +66:22:20.4: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:40:01.58 +66:22:20.4: 13.28 +/- 0.04 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
target,2461265.8646,12.33,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.34 19:30:48.17 +66:22:02.2
97.92070 20.90156 galactic Dra Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2242791209980932480 | 19:30:53.25 +66:21:37.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.421+/-0.027 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:30:48.17 +66:22:02.2: 13.48 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:30:48.17 +66:22:02.2: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2242791209980932480,2461265.8646,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2242791209980932480 20260813.3646 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.52 19:47:44.01 +66:38:34.4
98.86468 19.43967 galactic Dra Second-epoch detections are separated by 4.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:47:44.01 +66:38:34.4 (user input) | T | P | (position from user input) J-Ks=0.536+/-0.035 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:47:44.01 +66:38:34.4: 13.44 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:47:44.01 +66:38:34.4: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.52,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.37 19:31:14.74 +65:55:03.9
97.48631 20.70360 galactic Dra Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:31:14.74 +65:55:03.9 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.033 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:31:14.74 +65:55:03.9: 13.47 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:31:14.74 +65:55:03.9: 13.34 +/- 0.04 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
target,2461265.8646,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.29 19:24:50.71 +65:44:49.2
97.07690 21.26232 galactic Dra Second-epoch detections are separated by 4.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:24:50.71 +65:44:49.2 (user input) | T | P | (position from user input) J-Ks=0.117+/-0.034 (A)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:24:50.71 +65:44:49.2: 13.53 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:24:50.71 +65:44:49.2: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.29,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.52 21:23:40.72 +58:59:22.6
98.85030 6.20821 galactic Cep Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:23:40.72 +58:59:22.6 (user input) | T | P | (position from user input) J-Ks=0.471+/-0.029 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:23:40.72 +58:59:22.6: 13.40 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:23:40.72 +58:59:22.6: 13.51 +/- 0.05 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
target,2461265.8646,12.52,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.34 20:44:14.93 +59:07:57.8
95.59131 10.11399 galactic Cep Second-epoch detections are separated by 0.9" and 6.3 pix
The object was found in VSX 2" NSVS J2044147+590757
Type: L:
# Max. Min./Amp. JD0 Period
10.567 R1 Y 0.423 R1 96.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:44:14.93 +59:07:57.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:44:14.93 +59:07:57.8: 13.52 +/- 0.04 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
NSVS J2044147+590757,2461265.8646,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2044147+590757 20260813.3646 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.27 19:30:40.53 +66:21:20.5
97.90435 20.90955 galactic Dra Second-epoch detections are separated by 1.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:30:40.53 +66:21:20.5 (user input) | T | P | (position from user input) J-Ks=0.304+/-0.028 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:30:40.53 +66:21:20.5: 13.45 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:30:40.53 +66:21:20.5: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.27,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.46 21:03:05.67 +59:17:33.8
97.25664 8.34284 galactic Cep Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:05.67 +59:17:33.8 (user input) | T | P | (position from user input) J-Ks=1.013+/-0.032 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:03:05.67 +59:17:33.8: 13.38 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:03:05.67 +59:17:33.8: 13.44 +/- 0.04 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
target,2461265.8646,12.46,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.44 19:26:01.40 +65:26:32.5
96.81172 21.04679 galactic Dra Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:26:01.40 +65:26:32.5 (user input) | T | P | (position from user input) J-Ks=0.449+/-0.032 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:26:01.40 +65:26:32.5: 13.44 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:26:01.40 +65:26:32.5: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.44,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.35 19:27:20.84 +65:33:47.2
96.98289 20.95799 galactic Dra Second-epoch detections are separated by 0.8" and 7.0 pix
The object was found in VSX18" Gaia DR3 2242649372980527744
Type: ROT
# Max. Min./Amp. JD0 Period
14.870 G 14.920 G K
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:27:20.84 +65:33:47.2: 13.39 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:27:20.84 +65:33:47.2: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2242649372980527744,2461265.8646,12.35,0.05,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
Gaia DR3 2242649372980527744 20260813.3646 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 08 13.3646 2461265.8646 13.04 20:56:38.83 +60:14:56.7
97.46469 9.58007 galactic Cep Second-epoch detections are separated by 5.6" and 6.9 pix
The object was found in VSX11" Gaia DR3 2193997735798417920
Type: ROT
# Max. Min./Amp. JD0 Period
14.580 G 14.610 G G
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:56:38.83 +60:14:56.7: 14.15 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:56:38.83 +60:14:56.7: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 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
Gaia DR3 2193997735798417920,2461265.8646,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2193997735798417920 20260813.3646 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.38 19:35:57.50 +66:20:20.7
98.08810 20.40810 galactic Dra Second-epoch detections are separated by 1.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:35:57.50 +66:20:20.7 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.028 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:35:57.50 +66:20:20.7: 13.36 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:35:57.50 +66:20:20.7: 13.21 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.38,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.47 20:56:00.54 +60:25:05.7
97.54626 9.74855 galactic Cep Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:00.54 +60:25:05.7 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.033 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:56:00.54 +60:25:05.7: 13.36 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:56:00.54 +60:25:05.7: 13.52 +/- 0.04 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
target,2461265.8646,12.47,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.35 21:10:18.73 +58:47:48.7
97.50655 7.32015 galactic Cep Second-epoch detections are separated by 0.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.5759+58.8009 | 21:10:18.73 +58:47:48.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.085+/-0.037 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:10:18.73 +58:47:48.7: 13.32 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:10:18.73 +58:47:48.7: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J317.5759+58.8009,2461265.8646,12.35,0.05,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
ATO J317.5759+58.8009 20260813.3646 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 08 13.3646 2461265.8646 12.29 19:28:39.36 +66:16:56.7
97.75649 21.07517 galactic Dra Second-epoch detections are separated by 2.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:28:39.36 +66:16:56.7 (user input) | T | P | (position from user input) J-Ks=0.560+/-0.028 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:28:39.36 +66:16:56.7: 13.37 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:28:39.36 +66:16:56.7: 13.34 +/- 0.04 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
target,2461265.8646,12.29,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.50 21:23:36.40 +59:37:50.8
99.29882 6.66923 galactic Cep Second-epoch detections are separated by 1.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.8973+59.6329 | 21:23:36.40 +59:37:50.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.334+/-0.032 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:23:36.40 +59:37:50.8: 13.32 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:23:36.40 +59:37:50.8: 13.48 +/- 0.05 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
ATO J320.8973+59.6329,2461265.8646,12.50,0.05,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
ATO J320.8973+59.6329 20260813.3646 12.50CV 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 08 13.3646 2461265.8646 12.35 21:23:00.95 +59:19:20.8
99.02614 6.50393 galactic Cep Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:23:00.95 +59:19:20.8 (user input) | T | P | (position from user input) J-Ks=1.202+/-0.029 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:23:00.95 +59:19:20.8: 13.35 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:23:00.95 +59:19:20.8: 13.45 +/- 0.05 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
target,2461265.8646,12.35,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.36 19:38:22.71 +66:00:48.3
97.86134 20.06095 galactic Dra Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:38:22.71 +66:00:48.3 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.035 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:38:22.71 +66:00:48.3: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:38:22.71 +66:00:48.3: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.38 19:37:48.01 +66:31:57.0
98.35193 20.30753 galactic Dra Second-epoch detections are separated by 2.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:37:48.01 +66:31:57.0 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.033 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:37:48.01 +66:31:57.0: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:37:48.01 +66:31:57.0: 13.23 +/- 0.03 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
target,2461265.8646,12.38,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.44 20:56:58.40 +60:16:13.3
97.50746 9.56244 galactic Cep Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:58.40 +60:16:13.3 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.034 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:56:58.40 +60:16:13.3: 13.31 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:56:58.40 +60:16:13.3: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 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
target,2461265.8646,12.44,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.38 19:37:37.78 +66:19:57.0
98.14704 20.24962 galactic Dra Second-epoch detections are separated by 2.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:37:37.78 +66:19:57.0 (user input) | T | P | (position from user input) J-Ks=0.208+/-0.037 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:37:37.78 +66:19:57.0: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:37:37.78 +66:19:57.0: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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
target,2461265.8646,12.38,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.27 19:26:19.93 +65:28:02.2
96.84836 21.02488 galactic Dra Second-epoch detections are separated by 1.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:26:19.93 +65:28:02.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:26:19.93 +65:28:02.2: 13.32 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:26:19.93 +65:28:02.2: 13.21 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.27,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.14 20:42:02.70 +58:55:19.5
95.24709 10.21380 galactic Cep Second-epoch detections are separated by 0.6" and 6.4 pix
The object was found in VSX 1" V1034 Cep
Type: SRB
# Max. Min./Amp. JD0 Period
13.680 V 14.800 V 96.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:42:02.70 +58:55:19.5: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:42:02.70 +58:55:19.5: 13.28 +/- 0.03 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
V1034 Cep,2461265.8646,12.14,0.05,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
V1034 Cep 20260813.3646 12.14CV 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 08 13.3646 2461265.8646 12.28 19:26:16.35 +66:01:21.1
97.40752 21.21534 galactic Dra Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:26:16.35 +66:01:21.1 (user input) | T | P | (position from user input) J-Ks=0.622+/-0.028 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:26:16.35 +66:01:21.1: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:26:16.35 +66:01:21.1: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 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,2461265.8646,12.28,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.28 19:33:17.80 +65:57:04.3
97.59850 20.51973 galactic Dra Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:33:17.80 +65:57:04.3 (user input) | T | P | (position from user input) J-Ks=0.575+/-0.029 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:33:17.80 +65:57:04.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:33:17.80 +65:57:04.3: 13.10 +/- 0.03 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
target,2461265.8646,12.28,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.30 19:32:31.11 +65:59:09.8
97.60331 20.60616 galactic Dra Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:32:31.11 +65:59:09.8 (user input) | T | P | (position from user input) J-Ks=0.599+/-0.026 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:32:31.11 +65:59:09.8: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:32:31.11 +65:59:09.8: 13.21 +/- 0.03 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
target,2461265.8646,12.30,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.17 19:28:25.73 +66:09:11.5
97.61786 21.05308 galactic Dra Second-epoch detections are separated by 1.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:28:25.73 +66:09:11.5 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.028 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:28:25.73 +66:09:11.5: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:28:25.73 +66:09:11.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.23 19:42:45.67 +66:24:52.4
98.43462 19.80458 galactic Dra Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:42:45.67 +66:24:52.4 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.033 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:42:45.67 +66:24:52.4: 13.25 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:42:45.67 +66:24:52.4: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 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
target,2461265.8646,12.23,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 13.28 20:57:36.85 +60:49:12.7
97.98805 9.85248 galactic Cep Second-epoch detections are separated by 2.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:36.85 +60:49:12.7 (user input) | T | P | (position from user input) J-Ks=1.650+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:57:36.85 +60:49:12.7: 14.33 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:57:36.85 +60:49:12.7: 14.53 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.40 +/- 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
target,2461265.8646,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.28CV 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 08 13.3646 2461265.8646 12.34 19:38:27.19 +65:50:28.9
97.69453 19.98954 galactic Dra Second-epoch detections are separated by 2.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:38:27.19 +65:50:28.9 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.036 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:38:27.19 +65:50:28.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:38:27.19 +65:50:28.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.13 19:27:21.85 +65:54:08.4
97.32572 21.07048 galactic Dra Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:27:21.85 +65:54:08.4 (user input) | T | P | (position from user input) J-Ks=0.282+/-0.030 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:27:21.85 +65:54:08.4: 13.24 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:27:21.85 +65:54:08.4: 13.01 +/- 0.03 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
target,2461265.8646,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.17 19:37:29.60 +66:29:52.9
98.30576 20.32327 galactic Dra Second-epoch detections are separated by 0.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:37:29.60 +66:29:52.9 (user input) | T | P | (position from user input) J-Ks=0.646+/-0.033 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:37:29.60 +66:29:52.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:37:29.60 +66:29:52.9: 13.15 +/- 0.03 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
target,2461265.8646,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.26 19:38:40.00 +65:07:39.1
97.00047 19.69997 galactic Dra Second-epoch detections are separated by 1.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:38:40.00 +65:07:39.1 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.033 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:38:40.00 +65:07:39.1: 13.11 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:38:40.00 +65:07:39.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.26,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.23 19:23:56.39 +65:30:47.2
96.80695 21.27421 galactic Dra Second-epoch detections are separated by 1.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:23:56.39 +65:30:47.2 (user input) | T | P | (position from user input) J-Ks=0.274+/-0.032 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:23:56.39 +65:30:47.2: 13.26 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:23:56.39 +65:30:47.2: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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
target,2461265.8646,12.23,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.20 19:43:54.83 +66:28:24.4
98.53980 19.72131 galactic Dra Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:43:54.83 +66:28:24.4 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.034 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:43:54.83 +66:28:24.4: 13.13 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:43:54.83 +66:28:24.4: 13.08 +/- 0.03 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
target,2461265.8646,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.03 19:30:42.54 +66:01:17.3
97.56998 20.79090 galactic Dra Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:30:42.54 +66:01:17.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:30:42.54 +66:01:17.3: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:30:42.54 +66:01:17.3: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.10 19:38:12.45 +66:31:00.6
98.35238 20.26405 galactic Dra Second-epoch detections are separated by 2.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:38:12.45 +66:31:00.6 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.032 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:38:12.45 +66:31:00.6: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:38:12.45 +66:31:00.6: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.10,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 13.05 20:58:02.21 +60:39:58.5
97.90136 9.71439 galactic Cep Second-epoch detections are separated by 2.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:02.21 +60:39:58.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:58:02.21 +60:39:58.5: 14.01 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:58:02.21 +60:39:58.5: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,13.05,0.05,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
target 20260813.3646 13.05CV 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 08 13.3646 2461265.8646 12.09 21:25:07.48 +59:52:30.9
99.60880 6.70832 galactic Cep Second-epoch detections are separated by 0.4" and 5.9 pix
The object was found in VSX 1" ZTF J212507.54+595231.4
Type: SR
# Max. Min./Amp. JD0 Period
14.504 g Y 0.174 g 2458593.88490 28.963921600000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:25:07.48 +59:52:30.9: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:25:07.48 +59:52:30.9: 13.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 J212507.54+595231.4,2461265.8646,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212507.54+595231.4 20260813.3646 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.10 19:29:28.25 +65:54:31.4
