This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 10.52 21:27:40.11 +57:16:00.3
98.01876 4.60815 galactic Cep Second-epoch detections are separated by 6.1" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:27:40.11 +57:16:00.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:27:40.11 +57:16:00.3: 14.78 +/- 0.23 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:27:40.11 +57:16:00.3: 14.76 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 11.85 21:15:55.75 +54:48:14.3
95.11016 4.02659 galactic Cyg Second-epoch detections are separated by 8.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:15:55.75 +54:48:14.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:15:55.75 +54:48:14.3: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:15:55.75 +54:48:14.3: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 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 06 20.4285 2461211.9285 11.96 21:09:14.63 +54:35:04.7
94.28638 4.58003 galactic Cyg Second-epoch detections are separated by 7.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:09:14.63 +54:35:04.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:09:14.63 +54:35:04.7: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:09:14.63 +54:35:04.7: 15.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 12.05 20:58:44.50 +54:58:26.5
93.57047 5.97143 galactic Cyg Second-epoch detections are separated by 7.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:44.50 +54:58:26.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:58:44.50 +54:58:26.5: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:58:44.50 +54:58:26.5: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 12.04 21:20:24.89 +53:46:00.6
94.82574 2.83349 galactic Cyg Second-epoch detections are separated by 5.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:20:24.89 +53:46:00.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:20:24.89 +53:46:00.6: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:20:24.89 +53:46:00.6: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 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 06 20.4285 2461211.9285 12.06 21:15:00.93 +52:48:20.7
93.57288 2.73967 galactic Cyg Second-epoch detections are separated by 3.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:15:00.93 +52:48:20.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:15:00.93 +52:48:20.7: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:15:00.93 +52:48:20.7: 15.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 12.02 21:28:45.06 +52:13:13.3
94.64185 0.85092 galactic Cyg Second-epoch detections are separated by 6.0" and 4.7 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 2172532893704029440 | 21:28:46.20 +52:13:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:28:45.06 +52:13:13.3: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:28:45.06 +52:13:13.3: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2172532893704029440,2461211.9285,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2172532893704029440 20260620.4285 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 12.05 21:35:26.37 +53:29:06.7
96.24250 1.09119 galactic Cyg Second-epoch detections are separated by 4.2" and 4.4 pix
The object was found in VSX17" Gaia DR3 2174193465502871424
Type: ROT
# Max. Min./Amp. JD0 Period
16.090 G 16.130 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:26.37 +53:29:06.7: 15.16 +/- 0.34 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:26.37 +53:29:06.7: 15.22 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.16 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2174193465502871424,2461211.9285,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2174193465502871424 20260620.4285 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 10.80 21:35:51.53 +51:14:27.7
94.78366 -0.61538 galactic Cyg Second-epoch detections are separated by 8.1" and 4.6 pix
The object was found in VSX17" V1728 Cyg
Type: M
# Max. Min./Amp. JD0 Period
10.000 R 13.000 R 277.000000000000 M7-M9
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:51.53 +51:14:27.7: 12.46 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:51.53 +51:14:27.7: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1728 Cyg,2461211.9285,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1728 Cyg 20260620.4285 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.48 21:24:45.67 +54:10:57.0
95.57305 2.67863 galactic Cyg Second-epoch detections are separated by 3.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:24:45.67 +54:10:57.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:24:45.67 +54:10:57.0: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:24:45.67 +54:10:57.0: 15.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.33 21:31:17.47 +51:25:39.5
94.38442 0.00464 galactic Cyg Second-epoch detections are separated by 6.8" and 4.4 pix
The object was found in VSX10" Gaia DR3 2171687133050834304
Type: RS
# Max. Min./Amp. JD0 Period
15.250 G 15.350 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:31:17.47 +51:25:39.5: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:31:17.47 +51:25:39.5: 15.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171687133050834304,2461211.9285,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171687133050834304 20260620.4285 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.46 21:38:48.17 +54:12:18.2
97.09256 1.29605 galactic Cyg Second-epoch detections are separated by 4.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:38:48.17 +54:12:18.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:48.17 +54:12:18.2: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:48.17 +54:12:18.2: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.40 21:34:28.21 +55:37:27.2