97.41024 20.87038 galactic Dra Second-epoch detections are separated by 2.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2242752413536616960 | 19:29:28.04 +65:54:31.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.801+/-0.025 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:29:28.25 +65:54:31.4: 13.11 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:29:28.25 +65:54:31.4: 12.95 +/- 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
Gaia DR3 2242752413536616960,2461265.8646,12.10,0.05,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
Gaia DR3 2242752413536616960 20260813.3646 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 08 13.3646 2461265.8646 13.12 21:01:31.78 +59:14:23.1
97.08404 8.45955 galactic Cep Second-epoch detections are separated by 2.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:31.78 +59:14:23.1 (user input) | T | P | (position from user input) J-Ks=1.060+/-0.036 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:01:31.78 +59:14:23.1: 14.30 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:01:31.78 +59:14:23.1: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.21 +/- 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
target,2461265.8646,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.12CV 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 08 13.3646 2461265.8646 12.04 19:37:34.18 +66:27:06.3
98.26286 20.29916 galactic Dra Second-epoch detections are separated by 2.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:37:34.18 +66:27:06.3 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.034 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:37:34.18 +66:27:06.3: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:37:34.18 +66:27:06.3: 12.97 +/- 0.03 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
target,2461265.8646,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.88 19:31:54.56 +66:01:02.8
97.61141 20.67519 galactic Dra Second-epoch detections are separated by 1.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:31:54.56 +66:01:02.8 (user input) | T | P | (position from user input) J-Ks=0.270+/-0.029 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:31:54.56 +66:01:02.8: 13.03 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:31:54.56 +66:01:02.8: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 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
target,2461265.8646,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.95 19:30:03.39 +65:57:08.9
97.47617 20.82935 galactic Dra Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:30:03.39 +65:57:08.9 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.033 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:30:03.39 +65:57:08.9: 13.02 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:30:03.39 +65:57:08.9: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,11.95,0.05,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
target 20260813.3646 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
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.12 19:36:56.71 +66:01:07.1
97.80897 20.19815 galactic Dra Second-epoch detections are separated by 3.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:36:56.71 +66:01:07.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:36:56.71 +66:01:07.1: 12.99 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:36:56.71 +66:01:07.1: 13.05 +/- 0.03 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
target,2461265.8646,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.12CV 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 08 13.3646 2461265.8646 11.98 19:31:50.63 +66:12:14.3
97.79572 20.74671 galactic Dra Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2242786193459087744 | 19:31:50.60 +66:12:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.030 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:31:50.63 +66:12:14.3: 12.98 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:31:50.63 +66:12:14.3: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2242786193459087744,2461265.8646,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2242786193459087744 20260813.3646 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 08 13.3646 2461265.8646 11.85 19:24:21.96 +65:41:39.7
97.00624 21.29167 galactic Dra Second-epoch detections are separated by 3.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2254670299247424000 | 19:24:22.07 +65:41:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.248+/-0.029 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:24:21.96 +65:41:39.7: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:24:21.96 +65:41:39.7: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2254670299247424000,2461265.8646,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2254670299247424000 20260813.3646 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.19 20:58:39.33 +60:42:44.9
97.98657 9.68585 galactic Cep Second-epoch detections are separated by 1.5" and 6.3 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 | 20:58:39.33 +60:42:44.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:58:39.33 +60:42:44.9: 14.21 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:58:39.33 +60:42:44.9: 14.24 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.22 +/- 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
target,2461265.8646,13.19,0.05,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
target 20260813.3646 13.19CV 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 08 13.3646 2461265.8646 11.89 20:57:41.34 +59:29:45.2
96.96202 8.99844 galactic Cep Second-epoch detections are separated by 1.2" and 6.3 pix
The object was found in VSX 1" GSC 03964-00867
Type: IB
# Max. Min./Amp. JD0 Period
10.800 R1 11.050 R1
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:57:41.34 +59:29:45.2: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:57:41.34 +59:29:45.2: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 03964-00867,2461265.8646,11.89,0.05,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
GSC 03964-00867 20260813.3646 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 08 13.3646 2461265.8646 11.95 19:38:37.88 +66:21:08.3
98.20634 20.16364 galactic Dra Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2248746641693915392 | 19:38:37.86 +66:21:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.791+/-0.031 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:38:37.88 +66:21:08.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:38:37.88 +66:21:08.3: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2248746641693915392,2461265.8646,11.95,0.05,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
Gaia DR3 2248746641693915392 20260813.3646 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
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.66 21:11:52.50 +59:01:04.1
97.80822 7.32131 galactic Cep Second-epoch detections are separated by 0.5" and 6.1 pix
The object was found in VSX 3" NSVS J2111527+590102
Type: L:
# Max. Min./Amp. JD0 Period
10.630 R1 Y 0.432 R1 119.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:11:52.50 +59:01:04.1: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:11:52.50 +59:01:04.1: 12.84 +/- 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
NSVS J2111527+590102,2461265.8646,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2111527+590102 20260813.3646 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.16 20:55:55.86 +60:31:40.0
97.62600 9.82546 galactic Cep Second-epoch detections are separated by 1.7" and 6.2 pix
The object was found in VSX 1" Gaia DR3 2194062984941706496
Type: ROT
# Max. Min./Amp. JD0 Period
14.040 G 14.080 G K
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:55:55.86 +60:31:40.0: 14.16 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:55:55.86 +60:31:40.0: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 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
Gaia DR3 2194062984941706496,2461265.8646,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2194062984941706496 20260813.3646 13.16CV 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 08 13.3646 2461265.8646 11.97 19:49:42.01 +66:41:57.4
99.00303 19.28458 galactic Dra Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2248628723370801920 | 19:49:41.97 +66:41:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.347+/-0.033 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:49:42.01 +66:41:57.4: 12.79 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:49:42.01 +66:41:57.4: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2248628723370801920,2461265.8646,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2248628723370801920 20260813.3646 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.09 21:10:26.67 +59:03:25.0
97.71161 7.48319 galactic Cep Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:10:26.67 +59:03:25.0 (user input) | T | P | (position from user input) J-Ks=1.066+/-0.037 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:10:26.67 +59:03:25.0: 14.19 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:10:26.67 +59:03:25.0: 14.13 +/- 0.08 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
target,2461265.8646,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.14 21:10:02.27 +58:50:47.2
97.51928 7.37981 galactic Cep Second-epoch detections are separated by 2.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:10:02.27 +58:50:47.2 (user input) | T | P | (position from user input) J-Ks=0.225+/-0.043 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:10:02.27 +58:50:47.2: 14.18 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:10:02.27 +58:50:47.2: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.20 +/- 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
target,2461265.8646,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.14CV 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 08 13.3646 2461265.8646 11.88 21:22:53.63 +59:37:09.5
99.22646 6.72478 galactic Cep Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2191654058051818240 | 21:22:53.86 +59:37:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.181+/-0.027 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:22:53.63 +59:37:09.5: 12.79 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:22:53.63 +59:37:09.5: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2191654058051818240,2461265.8646,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2191654058051818240 20260813.3646 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.98 20:49:05.61 +58:53:57.4
95.79064 9.47786 galactic Cep Second-epoch detections are separated by 0.3" and 6.4 pix
The object was found in VSX 0" DR Cep
Type: DCEP
# Max. Min./Amp. JD0 Period
12.300 V 13.380 V 2430704.82000 19.065880000000 F5p
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:49:05.61 +58:53:57.4: 12.73 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:49:05.61 +58:53:57.4: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DR Cep,2461265.8646,11.98,0.05,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
DR Cep 20260813.3646 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 08 13.3646 2461265.8646 11.77 19:31:05.29 +66:10:19.2
97.73526 20.80707 galactic Dra Second-epoch detections are separated by 3.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2242784715990322176 | 19:31:05.30 +66:10:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.317+/-0.029 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:31:05.29 +66:10:19.2: 12.83 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:31:05.29 +66:10:19.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2242784715990322176,2461265.8646,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2242784715990322176 20260813.3646 11.77CV 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 08 13.3646 2461265.8646 13.05 21:20:51.12 +59:14:08.1
98.76809 6.63882 galactic Cep Second-epoch detections are separated by 0.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:20:51.12 +59:14:08.1 (user input) | T | P | (position from user input) J-Ks=0.672+/-0.026 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:20:51.12 +59:14:08.1: 14.17 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:20:51.12 +59:14:08.1: 14.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,13.05,0.05,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
target 20260813.3646 13.05CV 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 08 13.3646 2461265.8646 13.05 21:01:53.55 +59:23:58.7
97.23714 8.52867 galactic Cep Second-epoch detections are separated by 1.0" and 6.3 pix
The object was found in VSX 1" ASASSN-V J210153.59+592359.5
Type: SR
# Max. Min./Amp. JD0 Period
15.730 g Y 0.520 g 2458755.66100 39.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:01:53.55 +59:23:58.7: 14.12 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:01:53.55 +59:23:58.7: 14.21 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 J210153.59+592359.5,2461265.8646,13.05,0.05,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 J210153.59+592359.5 20260813.3646 13.05CV 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 08 13.3646 2461265.8646 11.53 19:23:54.10 +65:56:11.8
97.23570 21.41527 galactic Dra Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2254683287228690688 | 19:23:54.09 +65:56:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.347+/-0.028 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:23:54.10 +65:56:11.8: 12.70 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:23:54.10 +65:56:11.8: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 2254683287228690688,2461265.8646,11.53,0.05,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
Gaia DR3 2254683287228690688 20260813.3646 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 08 13.3646 2461265.8646 12.99 21:03:26.39 +58:57:08.5
97.02655 8.08604 galactic Cep Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.8594+58.9522 | 21:03:26.39 +58:57:08.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.340+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:03:26.39 +58:57:08.5: 14.13 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:03:26.39 +58:57:08.5: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.17 +/- 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
ATO J315.8594+58.9522,2461265.8646,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.8594+58.9522 20260813.3646 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.64 19:31:04.00 +65:56:51.5
97.50946 20.73113 galactic Dra Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2242763790909505920 | 19:31:05.82 +65:56:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.806+/-0.029 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:31:04.00 +65:56:51.5: 12.63 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:31:04.00 +65:56:51.5: 12.58 +/- 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
Gaia DR3 2242763790909505920,2461265.8646,11.64,0.05,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 2242763790909505920 20260813.3646 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 08 13.3646 2461265.8646 13.03 21:00:31.82 +58:27:53.3
96.40447 8.05341 galactic Cep Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1322+58.4645 | 21:00:31.82 +58:27:53.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.522+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:00:31.82 +58:27:53.3: 14.12 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:00:31.82 +58:27:53.3: 14.27 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.18 +/- 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
ATO J315.1322+58.4645,2461265.8646,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1322+58.4645 20260813.3646 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.96 21:09:59.60 +58:45:20.1
97.44773 7.32278 galactic Cep Second-epoch detections are separated by 1.0" and 6.3 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 | 21:09:59.60 +58:45:20.1 (user input) | T | P | (position from user input) J-Ks=0.769+/-0.034 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:09:59.60 +58:45:20.1: 14.10 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:09:59.60 +58:45:20.1: 14.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 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
target,2461265.8646,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.40 19:23:32.20 +65:56:25.4
97.22666 21.45171 galactic Dra Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2254683149789736064 | 19:23:32.07 +65:56:25.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.649+/-0.028 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:23:32.20 +65:56:25.4: 12.48 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:23:32.20 +65:56:25.4: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2254683149789736064,2461265.8646,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2254683149789736064 20260813.3646 11.40CV 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 08 13.3646 2461265.8646 11.53 19:30:22.58 +66:03:40.6
97.59744 20.83635 galactic Dra Second-epoch detections are separated by 0.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2242778428158134784 | 19:30:22.52 +66:03:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.320+/-0.030 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:30:22.58 +66:03:40.6: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:30:22.58 +66:03:40.6: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2242778428158134784,2461265.8646,11.53,0.05,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
Gaia DR3 2242778428158134784 20260813.3646 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 08 13.3646 2461265.8646 13.13 20:57:18.13 +60:16:59.1
97.54376 9.53917 galactic Cep Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:18.13 +60:16:59.1 (user input) | T | P | (position from user input) J-Ks=0.593+/-0.033 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:57:18.13 +60:16:59.1: 14.11 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:57:18.13 +60:16:59.1: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 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
target,2461265.8646,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.61 21:24:39.32 +59:43:01.8
99.45468 6.63730 galactic Cep Second-epoch detections are separated by 0.2" and 5.9 pix
The object was found in VSX 2" V0542 Cep
Type: SR:
# Max. Min./Amp. JD0 Period
13.000 V 14.300 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:24:39.32 +59:43:01.8: 12.53 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:24:39.32 +59:43:01.8: 12.57 +/- 0.02 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
V0542 Cep,2461265.8646,11.61,0.05,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
V0542 Cep 20260813.3646 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 08 13.3646 2461265.8646 13.06 21:09:09.15 +58:40:25.0
97.31251 7.34826 galactic Cep Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:09:09.15 +58:40:25.0 (user input) | T | P | (position from user input) J-Ks=1.014+/-0.034 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:09:09.15 +58:40:25.0: 14.12 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:09:09.15 +58:40:25.0: 14.16 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.14 +/- 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
target,2461265.8646,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.95 21:25:05.78 +59:49:01.9
99.56521 6.66948 galactic Cep Second-epoch detections are separated by 2.9" and 6.4 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 | 21:25:05.78 +59:49:01.9 (user input) | T | P | (position from user input) J-Ks=0.459+/-0.030 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:25:05.78 +59:49:01.9: 14.10 +/- 0.09 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:25:05.78 +59:49:01.9: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.02 +/- 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
target,2461265.8646,12.95,0.05,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
target 20260813.3646 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.54 19:30:53.45 +66:21:35.8
97.91659 20.89075 galactic Dra Second-epoch detections are separated by 2.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2242791209980932480 | 19:30:53.25 +66:21:37.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.884+/-0.027 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:30:53.45 +66:21:35.8: 12.54 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:30:53.45 +66:21:35.8: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2242791209980932480,2461265.8646,11.54,0.05,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
Gaia DR3 2242791209980932480 20260813.3646 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 08 13.3646 2461265.8646 11.50 19:30:16.62 +66:01:35.2