97.57965 2.76730 galactic Cep Second-epoch detections are separated by 3.8" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:28.21 +55:37:27.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:34:28.21 +55:37:27.2: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:34:28.21 +55:37:27.2: 15.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.32 21:36:07.30 +52:33:31.8
95.69706 0.33540 galactic Cyg Second-epoch detections are separated by 5.6" and 4.7 pix
The object was found in VSX13" ZTF J213605.92+523332.4
Type: EW
# Max. Min./Amp. JD0 Period
17.691 r Y 0.468 r 2458431.65420 0.597226000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:36:07.30 +52:33:31.8: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:36:07.30 +52:33:31.8: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J213605.92+523332.4,2461211.9285,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J213605.92+523332.4 20260620.4285 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.36 21:26:29.43 +49:53:58.3
92.78094 -0.58071 galactic Cyg Second-epoch detections are separated by 5.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.6124+49.9010 | 21:26:29.43 +49:53:58.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:26:29.43 +49:53:58.3: 15.47 +/- 0.33 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:26:29.43 +49:53:58.3: 15.50 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.47 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J321.6124+49.9010,2461211.9285,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.6124+49.9010 20260620.4285 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.44 21:10:39.98 +55:32:47.6
95.13444 5.08268 galactic Cep Second-epoch detections are separated by 4.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:10:39.98 +55:32:47.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:10:39.98 +55:32:47.6: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:10:39.98 +55:32:47.6: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.32 21:35:23.50 +51:40:26.6
95.02038 -0.24555 galactic Cyg Second-epoch detections are separated by 4.9" and 4.7 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 | 21:35:23.50 +51:40:26.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:23.50 +51:40:26.6: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:23.50 +51:40:26.6: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.23 21:42:13.87 +57:07:35.2
99.38337 3.17447 galactic Cep Second-epoch detections are separated by 3.1" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:13.87 +57:07:35.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:42:13.87 +57:07:35.2: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:42:13.87 +57:07:35.2: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.23CV 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 06 20.4285 2461211.9285 14.35 21:30:23.78 +54:47:04.6
96.58153 2.54691 galactic Cyg Second-epoch detections are separated by 6.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:23.78 +54:47:04.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:30:23.78 +54:47:04.6: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:30:23.78 +54:47:04.6: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.35CV 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 06 20.4285 2461211.9285 14.31 21:18:03.19 +54:36:11.6
95.17970 3.66657 galactic Cyg Second-epoch detections are separated by 6.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.4986+54.6028 | 21:18:03.19 +54:36:11.6 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:18:03.19 +54:36:11.6: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:18:03.19 +54:36:11.6: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J319.4986+54.6028,2461211.9285,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.4986+54.6028 20260620.4285 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.26 21:31:58.61 +50:55:32.5
94.12111 -0.43601 galactic Cyg Second-epoch detections are separated by 7.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:31:58.61 +50:55:32.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:31:58.61 +50:55:32.5: 15.38 +/- 0.29 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:31:58.61 +50:55:32.5: 15.10 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.22 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.40 21:43:07.54 +57:55:26.0
99.99690 3.69914 galactic Cep Second-epoch detections are separated by 5.3" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.7828+57.9259 | 21:43:07.54 +57:55:26.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:43:07.54 +57:55:26.0: 15.44 +/- 0.32 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:43:07.54 +57:55:26.0: 15.36 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.7828+57.9259,2461211.9285,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.7828+57.9259 20260620.4285 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.42 21:18:31.91 +57:59:35.9
97.66242 5.98554 galactic Cep Second-epoch detections are separated by 4.9" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:18:31.91 +57:59:35.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:18:31.91 +57:59:35.9: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:18:31.91 +57:59:35.9: 15.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.45 20:53:11.08 +49:55:09.3
89.14605 3.35944 galactic Cyg Second-epoch detections are separated by 5.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.2897+49.9088 | 20:53:11.08 +49:55:09.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:53:11.08 +49:55:09.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:53:11.08 +49:55:09.3: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J313.2897+49.9088,2461211.9285,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J313.2897+49.9088 20260620.4285 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.49 21:15:33.37 +58:11:01.9
97.52625 6.40101 galactic Cep Second-epoch detections are separated by 5.6" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.8831+58.1767 | 21:15:33.37 +58:11:01.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:15:33.37 +58:11:01.9: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:15:33.37 +58:11:01.9: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J318.8831+58.1767,2461211.9285,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.8831+58.1767 20260620.4285 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.21 21:39:36.79 +56:01:25.9
98.38487 2.58190 galactic Cep Second-epoch detections are separated by 1.8" and 4.7 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 | 21:39:36.79 +56:01:25.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:36.79 +56:01:25.9: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:36.79 +56:01:25.9: 15.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.43 20:43:10.69 +55:27:28.7
92.54303 8.00116 galactic Cep Second-epoch detections are separated by 6.2" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:43:10.69 +55:27:28.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:10.69 +55:27:28.7: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:10.69 +55:27:28.7: 15.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.61 20:51:34.30 +58:10:50.6
95.42472 8.77762 galactic Cep Second-epoch detections are separated by 5.9" and 4.5 pix
The object was found in VSX20" Gaia DR3 2190403157412191104
Type: RS
# Max. Min./Amp. JD0 Period
17.640 G 17.750 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:51:34.30 +58:10:50.6: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:51:34.30 +58:10:50.6: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2190403157412191104,2461211.9285,14.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2190403157412191104 20260620.4285 14.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.19 21:41:38.76 +56:10:24.3
98.69694 2.50761 galactic Cep Second-epoch detections are separated by 7.0" and 4.0 pix
The object was found in VSX15" ZTF J214138.77+561009.0
Type: RS
# Max. Min./Amp. JD0 Period
18.594 r Y 0.116 r 2458588.92330 0.232946100000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:38.76 +56:10:24.3: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:38.76 +56:10:24.3: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J214138.77+561009.0,2461211.9285,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J214138.77+561009.0 20260620.4285 14.19CV 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 06 20.4285 2461211.9285 14.47 20:43:06.81 +53:39:55.0
91.10338 6.91660 galactic Cyg Second-epoch detections are separated by 5.4" and 4.7 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 | 20:43:06.81 +53:39:55.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:06.81 +53:39:55.0: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:06.81 +53:39:55.0: 15.48 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.48 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.47CV 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 06 20.4285 2461211.9285 14.31 21:41:58.93 +56:33:06.9
98.98063 2.76280 galactic Cep Second-epoch detections are separated by 2.4" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5072+56.5490 | 21:41:58.93 +56:33:06.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=-0.080+/- (B)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:58.93 +56:33:06.9: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:58.93 +56:33:06.9: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.5072+56.5490,2461211.9285,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.5072+56.5490 20260620.4285 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.35 21:16:08.72 +56:47:44.5
96.57238 5.38463 galactic Cep Second-epoch detections are separated by 7.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:16:08.72 +56:47:44.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:16:08.72 +56:47:44.5: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:16:08.72 +56:47:44.5: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.35CV 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 06 20.4285 2461211.9285 14.28 21:35:59.50 +50:54:17.5
94.57372 -0.87877 galactic Cyg Second-epoch detections are separated by 5.2" and 4.8 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 J323.9897+50.8999 | 21:35:59.50 +50:54:17.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:59.50 +50:54:17.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:59.50 +50:54:17.5: 15.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J323.9897+50.8999,2461211.9285,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.9897+50.8999 20260620.4285 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.24 21:34:20.99 +51:20:57.2
94.68185 -0.37665 galactic Cyg Second-epoch detections are separated by 3.1" and 4.4 pix
The object was found in VSX25" Gaia DR3 2171721561509034368
Type: L
# Max. Min./Amp. JD0 Period
16.030 G 16.440 G M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:34:20.99 +51:20:57.2: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:34:20.99 +51:20:57.2: 15.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171721561509034368,2461211.9285,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2171721561509034368 20260620.4285 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.03 21:37:46.83 +50:47:24.9
94.70728 -1.15269 galactic Cyg Second-epoch detections are separated by 1.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:46.83 +50:47:24.9 (user input) | T | P | (position from user input) J-Ks=0.652+/-0.069 (K)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:46.83 +50:47:24.9: 15.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:46.83 +50:47:24.9: 15.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.27 21:08:54.08 +57:28:41.9