97.55874 20.83380 galactic Dra Second-epoch detections are separated by 0.3" and 6.8 pix
The object was found in VSX 0" Gaia DR3 2242776881969879936
Type: ROT
# Max. Min./Amp. JD0 Period
11.810 G 11.880 G G
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:30:16.62 +66:01:35.2: 12.53 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:30:16.62 +66:01:35.2: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2242776881969879936,2461265.8646,11.50,0.05,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
Gaia DR3 2242776881969879936 20260813.3646 11.50CV 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 08 13.3646 2461265.8646 12.96 21:01:00.08 +58:53:02.6
96.76645 8.27953 galactic Cep Second-epoch detections are separated by 3.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2469+58.8847 | 21:00:54.46 +58:53:13.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:01:00.08 +58:53:02.6: 14.08 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:01:00.08 +58:53:02.6: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 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
ATO J315.2469+58.8847,2461265.8646,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.2469+58.8847 20260813.3646 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 11.55 19:23:26.61 +66:08:26.9
97.42740 21.52497 galactic Dra Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2254779425775180672 | 19:23:26.55 +66:08:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.400+/-0.028 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:23:26.61 +66:08:26.9: 12.61 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:23:26.61 +66:08:26.9: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2254779425775180672,2461265.8646,11.55,0.05,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 2254779425775180672 20260813.3646 11.55CV 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 08 13.3646 2461265.8646 11.40 19:27:12.09 +66:17:02.6
97.70558 21.21351 galactic Dra Second-epoch detections are separated by 0.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2254796571282155904 | 19:27:11.65 +66:17:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:27:12.09 +66:17:02.6: 12.43 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:27:12.09 +66:17:02.6: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2254796571282155904,2461265.8646,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2254796571282155904 20260813.3646 11.40CV 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 08 13.3646 2461265.8646 13.04 21:10:59.36 +58:41:14.6
97.48514 7.18140 galactic Cep Second-epoch detections are separated by 2.0" and 6.4 pix
The object was found in VSX 0" Gaia DR3 2191355609362845184
Type: ROT
# Max. Min./Amp. JD0 Period
14.170 G 14.200 G K
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:10:59.36 +58:41:14.6: 14.04 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:10:59.36 +58:41:14.6: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 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
Gaia DR3 2191355609362845184,2461265.8646,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2191355609362845184 20260813.3646 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.98 20:59:44.15 +59:18:39.0
96.98834 8.68000 galactic Cep Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:44.15 +59:18:39.0 (user input) | T | P | (position from user input) J-Ks=1.112+/-0.034 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:59:44.15 +59:18:39.0: 14.03 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:59:44.15 +59:18:39.0: 14.22 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.11 +/- 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
target,2461265.8646,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.98CV 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 08 13.3646 2461265.8646 13.01 21:18:50.77 +58:52:25.2
98.32615 6.56988 galactic Cep Second-epoch detections are separated by 0.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.7120+58.8736 | 21:18:50.77 +58:52:25.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.235+/-0.028 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:18:50.77 +58:52:25.2: 14.01 +/- 0.08 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:18:50.77 +58:52:25.2: 14.03 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.02 +/- 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
ATO J319.7120+58.8736,2461265.8646,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J319.7120+58.8736 20260813.3646 13.01CV 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 08 13.3646 2461265.8646 12.94 21:02:52.30 +59:13:23.5
97.18470 8.31879 galactic Cep Second-epoch detections are separated by 1.3" and 6.3 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 2190703736405074560 | 21:02:54.93 +59:13:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.311+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:02:52.30 +59:13:23.5: 14.01 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:02:52.30 +59:13:23.5: 13.82 +/- 0.06 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
Gaia DR3 2190703736405074560,2461265.8646,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2190703736405074560 20260813.3646 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.07 21:05:15.17 +59:10:38.8
97.35263 8.05922 galactic Cep Second-epoch detections are separated by 4.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J316.3128+59.1746 | 21:05:15.17 +59:10:38.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.464+/-0.040 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:05:15.17 +59:10:38.8: 13.97 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:05:15.17 +59:10:38.8: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 J316.3128+59.1746,2461265.8646,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.3128+59.1746 20260813.3646 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.07 21:00:06.21 +59:07:32.4
96.87637 8.52430 galactic Cep Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:06.21 +59:07:32.4 (user input) | T | P | (position from user input) J-Ks=0.997+/-0.032 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:00:06.21 +59:07:32.4: 13.97 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:00:06.21 +59:07:32.4: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.03 21:12:30.11 +58:37:41.5
97.57597 6.99684 galactic Cep Second-epoch detections are separated by 2.1" and 6.3 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 | 21:12:30.11 +58:37:41.5 (user input) | T | P | (position from user input) J-Ks=0.586+/-0.030 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:12:30.11 +58:37:41.5: 13.97 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:12:30.11 +58:37:41.5: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.01 +/- 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
target,2461265.8646,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.05 20:58:00.93 +60:26:12.3
97.72076 9.56956 galactic Cep Second-epoch detections are separated by 0.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:00.93 +60:26:12.3 (user input) | T | P | (position from user input) J-Ks=1.031+/-0.032 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:58:00.93 +60:26:12.3: 13.99 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:58:00.93 +60:26:12.3: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 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
target,2461265.8646,13.05,0.05,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
target 20260813.3646 13.05CV 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 08 13.3646 2461265.8646 13.01 21:18:12.04 +58:40:09.5
98.11990 6.48758 galactic Cep Second-epoch detections are separated by 1.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:18:12.04 +58:40:09.5 (user input) | T | P | (position from user input) J-Ks=0.900+/-0.031 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:18:12.04 +58:40:09.5: 13.97 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:18:12.04 +58:40:09.5: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,13.01,0.05,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
target 20260813.3646 13.01CV 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 08 13.3646 2461265.8646 12.91 21:31:36.45 +58:22:22.5
99.16486 5.04900 galactic Cep Second-epoch detections are separated by 2.4" and 6.2 pix
The object was found in VSX 0" ZTF J213136.45+582222.1
Type: SR
# Max. Min./Amp. JD0 Period
15.707 g Y 0.121 g 2458608.68060 28.933659900000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:31:36.45 +58:22:22.5: 13.98 +/- 0.09 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:31:36.45 +58:22:22.5: 14.29 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J213136.45+582222.1,2461265.8646,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213136.45+582222.1 20260813.3646 12.91CV 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 08 13.3646 2461265.8646 13.03 21:09:52.17 +58:33:06.6
97.28514 7.19724 galactic Cep Second-epoch detections are separated by 2.1" and 6.4 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 | 21:09:52.17 +58:33:06.6 (user input) | T | P | (position from user input) J-Ks=0.896+/-0.037 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:09:52.17 +58:33:06.6: 13.97 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:09:52.17 +58:33:06.6: 14.18 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.04 +/- 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
target,2461265.8646,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.03 20:58:04.91 +61:04:17.8
98.22125 9.96936 galactic Cep Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:04.91 +61:04:17.8 (user input) | T | P | (position from user input) J-Ks=1.505+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:58:04.91 +61:04:17.8: 13.94 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:58:04.91 +61:04:17.8: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.01 21:25:39.04 +59:41:25.9
99.52588 6.53023 galactic Cep Second-epoch detections are separated by 2.6" and 5.9 pix
The object was found in VSX 1" ZTF J212539.13+594126.6
Type: SR
# Max. Min./Amp. JD0 Period
13.271 r Y 0.271 r 2458338.91760 175.480803300000 C
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:25:39.04 +59:41:25.9: 13.95 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:25:39.04 +59:41:25.9: 14.16 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J212539.13+594126.6,2461265.8646,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J212539.13+594126.6 20260813.3646 13.01CV 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 08 13.3646 2461265.8646 12.99 21:08:14.66 +58:54:37.4
97.40993 7.59438 galactic Cep Second-epoch detections are separated by 1.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.0640+58.9122 | 21:08:14.66 +58:54:37.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.032+/-0.032 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:08:14.66 +58:54:37.4: 13.98 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:08:14.66 +58:54:37.4: 14.08 +/- 0.08 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
ATO J317.0640+58.9122,2461265.8646,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.0640+58.9122 20260813.3646 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.96 21:02:39.13 +59:06:38.5
97.08017 8.26637 galactic Cep Second-epoch detections are separated by 0.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:39.13 +59:06:38.5 (user input) | T | P | (position from user input) J-Ks=0.986+/-0.032 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:02:39.13 +59:06:38.5: 13.93 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:02:39.13 +59:06:38.5: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 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
target,2461265.8646,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.96 20:57:49.39 +60:14:52.2
97.55813 9.46695 galactic Cep Second-epoch detections are separated by 1.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:49.39 +60:14:52.2 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.056 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:57:49.39 +60:14:52.2: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:57:49.39 +60:14:52.2: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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
target,2461265.8646,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.96 21:09:45.37 +58:42:55.6
97.39692 7.31844 galactic Cep Second-epoch detections are separated by 0.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.4384+58.7158 | 21:09:45.37 +58:42:55.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.317+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:09:45.37 +58:42:55.6: 13.90 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:09:45.37 +58:42:55.6: 14.05 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.96 +/- 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
ATO J317.4384+58.7158,2461265.8646,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.4384+58.7158 20260813.3646 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 10.79 21:02:07.23 +59:42:45.1
97.49606 8.71087 galactic Cep Second-epoch detections are separated by 0.5" and 6.2 pix
The object was found in VSX 1" V1036 Cep
Type: SR
# Max. Min./Amp. JD0 Period
12.760 V 14.290 V 2457845.00000 396.000000000000 M8
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:02:07.23 +59:42:45.1: 11.70 +/- 0.01 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:02:07.23 +59:42:45.1: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1036 Cep,2461265.8646,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1036 Cep 20260813.3646 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.02 20:55:42.34 +60:07:57.2
97.29803 9.59638 galactic Cep Second-epoch detections are separated by 0.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9280+60.1366 | 20:55:42.34 +60:07:57.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.524+/-0.032 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:55:42.34 +60:07:57.2: 13.91 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:55:42.34 +60:07:57.2: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 J313.9280+60.1366,2461265.8646,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.9280+60.1366 20260813.3646 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.01 21:22:51.08 +59:05:32.6
98.84749 6.35611 galactic Cep Second-epoch detections are separated by 0.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:22:51.08 +59:05:32.6 (user input) | T | P | (position from user input) J-Ks=0.891+/-0.030 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:22:51.08 +59:05:32.6: 13.89 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:22:51.08 +59:05:32.6: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,13.01,0.05,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
target 20260813.3646 13.01CV 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 08 13.3646 2461265.8646 13.02 21:09:13.88 +58:54:23.1
97.49322 7.49724 galactic Cep Second-epoch detections are separated by 1.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:09:13.88 +58:54:23.1 (user input) | T | P | (position from user input) J-Ks=0.850+/-0.035 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:09:13.88 +58:54:23.1: 13.84 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:09:13.88 +58:54:23.1: 14.02 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 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
target,2461265.8646,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.96 20:59:27.33 +59:38:08.9
97.21612 8.91707 galactic Cep Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:27.33 +59:38:08.9 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.035 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:59:27.33 +59:38:08.9: 13.87 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:59:27.33 +59:38:08.9: 13.85 +/- 0.06 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
target,2461265.8646,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.94 21:02:59.83 +59:03:36.8
97.07098 8.19983 galactic Cep Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:02:59.83 +59:03:36.8 (user input) | T | P | (position from user input) J-Ks=0.951+/-0.033 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:02:59.83 +59:03:36.8: 13.87 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:02:59.83 +59:03:36.8: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 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
target,2461265.8646,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.95 21:26:27.24 +59:48:39.9
99.68353 6.54559 galactic Cep Second-epoch detections are separated by 2.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.6132+59.8113 | 21:26:27.24 +59:48:39.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.342+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:26:27.24 +59:48:39.9: 13.88 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:26:27.24 +59:48:39.9: 14.13 +/- 0.09 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
ATO J321.6132+59.8113,2461265.8646,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.6132+59.8113 20260813.3646 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.97 21:26:20.50 +59:48:22.6
99.66998 6.55202 galactic Cep Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.5855+59.8066 | 21:26:20.50 +59:48:22.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.285+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:26:20.50 +59:48:22.6: 13.85 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:26:20.50 +59:48:22.6: 13.92 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J321.5855+59.8066,2461265.8646,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.5855+59.8066 20260813.3646 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.86 21:11:15.42 +58:55:27.1
97.68441 7.31632 galactic Cep Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:11:15.42 +58:55:27.1 (user input) | T | P | (position from user input) J-Ks=1.139+/-0.036 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:11:15.42 +58:55:27.1: 13.83 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:11:15.42 +58:55:27.1: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 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
target,2461265.8646,12.86,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.78 20:58:51.00 +59:56:15.8
97.40025 9.16983 galactic Cep Second-epoch detections are separated by 1.0" and 6.2 pix
The object was found in VSX 1" Gaia DR3 2190984111868137600
Type: ROT
# Max. Min./Amp. JD0 Period
13.400 G 13.420 G K
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:58:51.00 +59:56:15.8: 13.83 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:58:51.00 +59:56:15.8: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 2190984111868137600,2461265.8646,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2190984111868137600 20260813.3646 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 13.14 21:02:11.57 +59:48:34.2
97.57643 8.76723 galactic Cep Second-epoch detections are separated by 2.0" and 6.0 pix
The object was found in VSX 2" NSVS J2102117+594840
Type: M
# Max. Min./Amp. JD0 Period
17.394 g Y 3.819 g 2458533.99490 376.909353200000 C
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:02:11.57 +59:48:34.2: 14.61 +/- 0.11 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:02:11.57 +59:48:34.2: 14.65 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2102117+594840,2461265.8646,13.14,0.05,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
NSVS J2102117+594840 20260813.3646 13.14CV 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 08 13.3646 2461265.8646 12.54 20:56:59.63 +60:45:20.4
97.88861 9.86967 galactic Cep Second-epoch detections are separated by 1.4" and 6.2 pix
The object was found in VSX 1" ZTF J205659.58+604520.9
Type: SR
# Max. Min./Amp. JD0 Period
12.859 r Y 0.441 r 2458274.51480 296.530143300000 C
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:56:59.63 +60:45:20.4: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:56:59.63 +60:45:20.4: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 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
ZTF J205659.58+604520.9,2461265.8646,12.54,0.05,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
ZTF J205659.58+604520.9 20260813.3646 12.54CV 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 08 13.3646 2461265.8646 12.94 21:02:33.12 +59:52:22.7
97.65488 8.77449 galactic Cep Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.6482+59.8816 | 21:02:33.12 +59:52:22.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.474+/-0.034 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:02:33.12 +59:52:22.7: 13.80 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:02:33.12 +59:52:22.7: 13.87 +/- 0.06 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