96.39912 6.56862 galactic Cep Second-epoch detections are separated by 5.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:08:54.08 +57:28:41.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:08:54.08 +57:28:41.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:08:54.08 +57:28:41.9: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.27CV 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 06 20.4285 2461211.9285 14.19 21:43:00.71 +56:39:42.5
99.15988 2.75324 galactic Cep Second-epoch detections are separated by 5.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:43:00.71 +56:39:42.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:43:00.71 +56:39:42.5: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:43:00.71 +56:39:42.5: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.19CV 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 06 20.4285 2461211.9285 14.35 20:45:48.56 +53:45:55.1
91.42944 6.66312 galactic Cyg Second-epoch detections are separated by 5.4" and 4.7 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 | 20:45:48.56 +53:45:55.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:45:48.56 +53:45:55.1: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:45:48.56 +53:45:55.1: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.35CV 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 06 20.4285 2461211.9285 14.29 20:42:10.48 +53:40:59.9
91.03248 7.03786 galactic Cyg Second-epoch detections are separated by 3.0" and 5.1 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 2183262894545105792 | 20:42:06.23 +53:41:27.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:42:10.48 +53:40:59.9: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:42:10.48 +53:40:59.9: 15.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2183262894545105792,2461211.9285,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2183262894545105792 20260620.4285 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.03 21:34:03.64 +55:19:03.4
97.32950 2.58038 galactic Cyg Second-epoch detections are separated by 4.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:03.64 +55:19:03.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:34:03.64 +55:19:03.4: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:34:03.64 +55:19:03.4: 15.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.85 21:25:55.47 +51:51:35.0
94.07845 0.89133 galactic Cyg Second-epoch detections are separated by 5.1" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.4889+51.8688 | 21:25:55.47 +51:51:35.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:25:55.47 +51:51:35.0: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:25:55.47 +51:51:35.0: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J321.4889+51.8688,2461211.9285,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J321.4889+51.8688 20260620.4285 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.44 20:41:45.44 +57:14:15.4
93.85653 9.23377 galactic Cep Second-epoch detections are separated by 5.1" and 4.7 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 | 20:41:45.44 +57:14:15.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:41:45.44 +57:14:15.4: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:41:45.44 +57:14:15.4: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.13 20:47:48.00 +49:59:53.4
88.65798 4.07988 galactic Cyg Second-epoch detections are separated by 3.4" and 5.1 pix
The object was found in VSX18" Gaia DR3 2168352005048671488
Type: S
# Max. Min./Amp. JD0 Period
16.070 G 16.590 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:47:48.00 +49:59:53.4: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:47:48.00 +49:59:53.4: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168352005048671488,2461211.9285,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168352005048671488 20260620.4285 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.03 21:10:27.31 +56:35:47.1
95.88878 5.81698 galactic Cep Second-epoch detections are separated by 5.8" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:10:27.31 +56:35:47.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:10:27.31 +56:35:47.1: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:10:27.31 +56:35:47.1: 15.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.10 20:43:14.80 +54:35:24.9
91.85425 7.46523 galactic Cyg Second-epoch detections are separated by 8.7" and 4.6 pix
The object was found in VSX22" Gaia DR3 2183329376337420672
Type: S
# Max. Min./Amp. JD0 Period
17.470 G 18.230 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:14.80 +54:35:24.9: 15.34 +/- 0.32 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:14.80 +54:35:24.9: 15.52 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.34 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2183329376337420672,2461211.9285,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2183329376337420672 20260620.4285 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.82 21:41:34.07 +57:47:39.9
99.75503 3.73707 galactic Cep Second-epoch detections are separated by 5.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4019+57.7889 | 21:41:34.07 +57:47:39.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:34.07 +57:47:39.9: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:34.07 +57:47:39.9: 15.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.4019+57.7889,2461211.9285,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.4019+57.7889 20260620.4285 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.74 21:37:28.07 +52:54:40.7
96.08420 0.46145 galactic Cyg Second-epoch detections are separated by 4.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.3788+52.9186 | 21:37:28.07 +52:54:40.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:28.07 +52:54:40.7: 15.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:28.07 +52:54:40.7: 15.20 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.3788+52.9186,2461211.9285,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.3788+52.9186 20260620.4285 13.74CV 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 06 20.4285 2461211.9285 13.97 20:49:09.56 +54:26:00.7
92.26381 6.69341 galactic Cyg Second-epoch detections are separated by 3.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.2987+54.4285 | 20:49:09.56 +54:26:00.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:49:09.56 +54:26:00.7: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:49:09.56 +54:26:00.7: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J312.2987+54.4285,2461211.9285,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J312.2987+54.4285 20260620.4285 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.08 20:47:43.46 +56:36:18.9
93.85173 8.20292 galactic Cep Second-epoch detections are separated by 6.1" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.9222+56.6059 | 20:47:43.46 +56:36:18.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:47:43.46 +56:36:18.9: 15.11 +/- 0.22 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:47:43.46 +56:36:18.9: 15.57 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.9222+56.6059,2461211.9285,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.9222+56.6059 20260620.4285 14.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.65 21:37:12.39 +52:31:38.5
95.79868 0.20172 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.2879+52.5315 | 21:37:12.39 +52:31:38.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:12.39 +52:31:38.5: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:12.39 +52:31:38.5: 15.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.2879+52.5315,2461211.9285,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.2879+52.5315 20260620.4285 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.69 21:40:14.50 +53:44:30.6
96.94492 0.80867 galactic Cyg Second-epoch detections are separated by 2.1" and 4.7 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 | 21:40:14.50 +53:44:30.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:14.50 +53:44:30.6: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:14.50 +53:44:30.6: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.86 21:00:31.36 +55:52:32.7
94.42417 6.36708 galactic Cep Second-epoch detections are separated by 4.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:31.36 +55:52:32.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:00:31.36 +55:52:32.7: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:00:31.36 +55:52:32.7: 15.74 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.78 21:28:12.72 +50:38:59.3
93.49866 -0.22930 galactic Cyg Second-epoch detections are separated by 7.8" and 4.7 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 J322.0577+50.6564 | 21:28:12.72 +50:38:59.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:28:12.72 +50:38:59.3: 14.77 +/- 0.17 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:28:12.72 +50:38:59.3: 14.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J322.0577+50.6564,2461211.9285,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.0577+50.6564 20260620.4285 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.73 21:36:44.66 +55:43:08.2
97.88108 2.62199 galactic Cep Second-epoch detections are separated by 4.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:44.66 +55:43:08.2 (user input) | T | P | (position from user input) J-Ks=0.913+/-0.108 (M)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:36:44.66 +55:43:08.2: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:36:44.66 +55:43:08.2: 15.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.59 21:41:17.12 +57:21:52.3
99.44324 3.43806 galactic Cep Second-epoch detections are separated by 4.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:17.12 +57:21:52.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:17.12 +57:21:52.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:17.12 +57:21:52.3: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.81 20:51:43.68 +53:51:01.1
92.04561 6.03415 galactic Cyg Second-epoch detections are separated by 3.5" and 4.8 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 | 20:51:43.68 +53:51:01.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:51:43.68 +53:51:01.1: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:51:43.68 +53:51:01.1: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.47 21:30:50.18 +49:40:27.8
93.13449 -1.22704 galactic Cyg Second-epoch detections are separated by 4.4" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:50.18 +49:40:27.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:30:50.18 +49:40:27.8: 14.59 +/- 0.16 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:30:50.18 +49:40:27.8: 14.52 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.47CV 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 06 20.4285 2461211.9285 13.48 21:31:36.22 +55:52:52.6
97.45776 3.22979 galactic Cep Second-epoch detections are separated by 6.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.9056+55.8718 | 21:31:36.22 +55:52:52.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:31:36.22 +55:52:52.6: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:31:36.22 +55:52:52.6: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J322.9056+55.8718,2461211.9285,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.9056+55.8718 20260620.4285 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.79 20:45:29.19 +54:37:54.7