ATO J315.6482+59.8816,2461265.8646,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.6482+59.8816 20260813.3646 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.90 21:24:00.22 +59:43:41.2
99.40370 6.70290 galactic Cep Second-epoch detections are separated by 2.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J320.9848+59.7229 | 21:24:00.22 +59:43:41.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.477+/-0.028 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:24:00.22 +59:43:41.2: 13.79 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:24:00.22 +59:43:41.2: 13.85 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 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
ATO J320.9848+59.7229,2461265.8646,12.90,0.05,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
ATO J320.9848+59.7229 20260813.3646 12.90CV 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 08 13.3646 2461265.8646 12.79 21:10:09.15 +58:41:49.2
97.41819 7.26800 galactic Cep Second-epoch detections are separated by 1.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.5311+58.6989 | 21:10:09.15 +58:41:49.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.907+/-0.033 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:10:09.15 +58:41:49.2: 13.81 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:10:09.15 +58:41:49.2: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J317.5311+58.6989,2461265.8646,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.5311+58.6989 20260813.3646 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.70 19:37:34.84 +57:09:53.9
89.25309 16.65630 galactic Cyg Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J294.3991+57.1699 | 19:37:34.84 +57:09:53.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.398+/-0.033 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:37:34.84 +57:09:53.9: 13.80 +/- 0.07 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:37:34.84 +57:09:53.9: 13.84 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.82 +/- 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
ATO J294.3991+57.1699,2461265.8646,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.3991+57.1699 20260813.3646 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.96 20:58:08.10 +58:16:49.6
96.05727 8.17363 galactic Cep Second-epoch detections are separated by 0.7" and 6.4 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 | 20:58:08.10 +58:16:49.6 (user input) | T | P | (position from user input) J-Ks=0.615+/-0.032 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:58:08.10 +58:16:49.6: 13.76 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:58:08.10 +58:16:49.6: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461265.8646,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260813.3646 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.64 20:58:54.54 +60:02:20.0
97.48354 9.22925 galactic Cep Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.7271+60.0390 | 20:58:54.50 +60:02:20.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.611+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:58:54.54 +60:02:20.0: 13.77 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:58:54.54 +60:02:20.0: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 J314.7271+60.0390,2461265.8646,12.64,0.05,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 J314.7271+60.0390 20260813.3646 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 08 13.3646 2461265.8646 12.85 21:10:50.99 +58:43:26.6
97.49998 7.21956 galactic Cep Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.7058+58.7245 | 21:10:50.99 +58:43:26.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.807+/-0.035 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:10:50.99 +58:43:26.6: 13.71 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:10:50.99 +58:43:26.6: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J317.7058+58.7245,2461265.8646,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J317.7058+58.7245 20260813.3646 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.70 19:33:39.97 +59:15:24.4
91.04019 17.97179 galactic Dra Second-epoch detections are separated by 2.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J293.4157+59.2546 | 19:33:39.97 +59:15:24.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:33:39.97 +59:15:24.4: 13.73 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:33:39.97 +59:15:24.4: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J293.4157+59.2546,2461265.8646,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.4157+59.2546 20260813.3646 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 13.3646 2461265.8646 12.87 20:55:49.18 +59:47:24.2
97.03887 9.36798 galactic Cep Second-epoch detections are separated by 0.8" and 6.3 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 | 20:55:49.18 +59:47:24.2 (user input) | T | P | (position from user input) J-Ks=1.174+/-0.043 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:55:49.18 +59:47:24.2: 13.69 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:55:49.18 +59:47:24.2: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 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
target,2461265.8646,12.87,0.05,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
target 20260813.3646 12.87CV 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 08 13.3646 2461265.8646 12.51 19:25:43.80 +65:30:51.4
96.87355 21.09942 galactic Dra Second-epoch detections are separated by 3.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:25:43.80 +65:30:51.4 (user input) | T | P | (position from user input) J-Ks=0.687+/-0.029 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:25:43.80 +65:30:51.4: 13.45 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:25:43.80 +65:30:51.4: 13.39 +/- 0.04 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
target,2461265.8646,12.51,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.52 19:27:48.70 +66:07:31.6
97.56733 21.10251 galactic Dra Second-epoch detections are separated by 4.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:27:48.70 +66:07:31.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:27:48.70 +66:07:31.6: 13.76 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:27:48.70 +66:07:31.6: 13.62 +/- 0.05 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
target,2461265.8646,12.52,0.05,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
target 20260813.3646 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 08 13.3646 2461265.8646 12.71 21:07:57.31 +59:22:42.1
97.73592 7.93504 galactic Cep Second-epoch detections are separated by 1.5" and 5.8 pix
The object was found in VSX 1" ASASSN-V J210757.31+592242.9
Type: SR
# Max. Min./Amp. JD0 Period
14.940 g Y 0.510 g 2458244.92100 41.660000000000
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 21:07:57.31 +59:22:42.1: 13.68 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 21:07:57.31 +59:22:42.1: 13.69 +/- 0.06 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 J210757.31+592242.9,2461265.8646,12.71,0.05,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 J210757.31+592242.9 20260813.3646 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 08 13.3646 2461265.8646 12.86 20:39:20.73 +59:16:40.7
95.32859 10.70405 galactic Cep Second-epoch detections are separated by 0.8" and 6.4 pix
The object was found in VSX 1" ASASSN-V J203920.76+591642.1
Type: L
# Max. Min./Amp. JD0 Period
14.010 V 14.360 V
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 20:39:20.73 +59:16:40.7: 13.67 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 20:39:20.73 +59:16:40.7: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 J203920.76+591642.1,2461265.8646,12.86,0.05,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
ASASSN-V J203920.76+591642.1 20260813.3646 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461234.91091210 13.07.2026 09:51:32.805 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
First image: 2461234.91091210 13.07.2026 09:51:32.805 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
Last image: 2461265.86489644 13.08.2026 08:45:17.052 /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 19901
Objects passed selection criteria: 19826
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: 13899.8
Average stars matched: 13630.5 (98.0629 %)
Memory usage VmPeak: 245032 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 13 03:47:30 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: 2461234.91091210 13.07.2026 09:51:32.805 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
First image: 2461234.91091210 13.07.2026 09:51:32.805 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
Last image: 2461265.86489644 13.08.2026 08:45:17.052 /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 316
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.16
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: 45 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 127198
Objects passed selection criteria: 126814
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 92812.2
Average stars matched: 89536.2 (96.4703 %)
Memory usage VmPeak: 587748 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 13 03:49:05 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
SExtractor catalog cache: saved Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.cat to cache
SExtractor catalog cache: saved Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.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-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.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: 2461265.86424481
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-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits exists and is non-empty
Saving wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits to local_wcs_cache/
'wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits' -> 'local_wcs_cache/wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits'
wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits exists and is non-empty
Saving wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits to local_wcs_cache/
'wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits' -> 'local_wcs_cache/wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits'
wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits exists and is non-empty
Saving wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits to local_wcs_cache/
'wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits' -> 'local_wcs_cache/wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits'
wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits exists and is non-empty
Saving wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits to local_wcs_cache/
'wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits' -> 'local_wcs_cache/wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits (1st reference image)
verification OK: wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:22.565 +61:59:04.30 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits (1st new image)
verification OK: wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 20:34:38.253 +62:00:38.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:22.565 +61:59:04.30
Second-epoch image center 20:34:38.253 +62:00:38.74
Angular distance between the image centers 0.0404 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits (2nd new image)
verification OK: wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 20:34:41.055 +62:00:06.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:34:22.565 +61:59:04.30
Second-epoch image center 20:34:41.055 +62:00:06.53
Angular distance between the image centers 0.0401 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 20:34:38.253 +62:00:38.74
Second-epoch second image center 20:34:41.055 +62:00:06.53
Angular distance between the image centers 0.01049 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits &> /tmp/tmp.Kkp0N9OtqY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits &> /tmp/tmp.9aFCw1ZXz1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits &> /tmp/tmp.fSlLLi7XNS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits &> /tmp/tmp.FZ759DU77o
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.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-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits and wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits and wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat
Found non-empty wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits and wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat
The reference image (wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits) and catalog (wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat) found
'wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat' -> 'wcsmag.cat'
Read 22068 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.2509 to 328.1475 deg, Dec +55.8693 to +67.2520 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 289.2509 to 328.1475 deg, Dec 55.8693 to 67.2520 deg
Loaded 17165 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): 10557 out of 11305 total matches.
Matched with Tycho-2 11305 out of 22068 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.623800
a=0.000000 b=1.000000 c=22.623800
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 22068 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.2509 to 328.1475 deg, Dec +55.8693 to +67.2520 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 289.2509 to 328.1475 deg, Dec 55.8693 to 67.2520 deg
Loaded 17165 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): 10557 out of 11305 total matches.
Matched with Tycho-2 11305 out of 22068 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
Forced-photometry filter: calibrated wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits -> calib.txt_param_ref_wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits (aperture=6.4)
Read 20646 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.2096 to 328.1480 deg, Dec +55.8692 to +67.2833 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 289.2096 to 328.1480 deg, Dec 55.8692 to 67.2833 deg
Loaded 17206 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): 10535 out of 11246 total matches.
Matched with Tycho-2 11246 out of 20646 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
Forced-photometry filter: calibrated wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits -> calib.txt_param_ref_wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
2.3 pix Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
2.9 pix fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
2.9 pix fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
Limiting magnitude estimates:
15.2 mag. Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
15.1 mag. Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
13.4 mag. fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
13.2 mag. fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Kkp0N9OtqY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.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-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits' -> 'wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
WCS-calibrated image found: wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
Checking if the catalog wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits
WCS catalog name: wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1774, bad_region=0, passed=22068
Got 22068 stars (including 20263 good ones) from the SExtractor catalog wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat
util/solve_plate_with_UCAC5 got 22068 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 22068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 22068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 22068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4907 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits N_match=4907 sigma_overall_arcsec=0.544 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.644 sigma_q3_arcsec=0.523 sigma_q4_arcsec=0.652 n_q1=1234 n_q2=1085 n_q3=1142 n_q4=1446 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits -region wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9aFCw1ZXz1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.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-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits' -> 'wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
Checking if the catalog wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits
WCS catalog name: wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1675, bad_region=1, passed=20646
Got 20646 stars (including 18945 good ones) from the SExtractor catalog wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat
util/solve_plate_with_UCAC5 got 20646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 4905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 20646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 20646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 20646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4905 stars left (next iteration limit 5395)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits N_match=4905 sigma_overall_arcsec=0.516 sigma_q1_arcsec=0.415 sigma_q2_arcsec=0.602 sigma_q3_arcsec=0.530 sigma_q4_arcsec=0.585 n_q1=1222 n_q2=1105 n_q3=1127 n_q4=1451 worst_quadrant_to_overall_ratio=1.167
The image catalog is written to wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits -region wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fSlLLi7XNS (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_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.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_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
Checking if the catalog wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
WCS catalog name: wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=262, bad_region=0, passed=6944
Got 6944 stars (including 6679 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 6944 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 6944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 4907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 6944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 6944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4873 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4873 robust_rms=11.687 arcsec worst_quadrant_rms=15.150 arcsec
SIP_REFIT: SIP order 3 trial: matched=4873 robust_rms=0.416 arcsec worst_quadrant_rms=0.466 arcsec
SIP_REFIT: SIP order 5 trial: matched=4873 robust_rms=0.334 arcsec worst_quadrant_rms=0.417 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4873 robust_rms_before=0.674 arcsec robust_rms_before_corrected=0.354 arcsec robust_rms_after=0.334 arcsec worst_quadrant_rms_before=0.443 worst_quadrant_rms_after=0.417
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.443 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits N_match=4873 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.399 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.310 sigma_q4_arcsec=0.357 n_q1=885 n_q2=1112 n_q3=1805 n_q4=1071 worst_quadrant_to_overall_ratio=1.231
The image catalog is written to wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits -region wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FZ759DU77o (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_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.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_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
Checking if the catalog wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
WCS catalog name: wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=229, bad_region=0, passed=6302
Got 6302 stars (including 6068 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat
util/solve_plate_with_UCAC5 got 6302 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 4880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 6294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 6295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 6295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4884 stars left (next iteration limit 5372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4884 robust_rms=13.637 arcsec worst_quadrant_rms=15.014 arcsec
SIP_REFIT: SIP order 3 trial: matched=4884 robust_rms=0.417 arcsec worst_quadrant_rms=0.482 arcsec
SIP_REFIT: SIP order 5 trial: matched=4884 robust_rms=0.332 arcsec worst_quadrant_rms=0.465 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4884 robust_rms_before=0.683 arcsec robust_rms_before_corrected=0.338 arcsec robust_rms_after=0.417 arcsec worst_quadrant_rms_before=0.466 worst_quadrant_rms_after=0.482
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.466 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits N_match=4884 sigma_overall_arcsec=0.343 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.441 sigma_q3_arcsec=0.311 sigma_q4_arcsec=0.354 n_q1=1069 n_q2=666 n_q3=1535 n_q4=1614 worst_quadrant_to_overall_ratio=1.288
The image catalog is written to wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits -region wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits sigma_overall=0.544 worst_q_ratio=1.198
ref2=Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits sigma_overall=0.516 worst_q_ratio=1.167
new1=fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits sigma_overall=0.359 worst_q_ratio=1.231
new2=fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits sigma_overall=0.343 worst_q_ratio=1.288
reference average sigma_overall=0.53 worst_q_ratio=1.1825
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257_astrometric_residuals.png (4907 matched stars from wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256_astrometric_residuals.png (4905 matched stars from wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258_astrometric_residuals.png (4873 matched stars from wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259_astrometric_residuals.png (4884 matched stars from wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-44-20_20.00sec_-0.00C_LIGHTs_0258.fits'
Saving fully-calibrated image wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-13_CI_Cep-05-Q1b1x1_034602_TTUQ1b1x1_2037864_ttDFVe8y/wcs_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259.fits'
Preparing the HTML report for the field Cep-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-13_04-51-32_20.00sec_5.00C_LIGHT_0257.fits at 19:36:24.38 +65:10:26.4: 11.68 +/- 0.01 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-07-17_04-39-37_20.00sec_4.90C_LIGHT_0256.fits at 19:36:24.38 +65:10:26.4: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Forced photometry filter KEPT candidate at 19:36:24.38 +65:10:26.4: ref_mag=11.70 +/- 0.01 new_mean_mag=10.5873 delta=1.11 (need > 0.90)
Adding exclusion_list_local.txt__out02804.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30851_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 30851_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:19:14.40 +58:38:37.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 30923_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 30923_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:27:11.59 +59:45:18.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30935_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 30935_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:29:30.50 +57:59:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30206_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 30206_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:42:30.47 +59:15:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02804_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 02804_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15393_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 15393_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:21:57.18 +62:22:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163900_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 163900_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 163919_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 163919_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 163921_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 163921_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:07:01.52 +58:38:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163931_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 163931_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:01:40.26 +57:45:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163933_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 163933_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 163935_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 163935_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:29:34.34 +57:59:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163939_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 163939_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 163941_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 163941_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:36:31.81 +59:01:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164068_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164068_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:27:11.61 +59:45:18.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 164097_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164097_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 164131_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164131_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:13:16.29 +58:29:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164143_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164143_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:23:30.59 +59:51:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164267_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164267_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:01:48.79 +57:05:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164428_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164428_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:06:38.84 +58:27:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164549_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164549_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:20:13.61 +56:31:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164576_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164576_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:50:06.51 +56:48:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164589_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164589_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:11:47.30 +58:28:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164595_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164595_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 164601_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164601_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:01:54.84 +57:06:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164610_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164610_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 164661_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164661_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 164668_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164668_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164747_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164747_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164773_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164773_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:30:31.30 +58:19:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164807_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164807_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:11:18.90 +57:38:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164817_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164817_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164830_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164830_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164839_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164839_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:25:52.82 +60:07:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164867_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164867_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:10:23.50 +58:55:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164910_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164910_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164929_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164929_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164945_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164945_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164961_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164961_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:52:59.76 +62:10:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164962_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164962_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164985_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164985_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:42:24.70 +57:23:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164994_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 164994_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:59:20.31 +59:28:03.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165113_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 165113_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:25:08.86 +59:37:31.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165125_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 165125_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165131_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 165131_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:37:54.30 +62:03:02.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165242_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 165242_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165321_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 165321_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165328_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 165328_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165341_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 165341_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:01:22.61 +58:35:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165501_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 165501_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:24:11.83 +59:27:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80789_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 80789_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73093_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 73093_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133210_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 133210_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:24:04.43 +58:50:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88002_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 88002_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87752_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 87752_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 89690_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 89690_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83910_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 83910_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136723_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 136723_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85613_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 85613_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 131943_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 131943_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 87396_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 87396_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81835_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 81835_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91740_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 91740_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127548_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 127548_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101832_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 101832_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 77697_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 77697_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 130862_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 130862_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:24:01.27 +58:39:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131181_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 131181_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 132730_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 132730_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 89492_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 89492_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:28:48.36 +59:32:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99565_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 99565_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 84574_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 84574_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 138578_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 138578_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 09808_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 09808_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 129769_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 129769_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 138519_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 138519_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 01854_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01854_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 94844_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 94844_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:37:29.41 +57:05:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06851_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 06851_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 131305_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 131305_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:20:51.28 +58:44:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98797_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 98797_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:31:00.85 +58:07:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98010_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 98010_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 130534_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 130534_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 99448_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 99448_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 89349_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 89349_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 59891_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 59891_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 130841_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 130841_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 135041_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 135041_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 129767_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 129767_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 10257_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 10257_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 131090_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 131090_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 87629_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 87629_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 92939_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 92939_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:37:46.42 +56:56:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137029_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 137029_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:26:36.56 +59:08:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01668_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01668_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 127344_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 127344_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 125313_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 125313_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 97430_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 97430_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 132513_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 132513_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 139083_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 139083_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 20112_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 20112_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05883_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05883_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 04856_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 04856_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 04439_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 04439_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 77449_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 77449_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03395_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03395_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 130215_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 130215_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 131456_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 131456_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 04259_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 04259_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03493_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03493_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 01592_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01592_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 02295_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 02295_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05826_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05826_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05868_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05868_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 134680_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 134680_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 128952_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 128952_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 19823_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 19823_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 01654_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01654_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 133153_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 133153_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 09202_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 09202_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 08270_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 08270_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 135024_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 135024_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:34:19.78 +58:59:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88972_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 88972_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 02972_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 02972_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 136162_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 136162_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:31:07.48 +58:55:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86735_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 86735_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 129059_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 129059_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 01832_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01832_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 90456_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 90456_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 137847_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 137847_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 06466_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 06466_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 01548_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01548_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 88663_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 88663_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03356_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03356_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 08881_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 