92.08763 7.23433 galactic Cyg Second-epoch detections are separated by 3.2" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:45:29.19 +54:37:54.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:45:29.19 +54:37:54.7: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:45:29.19 +54:37:54.7: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.48 21:05:22.56 +54:01:53.9
93.49521 4.62613 galactic Cyg Second-epoch detections are separated by 5.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:05:22.56 +54:01:53.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:05:22.56 +54:01:53.9: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:05:22.56 +54:01:53.9: 15.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.54 20:47:42.43 +53:46:00.7
91.60562 6.44399 galactic Cyg Second-epoch detections are separated by 4.3" and 4.7 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 J311.9431+53.7691 | 20:47:42.43 +53:46:00.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:47:42.43 +53:46:00.7: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:47:42.43 +53:46:00.7: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.9431+53.7691,2461211.9285,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.9431+53.7691 20260620.4285 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.32 21:34:10.99 +51:07:14.8
94.50846 -0.52767 galactic Cyg Second-epoch detections are separated by 5.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.5592+51.1288 | 21:34:10.99 +51:07:14.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:34:10.99 +51:07:14.8: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:34:10.99 +51:07:14.8: 15.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J323.5592+51.1288,2461211.9285,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.5592+51.1288 20260620.4285 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.49 20:55:02.11 +54:56:37.9
93.20224 6.35864 galactic Cyg Second-epoch detections are separated by 6.3" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:02.11 +54:56:37.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:55:02.11 +54:56:37.9: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:55:02.11 +54:56:37.9: 15.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.06 21:35:32.19 +53:42:41.3
96.40519 1.24915 galactic Cyg Second-epoch detections are separated by 3.1" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:32.19 +53:42:41.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:32.19 +53:42:41.3: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:32.19 +53:42:41.3: 15.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 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 06 20.4285 2461211.9285 13.10 21:37:28.32 +55:01:48.3
97.49755 2.04030 galactic Cyg Second-epoch detections are separated by 4.2" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:28.32 +55:01:48.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:28.32 +55:01:48.3: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:28.32 +55:01:48.3: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 12.91 21:40:33.19 +53:58:50.4
97.13687 0.95805 galactic Cyg Second-epoch detections are separated by 3.3" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1552+53.9728 | 21:40:36.54 +53:59:05.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:33.19 +53:58:50.4: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:33.19 +53:58:50.4: 15.40 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.1552+53.9728,2461211.9285,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.1552+53.9728 20260620.4285 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 06 20.4285 2461211.9285 12.76 21:41:26.28 +57:15:39.7
99.39063 3.34652 galactic Cep Second-epoch detections are separated by 4.8" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:26.28 +57:15:39.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:26.28 +57:15:39.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:26.28 +57:15:39.7: 15.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 12.78 21:03:28.30 +56:47:41.6
95.39203 6.66224 galactic Cep Second-epoch detections are separated by 4.7" and 4.5 pix
The object was found in VSX15" Gaia DR3 2189598658499851520
Type: ROT
# Max. Min./Amp. JD0 Period
15.910 G 15.940 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:03:28.30 +56:47:41.6: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:03:28.30 +56:47:41.6: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2189598658499851520,2461211.9285,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2189598658499851520 20260620.4285 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 06 20.4285 2461211.9285 12.36 21:34:57.10 +55:05:43.9
97.27344 2.33070 galactic Cyg Second-epoch detections are separated by 3.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:57.10 +55:05:43.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:34:57.10 +55:05:43.9: 15.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:34:57.10 +55:05:43.9: 15.30 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 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 06 20.4285 2461211.9285 12.22 21:38:40.69 +53:42:12.9
96.74613 0.93295 galactic Cyg Second-epoch detections are separated by 2.8" and 4.8 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 J324.6749+53.6963 | 21:38:40.69 +53:42:12.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:40.69 +53:42:12.9: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:40.69 +53:42:12.9: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.6749+53.6963,2461211.9285,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.6749+53.6963 20260620.4285 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 06 20.4285 2461211.9285 12.02 21:35:48.50 +53:28:05.9