08881_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 126395_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 126395_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03646_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03646_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05992_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05992_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 06950_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 06950_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 95979_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 95979_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:36:27.54 +57:27:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05469_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05469_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 02705_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 02705_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03580_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03580_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 129075_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 129075_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:36:14.30 +58:31:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80340_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 80340_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03605_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 03605_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 02938_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 02938_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 08191_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 08191_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 136523_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 136523_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:28:13.82 +59:04:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05030_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05030_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 01773_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01773_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 15960_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 15960_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 07809_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 07809_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03246_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03246_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 04659_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 04659_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 01711_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 01711_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 01774_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01774_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 82371_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 82371_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 126198_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 126198_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:44:18.62 +58:55:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86430_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 86430_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05406_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05406_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 100474_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 100474_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 02194_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 02194_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05031_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05031_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05164_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05164_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 06103_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 06103_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03334_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03334_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 06149_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 06149_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 81685_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 81685_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03596_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 03596_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 134503_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 134503_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03333_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03333_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 125495_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 125495_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:29:30.42 +57:59:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130308_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 130308_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:42:30.48 +59:15:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131696_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 131696_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 84926_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 84926_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 02021_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 02021_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 132047_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 132047_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 129672_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 129672_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 91038_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 91038_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 08570_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 08570_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 126853_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 126853_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 97791_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 97791_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:18:08.62 +58:10:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03368_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03368_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05598_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 05598_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 136511_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 136511_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 134693_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 134693_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 137119_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 137119_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:02:12.85 +59:41:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03884_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03884_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 129367_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 129367_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 05453_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 05453_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 97572_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 97572_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 99154_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 99154_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 03710_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03710_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 04244_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 04244_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 88405_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 88405_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 89142_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 89142_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 98791_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 98791_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 87059_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 87059_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 01626_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01626_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 04517_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 04517_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 128259_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 128259_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 01785_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01785_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 07044_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 07044_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 01487_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 01487_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 04582_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 04582_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 127939_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 127939_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 132984_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 132984_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 132077_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 132077_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 132439_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 132439_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 132346_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 132346_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 98210_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 98210_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 131029_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 131029_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 127714_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 127714_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 85897_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 85897_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 129547_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 129547_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 129298_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 129298_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 126154_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 126154_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 76329_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 76329_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 88760_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 88760_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 129655_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 129655_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 132758_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 132758_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:39:05.47 +59:32:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130881_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 130881_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 128067_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 128067_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:30:46.20 +58:12:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88792_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 88792_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 128308_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 128308_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 02808_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 02808_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:26:59.92 +66:08:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 2.817 2254771110718545152 291.74906563709 +66.13575618263 12.9592 12.3932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137245_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 137245_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 90882_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 90882_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 135570_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 135570_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 130151_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 130151_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 136249_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 136249_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 130591_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 130591_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 86832_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 86832_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 86798_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 86798_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 92811_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 92811_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:37:46.84 +56:55:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130801_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 130801_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 139139_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 139139_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 138247_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 138247_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 81418_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 81418_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 139000_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 139000_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 100741_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 100741_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 19:36:28.66 +58:53:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88841_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 88841_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 127861_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 127861_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 99077_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 99077_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:30:28.67 +58:14:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95126_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 95126_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 126865_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 126865_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 21:17:46.44 +58:26:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120875_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 120875_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 91604_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 91604_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 90578_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 90578_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
**** FOUND 20:59:44.03 +60:05:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.734 2190986895006095744 314.93137912136 +60.09286262878 13.5429 12.2195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99272_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 99272_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 128489_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 128489_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 102568_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 102568_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 137307_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 137307_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 08312_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 08312_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 10819_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
The candidate 10819_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259 did not pass the final checks
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Considering the candidate 03130_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 03130_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 134845_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 134845_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
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Considering the candidate 130194_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
Preparing report for the candidate 130194_fd_Cep-05-Q1b1x1_2026-08-13_03-45-17_20.00sec_-0.00C_LIGHTs_0259
make_report_in_HTML.sh Phase 2 (HTML assembly): 12s
make_report_in_HTML.sh TOTAL: 358s
Prepared the HTML report for the field Cep-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:36:24.38 +65:10:26.4
19:27:12.09 +66:17:02.6
19:37:48.01 +66:31:57.0
19:30:48.17 +66:22:02.2
19:30:53.45 +66:21:35.8
19:30:40.53 +66:21:20.5
20:00:13.62 +66:53:49.9
19:37:29.60 +66:29:52.9
19:38:12.45 +66:31:00.6
19:23:26.61 +66:08:26.9
19:28:39.36 +66:16:56.7
19:43:58.65 +66:37:08.8
19:49:42.01 +66:41:57.4
19:37:34.18 +66:27:06.3
19:47:44.01 +66:38:34.4
19:28:25.73 +66:09:11.5
19:35:57.50 +66:20:20.7
19:27:48.70 +66:07:31.6
19:43:54.83 +66:28:24.4
19:38:37.88 +66:21:08.3
19:31:50.63 +66:12:14.3
19:37:37.78 +66:19:57.0
19:31:05.29 +66:10:19.2
19:27:30.14 +66:05:06.0
19:40:01.58 +66:22:20.4
19:42:45.67 +66:24:52.4
19:26:16.35 +66:01:21.1
19:23:32.20 +65:56:25.4
19:23:54.10 +65:56:11.8
19:30:22.58 +66:03:40.6
19:29:26.70 +66:02:10.2
19:29:30.80 +66:01:24.3
19:30:16.62 +66:01:35.2
19:30:42.54 +66:01:17.3
19:27:50.79 +65:55:45.9
19:27:21.85 +65:54:08.4
19:31:54.56 +66:01:02.8
19:30:03.39 +65:57:08.9
19:29:28.25 +65:54:31.4
19:31:04.00 +65:56:51.5
19:32:31.11 +65:59:09.8
19:31:14.74 +65:55:03.9
19:24:50.71 +65:44:49.2
19:31:27.58 +65:54:59.2
19:33:17.80 +65:57:04.3
19:36:56.71 +66:01:07.1
19:24:21.96 +65:41:39.7
19:38:22.71 +66:00:48.3
19:38:26.91 +65:58:47.8
19:23:56.39 +65:30:47.2
19:38:27.19 +65:50:28.9
19:27:20.84 +65:33:47.2
19:25:43.80 +65:30:51.4
19:26:19.93 +65:28:02.2
19:26:01.40 +65:26:32.5
21:01:31.78 +59:14:23.1
21:01:46.36 +59:34:54.4
19:33:39.97 +59:15:24.4
19:24:13.08 +65:17:39.4
20:58:08.10 +58:16:49.6
21:08:53.44 +58:28:55.7
21:09:52.17 +58:33:06.6
20:42:02.70 +58:55:19.5
20:49:05.61 +58:53:57.4
21:09:25.31 +58:40:42.5
21:12:30.11 +58:37:41.5
21:10:09.15 +58:41:49.2
21:10:59.36 +58:41:14.6
21:01:00.08 +58:53:02.6
21:09:45.37 +58:42:55.6
21:10:50.99 +58:43:26.6
20:44:14.93 +59:07:57.8
21:10:18.73 +58:47:48.7
21:31:36.45 +58:22:22.5
21:03:26.39 +58:57:08.5
21:18:12.04 +58:40:09.5
21:08:14.66 +58:54:37.4
21:10:02.27 +58:50:47.2
21:11:21.74 +58:49:49.2
21:09:13.88 +58:54:23.1
20:39:20.73 +59:16:40.7
21:09:32.55 +58:54:52.0
21:10:39.35 +58:55:53.9
21:02:59.83 +59:03:36.8
21:11:15.42 +58:55:27.1
21:14:23.70 +58:51:51.9
21:02:39.13 +59:06:38.5
21:00:06.21 +59:07:32.4
20:59:57.54 +59:09:21.8
21:00:17.49 +59:12:01.0
20:59:55.88 +59:11:31.6
21:11:52.50 +59:01:04.1
21:03:27.39 +59:10:26.3
21:10:26.67 +59:03:25.0
21:18:50.77 +58:52:25.2
21:05:15.17 +59:10:38.8
21:02:52.30 +59:13:23.5
21:11:45.27 +59:06:01.3
21:01:23.16 +59:16:47.5
20:59:44.15 +59:18:39.0
21:03:05.67 +59:17:33.8
20:57:41.34 +59:29:45.2
21:23:40.72 +58:59:22.6
21:01:53.55 +59:23:58.7
21:07:57.31 +59:22:42.1
20:59:34.78 +59:31:00.7
21:22:51.08 +59:05:32.6
20:59:27.33 +59:38:08.9
21:20:51.12 +59:14:08.1
21:24:27.49 +59:09:56.6
21:02:07.23 +59:42:45.1
20:55:49.18 +59:47:24.2
21:23:00.95 +59:19:20.8
21:02:11.57 +59:48:34.2
21:24:37.01 +59:20:33.2
21:02:33.12 +59:52:22.7
20:59:11.34 +59:56:10.5
20:58:51.00 +59:56:15.8
19:38:40.00 +65:07:39.1
19:39:10.71 +64:46:34.5
21:24:08.16 +61:40:56.4
20:57:02.38 +61:18:01.7
20:58:04.91 +61:04:17.8
20:57:55.84 +60:59:51.1
20:56:25.11 +61:00:21.8
20:57:36.85 +60:49:12.7
20:56:50.52 +60:47:43.6
20:56:59.63 +60:45:20.4
20:58:39.33 +60:42:44.9
20:55:44.69 +60:44:23.8
20:58:02.21 +60:39:58.5
20:59:44.23 +60:32:31.4
20:56:22.53 +60:33:25.7
20:55:55.86 +60:31:40.0
20:55:59.56 +60:28:49.1
20:58:00.93 +60:26:12.3
21:25:07.48 +59:52:30.9
20:56:00.54 +60:25:05.7
21:26:20.50 +59:48:22.6
21:26:27.24 +59:48:39.9
21:25:05.78 +59:49:01.9
21:30:03.89 +59:39:40.9
21:30:27.51 +59:37:56.0
21:23:15.30 +59:49:21.6
21:23:22.05 +59:48:19.9
20:57:18.13 +60:16:59.1
20:56:58.40 +60:16:13.3
21:25:39.04 +59:41:25.9
20:57:49.39 +60:14:52.2
21:24:00.22 +59:43:41.2
20:56:38.83 +60:14:56.7
21:24:39.32 +59:43:01.8
21:25:59.43 +59:39:01.8
21:25:57.61 +59:36:56.1
21:23:36.40 +59:37:50.8
20:55:42.34 +60:07:57.2
21:22:53.63 +59:37:09.5
20:58:54.54 +60:02:20.0
21:26:17.42 +59:27:42.6
19:37:34.84 +57:09:53.9
21:13:29.33 +58:09:45.0
21:00:31.82 +58:27:53.3
21:00:50.07 +58:35:50.2
21:09:09.15 +58:40:25.0
21:09:59.60 +58:45:20.1
21:09:22.48 +58:51:24.7
21:01:45.02 +59:00:58.6
########### Completed Cep-05-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 ####
19:36:24.38 +65:10:26.4
20:56:50.52 +60:47:43.6
20:57:02.38 +61:18:01.7
21:23:22.05 +59:48:19.9
21:23:15.30 +59:49:21.6
21:25:57.61 +59:36:56.1
20:59:44.23 +60:32:31.4
21:24:27.49 +59:09:56.6
20:55:59.56 +60:28:49.1
21:03:27.39 +59:10:26.3
21:30:03.89 +59:39:40.9
20:55:44.69 +60:44:23.8
21:26:17.42 +59:27:42.6
21:09:25.31 +58:40:42.5
21:01:46.36 +59:34:54.4
20:56:25.11 +61:00:21.8
21:00:17.49 +59:12:01.0
21:01:23.16 +59:16:47.5
21:01:45.02 +59:00:58.6
20:56:22.53 +60:33:25.7
21:11:21.74 +58:49:49.2
21:24:37.01 +59:20:33.2
19:43:58.65 +66:37:08.8
19:38:26.91 +65:58:47.8
21:00:50.07 +58:35:50.2
21:10:39.35 +58:55:53.9
21:09:22.48 +58:51:24.7
21:25:59.43 +59:39:01.8
21:24:08.16 +61:40:56.4
21:14:23.70 +58:51:51.9
20:59:34.78 +59:31:00.7
19:24:13.08 +65:17:39.4
20:59:57.54 +59:09:21.8
21:30:27.51 +59:37:56.0
20:00:13.62 +66:53:49.9
21:08:53.44 +58:28:55.7
21:13:29.33 +58:09:45.0
21:11:45.27 +59:06:01.3
20:59:11.34 +59:56:10.5
19:39:10.71 +64:46:34.5
19:31:27.58 +65:54:59.2
19:27:50.79 +65:55:45.9
19:29:30.80 +66:01:24.3
20:57:55.84 +60:59:51.1
19:27:30.14 +66:05:06.0
21:09:32.55 +58:54:52.0
20:59:55.88 +59:11:31.6
19:29:26.70 +66:02:10.2
19:40:01.58 +66:22:20.4
19:30:48.17 +66:22:02.2
19:47:44.01 +66:38:34.4
19:31:14.74 +65:55:03.9
19:24:50.71 +65:44:49.2
21:23:40.72 +58:59:22.6
20:44:14.93 +59:07:57.8
19:30:40.53 +66:21:20.5
21:03:05.67 +59:17:33.8
19:26:01.40 +65:26:32.5
19:27:20.84 +65:33:47.2
20:56:38.83 +60:14:56.7
19:35:57.50 +66:20:20.7
20:56:00.54 +60:25:05.7
21:10:18.73 +58:47:48.7
19:28:39.36 +66:16:56.7
21:23:36.40 +59:37:50.8
21:23:00.95 +59:19:20.8
19:38:22.71 +66:00:48.3
19:37:48.01 +66:31:57.0
20:56:58.40 +60:16:13.3
19:37:37.78 +66:19:57.0
19:26:19.93 +65:28:02.2
20:42:02.70 +58:55:19.5
19:26:16.35 +66:01:21.1
19:33:17.80 +65:57:04.3
19:32:31.11 +65:59:09.8
19:28:25.73 +66:09:11.5
19:42:45.67 +66:24:52.4
20:57:36.85 +60:49:12.7
19:38:27.19 +65:50:28.9
19:27:21.85 +65:54:08.4
19:37:29.60 +66:29:52.9
19:38:40.00 +65:07:39.1
19:23:56.39 +65:30:47.2
19:43:54.83 +66:28:24.4
19:30:42.54 +66:01:17.3
19:38:12.45 +66:31:00.6
20:58:02.21 +60:39:58.5
21:25:07.48 +59:52:30.9
19:29:28.25 +65:54:31.4
21:01:31.78 +59:14:23.1
19:37:34.18 +66:27:06.3
19:31:54.56 +66:01:02.8
19:30:03.39 +65:57:08.9
19:36:56.71 +66:01:07.1
19:31:50.63 +66:12:14.3
19:24:21.96 +65:41:39.7
20:58:39.33 +60:42:44.9
20:57:41.34 +59:29:45.2
19:38:37.88 +66:21:08.3
21:11:52.50 +59:01:04.1
20:55:55.86 +60:31:40.0
19:49:42.01 +66:41:57.4
21:10:26.67 +59:03:25.0
21:10:02.27 +58:50:47.2
21:22:53.63 +59:37:09.5
20:49:05.61 +58:53:57.4
19:31:05.29 +66:10:19.2
21:20:51.12 +59:14:08.1
21:01:53.55 +59:23:58.7
19:23:54.10 +65:56:11.8
21:03:26.39 +58:57:08.5
19:31:04.00 +65:56:51.5
21:00:31.82 +58:27:53.3
21:09:59.60 +58:45:20.1
19:23:32.20 +65:56:25.4
19:30:22.58 +66:03:40.6
20:57:18.13 +60:16:59.1
21:24:39.32 +59:43:01.8
21:09:09.15 +58:40:25.0
21:25:05.78 +59:49:01.9
19:30:53.45 +66:21:35.8
19:30:16.62 +66:01:35.2
21:01:00.08 +58:53:02.6
19:23:26.61 +66:08:26.9
19:27:12.09 +66:17:02.6
21:10:59.36 +58:41:14.6
20:59:44.15 +59:18:39.0
21:18:50.77 +58:52:25.2
21:02:52.30 +59:13:23.5
21:05:15.17 +59:10:38.8
21:00:06.21 +59:07:32.4
21:12:30.11 +58:37:41.5
20:58:00.93 +60:26:12.3
21:18:12.04 +58:40:09.5
21:31:36.45 +58:22:22.5
21:09:52.17 +58:33:06.6
20:58:04.91 +61:04:17.8
21:25:39.04 +59:41:25.9
21:08:14.66 +58:54:37.4
21:02:39.13 +59:06:38.5
20:57:49.39 +60:14:52.2
21:09:45.37 +58:42:55.6
21:02:07.23 +59:42:45.1
20:55:42.34 +60:07:57.2
21:22:51.08 +59:05:32.6
21:09:13.88 +58:54:23.1
20:59:27.33 +59:38:08.9
21:02:59.83 +59:03:36.8
21:26:27.24 +59:48:39.9
21:26:20.50 +59:48:22.6
21:11:15.42 +58:55:27.1
20:58:51.00 +59:56:15.8
21:02:11.57 +59:48:34.2
20:56:59.63 +60:45:20.4
21:02:33.12 +59:52:22.7
21:24:00.22 +59:43:41.2
21:10:09.15 +58:41:49.2
19:37:34.84 +57:09:53.9
20:58:08.10 +58:16:49.6
20:58:54.54 +60:02:20.0
21:10:50.99 +58:43:26.6
19:33:39.97 +59:15:24.4
20:55:49.18 +59:47:24.2
19:25:43.80 +65:30:51.4
19:27:48.70 +66:07:31.6
21:07:57.31 +59:22:42.1
20:39:20.73 +59:16:40.7
###################################################################################
19:36:24.38 +65:10:26.4 -- not an asteroid (will add it to exclusion list)
20:56:50.52 +60:47:43.6 -- not an asteroid (will add it to exclusion list)
20:57:02.38 +61:18:01.7 -- not an asteroid (will add it to exclusion list)
21:23:22.05 +59:48:19.9 -- not an asteroid (will add it to exclusion list)
21:23:15.30 +59:49:21.6 -- not an asteroid (will add it to exclusion list)
21:25:57.61 +59:36:56.1 -- not an asteroid (will add it to exclusion list)
20:59:44.23 +60:32:31.4 -- not an asteroid (will add it to exclusion list)
21:24:27.49 +59:09:56.6 -- not an asteroid (will add it to exclusion list)
20:55:59.56 +60:28:49.1 -- not an asteroid (will add it to exclusion list)
21:03:27.39 +59:10:26.3 -- not an asteroid (will add it to exclusion list)
21:30:03.89 +59:39:40.9 -- not an asteroid (will add it to exclusion list)
20:55:44.69 +60:44:23.8 -- not an asteroid (will add it to exclusion list)
21:26:17.42 +59:27:42.6 -- not an asteroid (will add it to exclusion list)
21:09:25.31 +58:40:42.5 -- not an asteroid (will add it to exclusion list)
21:01:46.36 +59:34:54.4 -- not an asteroid (will add it to exclusion list)
20:56:25.11 +61:00:21.8 -- not an asteroid (will add it to exclusion list)
21:00:17.49 +59:12:01.0 -- not an asteroid (will add it to exclusion list)
21:01:23.16 +59:16:47.5 -- not an asteroid (will add it to exclusion list)
21:01:45.02 +59:00:58.6 -- not an asteroid (will add it to exclusion list)
20:56:22.53 +60:33:25.7 -- not an asteroid (will add it to exclusion list)
21:11:21.74 +58:49:49.2 -- not an asteroid (will add it to exclusion list)
21:24:37.01 +59:20:33.2 -- not an asteroid (will add it to exclusion list)
19:43:58.65 +66:37:08.8 -- not an asteroid (will add it to exclusion list)
19:38:26.91 +65:58:47.8 -- not an asteroid (will add it to exclusion list)
21:00:50.07 +58:35:50.2 -- not an asteroid (will add it to exclusion list)
21:10:39.35 +58:55:53.9 -- not an asteroid (will add it to exclusion list)
21:09:22.48 +58:51:24.7 -- not an asteroid (will add it to exclusion list)
21:25:59.43 +59:39:01.8 -- not an asteroid (will add it to exclusion list)
21:24:08.16 +61:40:56.4 -- not an asteroid (will add it to exclusion list)
21:14:23.70 +58:51:51.9 -- not an asteroid (will add it to exclusion list)
20:59:34.78 +59:31:00.7 -- not an asteroid (will add it to exclusion list)
19:24:13.08 +65:17:39.4 -- not an asteroid (will add it to exclusion list)
20:59:57.54 +59:09:21.8 -- not an asteroid (will add it to exclusion list)
21:30:27.51 +59:37:56.0 -- not an asteroid (will add it to exclusion list)
20:00:13.62 +66:53:49.9 -- not an asteroid (will add it to exclusion list)
21:08:53.44 +58:28:55.7 -- not an asteroid (will add it to exclusion list)
21:13:29.33 +58:09:45.0 -- not an asteroid (will add it to exclusion list)
21:11:45.27 +59:06:01.3 -- not an asteroid (will add it to exclusion list)
20:59:11.34 +59:56:10.5 -- not an asteroid (will add it to exclusion list)
19:39:10.71 +64:46:34.5 -- not an asteroid (will add it to exclusion list)
19:31:27.58 +65:54:59.2 -- not an asteroid (will add it to exclusion list)
19:27:50.79 +65:55:45.9 -- not an asteroid (will add it to exclusion list)
19:29:30.80 +66:01:24.3 -- not an asteroid (will add it to exclusion list)
20:57:55.84 +60:59:51.1 -- not an asteroid (will add it to exclusion list)
19:27:30.14 +66:05:06.0 -- not an asteroid (will add it to exclusion list)
21:09:32.55 +58:54:52.0 -- not an asteroid (will add it to exclusion list)
20:59:55.88 +59:11:31.6 -- not an asteroid (will add it to exclusion list)
19:29:26.70 +66:02:10.2 -- not an asteroid (will add it to exclusion list)
19:40:01.58 +66:22:20.4 -- not an asteroid (will add it to exclusion list)
19:30:48.17 +66:22:02.2 -- not an asteroid (will add it to exclusion list)
19:47:44.01 +66:38:34.4 -- not an asteroid (will add it to exclusion list)
19:31:14.74 +65:55:03.9 -- not an asteroid (will add it to exclusion list)
19:24:50.71 +65:44:49.2 -- not an asteroid (will add it to exclusion list)
21:23:40.72 +58:59:22.6 -- not an asteroid (will add it to exclusion list)
20:44:14.93 +59:07:57.8 -- not an asteroid (will add it to exclusion list)
19:30:40.53 +66:21:20.5 -- not an asteroid (will add it to exclusion list)
21:03:05.67 +59:17:33.8 -- not an asteroid (will add it to exclusion list)
19:26:01.40 +65:26:32.5 -- not an asteroid (will add it to exclusion list)
19:27:20.84 +65:33:47.2 -- not an asteroid (will add it to exclusion list)
20:56:38.83 +60:14:56.7 -- not an asteroid (will add it to exclusion list)
19:35:57.50 +66:20:20.7 -- not an asteroid (will add it to exclusion list)
20:56:00.54 +60:25:05.7 -- not an asteroid (will add it to exclusion list)
21:10:18.73 +58:47:48.7 -- not an asteroid (will add it to exclusion list)
19:28:39.36 +66:16:56.7 -- not an asteroid (will add it to exclusion list)
21:23:36.40 +59:37:50.8 -- not an asteroid (will add it to exclusion list)
21:23:00.95 +59:19:20.8 -- not an asteroid (will add it to exclusion list)
19:38:22.71 +66:00:48.3 -- not an asteroid (will add it to exclusion list)
19:37:48.01 +66:31:57.0 -- not an asteroid (will add it to exclusion list)
20:56:58.40 +60:16:13.3 -- not an asteroid (will add it to exclusion list)
19:37:37.78 +66:19:57.0 -- not an asteroid (will add it to exclusion list)
19:26:19.93 +65:28:02.2 -- not an asteroid (will add it to exclusion list)
20:42:02.70 +58:55:19.5 -- not an asteroid (will add it to exclusion list)
19:26:16.35 +66:01:21.1 -- not an asteroid (will add it to exclusion list)
19:33:17.80 +65:57:04.3 -- not an asteroid (will add it to exclusion list)
19:32:31.11 +65:59:09.8 -- not an asteroid (will add it to exclusion list)
19:28:25.73 +66:09:11.5 -- not an asteroid (will add it to exclusion list)
19:42:45.67 +66:24:52.4 -- not an asteroid (will add it to exclusion list)
20:57:36.85 +60:49:12.7 -- not an asteroid (will add it to exclusion list)
19:38:27.19 +65:50:28.9 -- not an asteroid (will add it to exclusion list)
19:27:21.85 +65:54:08.4 -- not an asteroid (will add it to exclusion list)
19:37:29.60 +66:29:52.9 -- not an asteroid (will add it to exclusion list)
19:38:40.00 +65:07:39.1 -- not an asteroid (will add it to exclusion list)
19:23:56.39 +65:30:47.2 -- not an asteroid (will add it to exclusion list)
19:43:54.83 +66:28:24.4 -- not an asteroid (will add it to exclusion list)
19:30:42.54 +66:01:17.3 -- not an asteroid (will add it to exclusion list)
19:38:12.45 +66:31:00.6 -- not an asteroid (will add it to exclusion list)
20:58:02.21 +60:39:58.5 -- not an asteroid (will add it to exclusion list)
21:25:07.48 +59:52:30.9 -- not an asteroid (will add it to exclusion list)
19:29:28.25 +65:54:31.4 -- not an asteroid (will add it to exclusion list)
21:01:31.78 +59:14:23.1 -- not an asteroid (will add it to exclusion list)
19:37:34.18 +66:27:06.3 -- not an asteroid (will add it to exclusion list)
19:31:54.56 +66:01:02.8 -- not an asteroid (will add it to exclusion list)
19:30:03.39 +65:57:08.9 -- not an asteroid (will add it to exclusion list)
19:36:56.71 +66:01:07.1 -- not an asteroid (will add it to exclusion list)
19:31:50.63 +66:12:14.3 -- not an asteroid (will add it to exclusion list)
19:24:21.96 +65:41:39.7 -- not an asteroid (will add it to exclusion list)
20:58:39.33 +60:42:44.9 -- not an asteroid (will add it to exclusion list)
20:57:41.34 +59:29:45.2 -- not an asteroid (will add it to exclusion list)
19:38:37.88 +66:21:08.3 -- not an asteroid (will add it to exclusion list)
21:11:52.50 +59:01:04.1 -- not an asteroid (will add it to exclusion list)
20:55:55.86 +60:31:40.0 -- not an asteroid (will add it to exclusion list)
19:49:42.01 +66:41:57.4 -- not an asteroid (will add it to exclusion list)
21:10:26.67 +59:03:25.0 -- not an asteroid (will add it to exclusion list)
21:10:02.27 +58:50:47.2 -- not an asteroid (will add it to exclusion list)
21:22:53.63 +59:37:09.5 -- not an asteroid (will add it to exclusion list)
20:49:05.61 +58:53:57.4 -- not an asteroid (will add it to exclusion list)
19:31:05.29 +66:10:19.2 -- not an asteroid (will add it to exclusion list)
21:20:51.12 +59:14:08.1 -- not an asteroid (will add it to exclusion list)
21:01:53.55 +59:23:58.7 -- not an asteroid (will add it to exclusion list)
19:23:54.10 +65:56:11.8 -- not an asteroid (will add it to exclusion list)
21:03:26.39 +58:57:08.5 -- not an asteroid (will add it to exclusion list)
19:31:04.00 +65:56:51.5 -- not an asteroid (will add it to exclusion list)
21:00:31.82 +58:27:53.3 -- not an asteroid (will add it to exclusion list)
21:09:59.60 +58:45:20.1 -- not an asteroid (will add it to exclusion list)
19:23:32.20 +65:56:25.4 -- not an asteroid (will add it to exclusion list)
19:30:22.58 +66:03:40.6 -- not an asteroid (will add it to exclusion list)
20:57:18.13 +60:16:59.1 -- not an asteroid (will add it to exclusion list)
21:24:39.32 +59:43:01.8 -- not an asteroid (will add it to exclusion list)
21:09:09.15 +58:40:25.0 -- not an asteroid (will add it to exclusion list)
21:25:05.78 +59:49:01.9 -- not an asteroid (will add it to exclusion list)
19:30:53.45 +66:21:35.8 -- not an asteroid (will add it to exclusion list)
19:30:16.62 +66:01:35.2 -- not an asteroid (will add it to exclusion list)
21:01:00.08 +58:53:02.6 -- not an asteroid (will add it to exclusion list)
19:23:26.61 +66:08:26.9 -- not an asteroid (will add it to exclusion list)
19:27:12.09 +66:17:02.6 -- not an asteroid (will add it to exclusion list)
21:10:59.36 +58:41:14.6 -- not an asteroid (will add it to exclusion list)
20:59:44.15 +59:18:39.0 -- not an asteroid (will add it to exclusion list)
21:18:50.77 +58:52:25.2 -- not an asteroid (will add it to exclusion list)
21:02:52.30 +59:13:23.5 -- not an asteroid (will add it to exclusion list)
21:05:15.17 +59:10:38.8 -- not an asteroid (will add it to exclusion list)
21:00:06.21 +59:07:32.4 -- not an asteroid (will add it to exclusion list)
21:12:30.11 +58:37:41.5 -- not an asteroid (will add it to exclusion list)
20:58:00.93 +60:26:12.3 -- not an asteroid (will add it to exclusion list)
21:18:12.04 +58:40:09.5 -- not an asteroid (will add it to exclusion list)
21:31:36.45 +58:22:22.5 -- not an asteroid (will add it to exclusion list)
21:09:52.17 +58:33:06.6 -- not an asteroid (will add it to exclusion list)
20:58:04.91 +61:04:17.8 -- not an asteroid (will add it to exclusion list)
21:25:39.04 +59:41:25.9 -- not an asteroid (will add it to exclusion list)
21:08:14.66 +58:54:37.4 -- not an asteroid (will add it to exclusion list)
21:02:39.13 +59:06:38.5 -- not an asteroid (will add it to exclusion list)
20:57:49.39 +60:14:52.2 -- not an asteroid (will add it to exclusion list)
21:09:45.37 +58:42:55.6 -- not an asteroid (will add it to exclusion list)
21:02:07.23 +59:42:45.1 -- not an asteroid (will add it to exclusion list)
20:55:42.34 +60:07:57.2 -- not an asteroid (will add it to exclusion list)
21:22:51.08 +59:05:32.6 -- not an asteroid (will add it to exclusion list)
21:09:13.88 +58:54:23.1 -- not an asteroid (will add it to exclusion list)
20:59:27.33 +59:38:08.9 -- not an asteroid (will add it to exclusion list)
21:02:59.83 +59:03:36.8 -- not an asteroid (will add it to exclusion list)
21:26:27.24 +59:48:39.9 -- not an asteroid (will add it to exclusion list)
21:26:20.50 +59:48:22.6 -- not an asteroid (will add it to exclusion list)
21:11:15.42 +58:55:27.1 -- not an asteroid (will add it to exclusion list)
20:58:51.00 +59:56:15.8 -- not an asteroid (will add it to exclusion list)
21:02:11.57 +59:48:34.2 -- not an asteroid (will add it to exclusion list)
20:56:59.63 +60:45:20.4 -- not an asteroid (will add it to exclusion list)
21:02:33.12 +59:52:22.7 -- not an asteroid (will add it to exclusion list)
21:24:00.22 +59:43:41.2 -- not an asteroid (will add it to exclusion list)
21:10:09.15 +58:41:49.2 -- not an asteroid (will add it to exclusion list)
19:37:34.84 +57:09:53.9 -- not an asteroid (will add it to exclusion list)
20:58:08.10 +58:16:49.6 -- not an asteroid (will add it to exclusion list)
20:58:54.54 +60:02:20.0 -- not an asteroid (will add it to exclusion list)
21:10:50.99 +58:43:26.6 -- not an asteroid (will add it to exclusion list)
19:33:39.97 +59:15:24.4 -- not an asteroid (will add it to exclusion list)
20:55:49.18 +59:47:24.2 -- not an asteroid (will add it to exclusion list)
19:25:43.80 +65:30:51.4 -- not an asteroid (will add it to exclusion list)
19:27:48.70 +66:07:31.6 -- not an asteroid (will add it to exclusion list)
21:07:57.31 +59:22:42.1 -- not an asteroid (will add it to exclusion list)
20:39:20.73 +59:16:40.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:23:26.61 +66:08:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:32.20 +65:56:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:54.10 +65:56:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:56.39 +65:30:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:13.08 +65:17:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:21.96 +65:41:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:50.71 +65:44:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:43.80 +65:30:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:01.40 +65:26:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:16.35 +66:01:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:26:19.93 +65:28:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:12.09 +66:17:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:20.84 +65:33:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:21.85 +65:54:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:30.14 +66:05:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:48.70 +66:07:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:50.79 +65:55:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:28:25.73 +66:09:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:28:39.36 +66:16:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:26.70 +66:02:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:28.25 +65:54:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:30.80 +66:01:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:03.39 +65:57:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:16.62 +66:01:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:22.58 +66:03:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:40.53 +66:21:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:42.54 +66:01:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:48.17 +66:22:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:53.45 +66:21:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:04.00 +65:56:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:05.29 +66:10:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:14.74 +65:55:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:27.58 +65:54:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:50.63 +66:12:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:54.56 +66:01:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:31.11 +65:59:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:17.80 +65:57:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:39.97 +59:15:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:57.50 +66:20:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:24.38 +65:10:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:56.71 +66:01:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:29.60 +66:29:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:34.18 +66:27:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:34.84 +57:09:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:37.78 +66:19:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:48.01 +66:31:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:12.45 +66:31:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:22.71 +66:00:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:26.91 +65:58:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:27.19 +65:50:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:37.88 +66:21:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:40.00 +65:07:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:10.71 +64:46:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:01.58 +66:22:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:45.67 +66:24:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:54.83 +66:28:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:58.65 +66:37:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:44.01 +66:38:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:42.01 +66:41:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:13.62 +66:53:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:20.73 +59:16:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:02.70 +58:55:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:14.93 +59:07:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:05.61 +58:53:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:42.34 +60:07:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:44.69 +60:44:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:49.18 +59:47:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:55.86 +60:31:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:59.56 +60:28:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:00.54 +60:25:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:22.53 +60:33:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:25.11 +61:00:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:38.83 +60:14:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:50.52 +60:47:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:58.40 +60:16:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:59.63 +60:45:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:02.38 +61:18:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:18.13 +60:16:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:36.85 +60:49:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:41.34 +59:29:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:49.39 +60:14:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:55.84 +60:59:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:00.93 +60:26:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:02.21 +60:39:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:04.91 +61:04:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:08.10 +58:16:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:39.33 +60:42:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:51.00 +59:56:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:54.54 +60:02:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:11.34 +59:56:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:27.33 +59:38:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:34.78 +59:31:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:44.15 +59:18:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:44.23 +60:32:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:55.88 +59:11:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:57.54 +59:09:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:06.21 +59:07:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:17.49 +59:12:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:31.82 +58:27:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:50.07 +58:35:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:00.08 +58:53:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:23.16 +59:16:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:31.78 +59:14:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.02 +59:00:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:46.36 +59:34:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:53.55 +59:23:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:07.23 +59:42:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:11.57 +59:48:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:33.12 +59:52:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:39.13 +59:06:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:52.30 +59:13:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:59.83 +59:03:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:05.67 +59:17:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:26.39 +58:57:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:27.39 +59:10:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:15.17 +59:10:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:07:57.31 +59:22:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:14.66 +58:54:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:53.44 +58:28:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:09.15 +58:40:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:13.88 +58:54:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:22.48 +58:51:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:25.31 +58:40:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:32.55 +58:54:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:45.37 +58:42:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:52.17 +58:33:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:59.60 +58:45:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:02.27 +58:50:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:09.15 +58:41:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:18.73 +58:47:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:26.67 +59:03:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:39.35 +58:55:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:50.99 +58:43:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:59.36 +58:41:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:15.42 +58:55:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:21.74 +58:49:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:45.27 +59:06:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:52.50 +59:01:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:30.11 +58:37:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:29.33 +58:09:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:23.70 +58:51:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:12.04 +58:40:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:50.77 +58:52:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:51.12 +59:14:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:51.08 +59:05:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:22:53.63 +59:37:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:00.95 +59:19:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:15.30 +59:49:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:22.05 +59:48:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:36.40 +59:37:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:40.72 +58:59:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:00.22 +59:43:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:08.16 +61:40:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:27.49 +59:09:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:37.01 +59:20:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:39.32 +59:43:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:05.78 +59:49:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:07.48 +59:52:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:39.04 +59:41:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:57.61 +59:36:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:59.43 +59:39:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:17.42 +59:27:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:20.50 +59:48:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:27.24 +59:48:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:03.89 +59:39:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:27.51 +59:37:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:36.45 +58:22:22.5 -- 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)
19:23:26.61 +66:08:26.9 -- not a known variable star
19:23:32.20 +65:56:25.4 -- not a known variable star
19:23:54.10 +65:56:11.8 -- not a known variable star
19:23:56.39 +65:30:47.2 -- not a known variable star
19:24:13.08 +65:17:39.4 -- not a known variable star
19:24:21.96 +65:41:39.7 -- not a known variable star
19:24:50.71 +65:44:49.2 -- not a known variable star
19:25:43.80 +65:30:51.4 -- not a known variable star
19:26:01.40 +65:26:32.5 -- not a known variable star
19:26:16.35 +66:01:21.1 -- not a known variable star
19:26:19.93 +65:28:02.2 -- not a known variable star
19:27:12.09 +66:17:02.6 -- not a known variable star
19:27:20.84 +65:33:47.2 -- a known variable star
19:27:21.85 +65:54:08.4 -- not a known variable star
19:27:30.14 +66:05:06.0 -- not a known variable star
19:27:48.70 +66:07:31.6 -- not a known variable star
19:27:50.79 +65:55:45.9 -- not a known variable star
19:28:25.73 +66:09:11.5 -- not a known variable star
19:28:39.36 +66:16:56.7 -- not a known variable star
19:29:26.70 +66:02:10.2 -- not a known variable star
19:29:28.25 +65:54:31.4 -- not a known variable star
19:29:30.80 +66:01:24.3 -- not a known variable star
19:30:03.39 +65:57:08.9 -- not a known variable star
19:30:16.62 +66:01:35.2 -- a known variable star
19:30:22.58 +66:03:40.6 -- not a known variable star
19:30:40.53 +66:21:20.5 -- not a known variable star
19:30:42.54 +66:01:17.3 -- not a known variable star
19:30:48.17 +66:22:02.2 -- not a known variable star
19:30:53.45 +66:21:35.8 -- not a known variable star
19:31:04.00 +65:56:51.5 -- not a known variable star
19:31:05.29 +66:10:19.2 -- not a known variable star
19:31:14.74 +65:55:03.9 -- not a known variable star
19:31:27.58 +65:54:59.2 -- not a known variable star
19:31:50.63 +66:12:14.3 -- not a known variable star
19:31:54.56 +66:01:02.8 -- not a known variable star
19:32:31.11 +65:59:09.8 -- not a known variable star
19:33:17.80 +65:57:04.3 -- not a known variable star
19:33:39.97 +59:15:24.4 -- not a known variable star
19:35:57.50 +66:20:20.7 -- not a known variable star
19:36:24.38 +65:10:26.4 -- a known variable star
19:36:56.71 +66:01:07.1 -- not a known variable star
19:37:29.60 +66:29:52.9 -- not a known variable star
19:37:34.18 +66:27:06.3 -- not a known variable star
19:37:34.84 +57:09:53.9 -- not a known variable star
19:37:37.78 +66:19:57.0 -- not a known variable star
19:37:48.01 +66:31:57.0 -- not a known variable star
19:38:12.45 +66:31:00.6 -- not a known variable star
19:38:22.71 +66:00:48.3 -- not a known variable star
19:38:26.91 +65:58:47.8 -- not a known variable star
19:38:27.19 +65:50:28.9 -- not a known variable star
19:38:37.88 +66:21:08.3 -- not a known variable star
19:38:40.00 +65:07:39.1 -- not a known variable star
19:39:10.71 +64:46:34.5 -- not a known variable star
19:40:01.58 +66:22:20.4 -- not a known variable star
19:42:45.67 +66:24:52.4 -- not a known variable star
19:43:54.83 +66:28:24.4 -- not a known variable star
19:43:58.65 +66:37:08.8 -- a known variable star
19:47:44.01 +66:38:34.4 -- not a known variable star
19:49:42.01 +66:41:57.4 -- not a known variable star
20:00:13.62 +66:53:49.9 -- not a known variable star
20:39:20.73 +59:16:40.7 -- a known variable star
20:42:02.70 +58:55:19.5 -- a known variable star
20:44:14.93 +59:07:57.8 -- a known variable star
20:49:05.61 +58:53:57.4 -- a known variable star
20:55:42.34 +60:07:57.2 -- not a known variable star
20:55:44.69 +60:44:23.8 -- not a known variable star
20:55:49.18 +59:47:24.2 -- not a known variable star
20:55:55.86 +60:31:40.0 -- a known variable star
20:55:59.56 +60:28:49.1 -- not a known variable star
20:56:00.54 +60:25:05.7 -- not a known variable star
20:56:22.53 +60:33:25.7 -- not a known variable star
20:56:25.11 +61:00:21.8 -- not a known variable star
20:56:38.83 +60:14:56.7 -- a known variable star
20:56:50.52 +60:47:43.6 -- not a known variable star
20:56:58.40 +60:16:13.3 -- not a known variable star
20:56:59.63 +60:45:20.4 -- a known variable star
20:57:02.38 +61:18:01.7 -- a known variable star
20:57:18.13 +60:16:59.1 -- not a known variable star
20:57:36.85 +60:49:12.7 -- not a known variable star
20:57:41.34 +59:29:45.2 -- a known variable star
20:57:49.39 +60:14:52.2 -- not a known variable star
20:57:55.84 +60:59:51.1 -- not a known variable star
20:58:00.93 +60:26:12.3 -- not a known variable star
20:58:02.21 +60:39:58.5 -- not a known variable star
20:58:04.91 +61:04:17.8 -- not a known variable star
20:58:08.10 +58:16:49.6 -- not a known variable star
20:58:39.33 +60:42:44.9 -- not a known variable star
20:58:51.00 +59:56:15.8 -- a known variable star
20:58:54.54 +60:02:20.0 -- not a known variable star
20:59:11.34 +59:56:10.5 -- not a known variable star
20:59:27.33 +59:38:08.9 -- not a known variable star
20:59:34.78 +59:31:00.7 -- not a known variable star
20:59:44.15 +59:18:39.0 -- not a known variable star
20:59:44.23 +60:32:31.4 -- not a known variable star
20:59:55.88 +59:11:31.6 -- not a known variable star
20:59:57.54 +59:09:21.8 -- not a known variable star
21:00:06.21 +59:07:32.4 -- not a known variable star
21:00:17.49 +59:12:01.0 -- not a known variable star
21:00:31.82 +58:27:53.3 -- not a known variable star
21:00:50.07 +58:35:50.2 -- not a known variable star
21:01:00.08 +58:53:02.6 -- not a known variable star
21:01:23.16 +59:16:47.5 -- not a known variable star
21:01:31.78 +59:14:23.1 -- not a known variable star
21:01:45.02 +59:00:58.6 -- not a known variable star
21:01:46.36 +59:34:54.4 -- not a known variable star
21:01:53.55 +59:23:58.7 -- a known variable star
21:02:07.23 +59:42:45.1 -- a known variable star
21:02:11.57 +59:48:34.2 -- a known variable star
21:02:33.12 +59:52:22.7 -- not a known variable star
21:02:39.13 +59:06:38.5 -- not a known variable star
21:02:52.30 +59:13:23.5 -- not a known variable star
21:02:59.83 +59:03:36.8 -- not a known variable star
21:03:05.67 +59:17:33.8 -- not a known variable star
21:03:26.39 +58:57:08.5 -- not a known variable star
21:03:27.39 +59:10:26.3 -- not a known variable star
21:05:15.17 +59:10:38.8 -- not a known variable star
21:07:57.31 +59:22:42.1 -- a known variable star
21:08:14.66 +58:54:37.4 -- not a known variable star
21:08:53.44 +58:28:55.7 -- a known variable star
21:09:09.15 +58:40:25.0 -- not a known variable star
21:09:13.88 +58:54:23.1 -- not a known variable star
21:09:22.48 +58:51:24.7 -- not a known variable star
21:09:25.31 +58:40:42.5 -- not a known variable star
21:09:32.55 +58:54:52.0 -- not a known variable star
21:09:45.37 +58:42:55.6 -- not a known variable star
21:09:52.17 +58:33:06.6 -- not a known variable star
21:09:59.60 +58:45:20.1 -- not a known variable star
21:10:02.27 +58:50:47.2 -- not a known variable star
21:10:09.15 +58:41:49.2 -- not a known variable star
21:10:18.73 +58:47:48.7 -- not a known variable star
21:10:26.67 +59:03:25.0 -- not a known variable star
21:10:39.35 +58:55:53.9 -- not a known variable star
21:10:50.99 +58:43:26.6 -- not a known variable star
21:10:59.36 +58:41:14.6 -- a known variable star
21:11:15.42 +58:55:27.1 -- not a known variable star
21:11:21.74 +58:49:49.2 -- not a known variable star
21:11:45.27 +59:06:01.3 -- not a known variable star
21:11:52.50 +59:01:04.1 -- a known variable star
21:12:30.11 +58:37:41.5 -- not a known variable star
21:13:29.33 +58:09:45.0 -- a known variable star
21:14:23.70 +58:51:51.9 -- not a known variable star
21:18:12.04 +58:40:09.5 -- not a known variable star
21:18:50.77 +58:52:25.2 -- not a known variable star
21:20:51.12 +59:14:08.1 -- not a known variable star
21:22:51.08 +59:05:32.6 -- not a known variable star
21:22:53.63 +59:37:09.5 -- not a known variable star
21:23:00.95 +59:19:20.8 -- not a known variable star
21:23:15.30 +59:49:21.6 -- not a known variable star
21:23:22.05 +59:48:19.9 -- not a known variable star
21:23:36.40 +59:37:50.8 -- not a known variable star
21:23:40.72 +58:59:22.6 -- not a known variable star
21:24:00.22 +59:43:41.2 -- not a known variable star
21:24:08.16 +61:40:56.4 -- a known variable star
21:24:27.49 +59:09:56.6 -- not a known variable star
21:24:37.01 +59:20:33.2 -- not a known variable star
21:24:39.32 +59:43:01.8 -- a known variable star
21:25:05.78 +59:49:01.9 -- not a known variable star
21:25:07.48 +59:52:30.9 -- a known variable star
21:25:39.04 +59:41:25.9 -- a known variable star
21:25:57.61 +59:36:56.1 -- not a known variable star
21:25:59.43 +59:39:01.8 -- a known variable star
21:26:17.42 +59:27:42.6 -- not a known variable star
21:26:20.50 +59:48:22.6 -- not a known variable star
21:26:27.24 +59:48:39.9 -- not a known variable star
21:30:03.89 +59:39:40.9 -- not a known variable star
21:30:27.51 +59:37:56.0 -- not a known variable star
21:31:36.45 +58:22:22.5 -- a known variable star
Found 139 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
167 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 167 (excluding asteroids and hot pixels, 139 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461265.86424481 -observatory V36
08:33:41.49 +19:29:50.5 Mercury (-1.1mag)
12:20:36.37 -03:32:22.6 Venus (-4.4mag)
06:04:10.59 +23:41:41.5 Mars (1.3mag)
08:47:33.34 +18:23:57.1 Jupiter (-1.8mag)
00:55:58.50 +03:11:09.4 Saturn (0.6mag)
04:12:17.01 +20:58:23.0 Uranus (5.7mag)
00:15:46.98 +00:10:51.5 Neptune (7.7mag)
20:27:39.29 -23:32:06.7 Pluto (14.5mag)
10:04:28.63 +11:18:43.0 Moon (-8.3mag)
-rw-r--r-- 1 apache apache 362 Aug 13 03:47 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461265.86424481:
08:47:39.46 +18:23:30.1 Io (6.1mag)
08:47:29.64 +18:24:14.2 Europa (6.3mag)
08:47:29.31 +18:24:18.7 Ganymede (5.6mag)
08:47:59.31 +18:22:02.4 Callisto (6.8mag)
08:45:02.91 +18:26:28.7 Himalia (15.7mag)
08:47:37.78 +18:23:38.6 Thebe (16.6mag)
08:44:38.10 +18:23:59.9 Elara (17.7mag)
08:51:41.85 +18:01:03.3 Pasiphae (17.9mag)
08:50:23.54 +18:35:22.6 Carme (19.0mag)
00:55:55.94 +03:10:36.4 Titan (8.4mag)
00:56:03.16 +03:11:02.0 Rhea (9.7mag)
00:56:21.13 +03:10:59.0 Iapetus (11.1mag)
00:56:00.81 +03:10:26.0 Hyperion (14.4mag)
00:55:14.37 +03:03:40.4 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 13 03:47 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461265.86424481:
19:24:28.20 -20:12:31.5 JWST
14:25:37.40 +53:21:50.6 Chandra
06:00:46.47 +30:36:14.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 13 03:47 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461265.86424481 -observatory V36
03:19:20.65 +17:47:40.2 17.6mag P/1996 R2 (Lagerkvist)
18:00:35.95 -34:35:11.9 14.0mag P/2010 H2 (Vales)
06:58:31.54 -69:05:58.0 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:11:08.05 +33:06:13.9 17.7mag C/2017 K2 (PANSTARRS)
03:58:25.37 +39:43:07.1 17.0mag P/2021 N1 (ZTF)
22:34:21.36 +31:06:42.9 17.3mag C/2022 E2 (ATLAS)
06:48:32.11 +26:27:02.6 16.8mag C/2022 N2 (PANSTARRS)
10:26:20.22 +28:14:24.6 17.0mag C/2022 QE78 (ATLAS)
09:32:18.60 +05:18:34.0 17.9mag C/2022 R6 (PANSTARRS)
15:13:25.63 -12:29:27.1 17.9mag P/2023 B1 (PANSTARRS)
21:04:03.95 +65:23:52.3 17.9mag C/2023 H5 (Lemmon)
15:43:03.01 -13:24:50.0 14.4mag C/2023 R1 (PANSTARRS)
08:13:47.56 +31:34:50.7 15.4mag C/2024 E1 (Wierzchos)
15:06:15.40 +15:34:57.6 17.8mag C/2024 G6 (ATLAS)
18:56:48.54 +43:19:34.2 13.7mag C/2024 J3 (ATLAS)
21:03:03.07 +49:28:34.8 17.6mag C/2024 R4 (PANSTARRS)
05:19:11.10 -12:55:12.1 15.4mag C/2024 T5 (ATLAS)
06:59:29.38 +23:14:41.3 17.9mag C/2025 J1 (Borisov)
07:32:52.12 -16:52:19.0 17.9mag C/2025 R3 (PANSTARRS)
10:40:07.97 +20:34:28.2 17.2mag C/2025 V2 (Rankin)
13:01:18.60 +02:00:06.6 16.9mag C/2025 Y1 (ATLAS)
16:03:22.15 +77:19:10.8 16.7mag C/2026 A2 (Bok)
03:09:02.35 +46:16:36.5 17.2mag C/2026 B2 (Sun-Gao)
11:51:04.76 +09:04:46.8 17.3mag A/2026 E1
22:03:48.58 -29:21:11.7 7.0mag 10P/Tempel
11:32:04.55 -03:43:18.9 16.3mag 29P/Schwassmann-Wachmann
04:45:29.33 +32:55:01.7 18.0mag 47P/Ashbrook-Jackson
11:18:10.04 +02:57:28.8 17.3mag 63P/Wild
00:53:42.10 -05:39:20.4 15.4mag 65P/Gunn
05:47:08.26 +20:35:05.2 13.7mag 78P/Gehrels
20:33:20.11 -24:06:12.7 17.6mag 84P/Giclas
03:05:30.33 +14:02:56.8 16.8mag 88P/Howell
08:08:52.58 +26:56:38.1 16.2mag 93P/Lovas
04:20:57.33 +18:52:41.6 17.4mag 112P/Urata-Niijima
06:13:26.25 +29:42:18.5 16.2mag 114P/Wiseman-Skiff
09:30:39.69 +25:45:33.8 15.0mag 123P/West-Hartley
11:54:03.10 -12:14:01.7 17.2mag 124P/Mrkos
05:44:04.96 +21:08:58.1 16.1mag 128P/Shoemaker-Holt
06:37:14.66 +18:38:17.1 17.9mag 131P/Mueller
00:02:22.46 +03:20:16.0 17.5mag 139P/Vaisala-Oterma
03:17:52.19 -18:58:18.7 13.5mag 161P/Hartley-IRAS
07:33:48.53 +38:01:15.3 15.9mag 162P/SidingSpring
13:27:42.88 +40:48:45.8 12.0mag 169P/NEAT
02:52:07.32 +09:33:04.6 17.6mag 220P/McNaught
16:44:29.08 -10:28:01.4 17.8mag 235P/LINEAR
20:19:19.91 -52:39:10.7 17.9mag 259P/Garradd
03:37:08.19 +27:18:31.8 15.3mag 260P/McNaught
07:20:50.18 +37:33:47.3 17.3mag 295P/LINEAR
15:12:16.53 +02:34:07.1 17.8mag 391P/Kowalski
09:05:34.70 +18:07:20.1 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 13 03:47 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
-rw-r--r-- 1 apache apache 190K Aug 13 03:47 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:52:57.976 +33:57:42.42 AT 2026wpj 2026-07-21.38 20.2881
23:05:20.855 +37:19:46.09 AT 2026wpi 2026-07-22.37 21.0894
19:59:56.516 +50:04:12.95 AT 2026wph 2026-06-09.39 19.6831
21:38:56.950 -14:47:13.40 AT 2026wpg 2026-07-27.34 19.8349
10:38:44.628 +53:30:05.28 AT 2026wpf 2026-07-30.75 15
19:30:54.423 -04:13:56.01 AT 2026wpe 2026-08-02.23 18.2988
01:28:20.623 +40:13:26.65 SN 2026wpd 2026-08-01.50 18.264
19:14:14.360 -08:23:17.18 AT 2026wpc 2026-07-16.27 16.4563
17:30:15.259 +75:34:03.18 AT 2026wpb 2026-07-23.28 20.7507
18:41:41.346 +36:04:18.98 AT 2026wpa 2026-07-28.24 20.2756
11:44:41.850 +35:58:18.99 AT 2026woz 2026-07-27.16 19.2219
16:40:37.874 -01:07:30.43 AT 2026woy 2026-07-22.18 20.4047
15:38:03.502 -05:11:41.15 AT 2026wox 2026-07-20.18 20.5151
18:28:32.457 +42:57:28.98 AT 2026wow 2026-07-24.35 20.7464
18:00:39.265 +51:42:53.99 SN 2026wov 2026-07-22.33 21.0926
18:44:42.741 +19:36:15.57 AT 2026wou 2026-07-27.30 20.2793
15:41:26.080 -16:40:01.56 AT 2026wot 2026-07-28.19 19.0974
15:06:59.340 +10:34:40.09 AT 2026wos 2026-08-02.18 19.3236
18:18:44.104 +68:21:06.31 AT 2026wor 2026-07-27.32 20.2081
19:20:43.805 +66:32:12.77 SN 2026woq 2026-07-28.33 19.5651
-rw-r--r-- 1 apache apache 87K Aug 13 03:47 tns_transients_list.txt