96.27184 1.04183 galactic Cyg Second-epoch detections are separated by 1.7" and 4.6 pix
The object was found in VSX21" ZTF J213547.97+532825.8
Type: SR
# Max. Min./Amp. JD0 Period
16.306 r Y 0.127 r 2458337.99100 28.203135000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:48.50 +53:28:05.9: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:48.50 +53:28:05.9: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J213547.97+532825.8,2461211.9285,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J213547.97+532825.8 20260620.4285 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 11.62 21:39:01.38 +56:54:02.1
98.90539 3.29257 galactic Cep Second-epoch detections are separated by 4.5" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.7651+56.8957 | 21:39:01.38 +56:54:02.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:01.38 +56:54:02.1: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:01.38 +56:54:02.1: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.7651+56.8957,2461211.9285,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.7651+56.8957 20260620.4285 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 11.77 21:40:14.46 +54:14:13.0
97.27137 1.18095 galactic Cyg Second-epoch detections are separated by 7.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2174333893752274432 | 21:40:10.88 +54:14:27.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:14.46 +54:14:13.0: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:14.46 +54:14:13.0: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2174333893752274432,2461211.9285,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2174333893752274432 20260620.4285 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 06 20.4285 2461211.9285 12.19 20:44:09.08 +55:47:28.0
92.89439 8.09506 galactic Cep Second-epoch detections are separated by 5.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:09.08 +55:47:28.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:44:09.08 +55:47:28.0: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:44:09.08 +55:47:28.0: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 12.26 20:54:07.45 +57:07:51.8
94.81889 7.85082 galactic Cep Second-epoch detections are separated by 5.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:07.45 +57:07:51.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:54:07.45 +57:07:51.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:54:07.45 +57:07:51.8: 15.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 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 06 20.4285 2461211.9285 12.47 20:44:10.58 +55:47:53.1
92.90213 8.09653 galactic Cep Second-epoch detections are separated by 5.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:10.58 +55:47:53.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:44:10.58 +55:47:53.1: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:44:10.58 +55:47:53.1: 15.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 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 06 20.4285 2461211.9285 12.68 20:50:07.38 +56:46:24.1
94.19151 8.04938 galactic Cep Second-epoch detections are separated by 5.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.5387+56.7851 | 20:50:07.38 +56:46:24.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:50:07.38 +56:46:24.1: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:50:07.38 +56:46:24.1: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J312.5387+56.7851,2461211.9285,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J312.5387+56.7851 20260620.4285 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 12.37 21:32:49.84 +51:49:55.0
94.83455 0.13849 galactic Cyg Second-epoch detections are separated by 6.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.2217+51.8320 | 21:32:49.84 +51:49:55.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:32:49.84 +51:49:55.0: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:32:49.84 +51:49:55.0: 15.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J323.2217+51.8320,2461211.9285,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.2217+51.8320 20260620.4285 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 06 20.4285 2461211.9285 12.60 21:40:16.97 +53:54:37.5
97.06065 0.93141 galactic Cyg Second-epoch detections are separated by 3.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0646+53.9074 | 21:40:16.97 +53:54:37.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:16.97 +53:54:37.5: 15.09 +/- 0.26 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:16.97 +53:54:37.5: 15.47 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.09 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.0646+53.9074,2461211.9285,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.0646+53.9074 20260620.4285 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 06 20.4285 2461211.9285 12.85 20:49:02.95 +54:34:53.1
92.37000 6.79832 galactic Cyg Second-epoch detections are separated by 3.6" and 4.8 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 J312.2691+54.5878 | 20:49:02.95 +54:34:53.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:49:02.95 +54:34:53.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:49:02.95 +54:34:53.1: 15.40 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J312.2691+54.5878,2461211.9285,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J312.2691+54.5878 20260620.4285 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 06 20.4285 2461211.9285 13.04 21:01:39.26 +57:43:29.9
95.93601 7.45848 galactic Cep Second-epoch detections are separated by 5.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:01:39.26 +57:43:29.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:01:39.26 +57:43:29.9: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:01:39.26 +57:43:29.9: 15.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 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 06 20.4285 2461211.9285 13.24 20:42:11.44 +54:10:24.0
91.42624 7.33367 galactic Cyg Second-epoch detections are separated by 4.3" and 4.8 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 | 20:42:11.44 +54:10:24.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:42:11.44 +54:10:24.0: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:42:11.44 +54:10:24.0: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.03 21:33:53.98 +49:34:20.1
93.42908 -1.63915 galactic Cyg Second-epoch detections are separated by 4.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.5039+49.5758 | 21:33:57.97 +49:34:44.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:33:53.98 +49:34:20.1: 13.95 +/- 0.11 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:33:53.98 +49:34:20.1: 14.34 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J323.5039+49.5758,2461211.9285,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.5039+49.5758 20260620.4285 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 06 20.4285 2461211.9285 13.39 20:52:42.71 +57:09:44.3
94.72093 8.01890 galactic Cep Second-epoch detections are separated by 5.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:52:42.71 +57:09:44.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:52:42.71 +57:09:44.3: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:52:42.71 +57:09:44.3: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.51 21:01:36.62 +57:43:17.8
95.92957 7.46072 galactic Cep Second-epoch detections are separated by 6.8" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.3795+57.7208 | 21:01:36.62 +57:43:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:01:36.62 +57:43:17.8: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:01:36.62 +57:43:17.8: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J315.3795+57.7208,2461211.9285,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J315.3795+57.7208 20260620.4285 13.51CV 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 06 20.4285 2461211.9285 13.22 21:34:59.04 +55:36:39.3
97.62430 2.70856 galactic Cep Second-epoch detections are separated by 5.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:59.04 +55:36:39.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:34:59.04 +55:36:39.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:34:59.04 +55:36:39.3: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.22CV 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 06 20.4285 2461211.9285 13.56 20:54:29.12 +57:36:37.1
95.22400 8.11746 galactic Cep Second-epoch detections are separated by 6.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.6395+57.6156 | 20:54:29.12 +57:36:37.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:54:29.12 +57:36:37.1: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:54:29.12 +57:36:37.1: 15.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J313.6395+57.6156,2461211.9285,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J313.6395+57.6156 20260620.4285 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.67 20:48:12.23 +55:48:05.4
93.25648 7.65257 galactic Cep Second-epoch detections are separated by 8.6" and 5.7 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 | 20:48:12.23 +55:48:05.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:48:12.23 +55:48:05.4: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:48:12.23 +55:48:05.4: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.86 21:12:52.25 +56:22:35.3
95.95524 5.42304 galactic Cep Second-epoch detections are separated by 6.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.2214+56.3816 | 21:12:52.25 +56:22:35.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:12:52.25 +56:22:35.3: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:12:52.25 +56:22:35.3: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J318.2214+56.3816,2461211.9285,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J318.2214+56.3816 20260620.4285 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.09 20:43:40.80 +54:05:52.8
91.49998 7.11479 galactic Cyg Second-epoch detections are separated by 5.4" and 4.8 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 | 20:43:40.80 +54:05:52.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:40.80 +54:05:52.8: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:40.80 +54:05:52.8: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.98 21:01:45.07 +57:43:15.3
95.94144 7.44604 galactic Cep Second-epoch detections are separated by 3.8" and 4.7 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 2189698817138924800 | 21:01:49.68 +57:43:10.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A8 1958TrRig...7...33A Cl Trumpler 37 546
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:01:45.07 +57:43:15.3: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:01:45.07 +57:43:15.3: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2189698817138924800,2461211.9285,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2189698817138924800 20260620.4285 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.14 20:40:58.80 +55:28:52.2
92.37133 8.26323 galactic Cep Second-epoch detections are separated by 5.7" and 4.7 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 J310.2346+55.4852 | 20:40:58.80 +55:28:52.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:40:58.80 +55:28:52.2: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:40:58.80 +55:28:52.2: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J310.2346+55.4852,2461211.9285,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J310.2346+55.4852 20260620.4285 14.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.88 21:40:12.38 +53:50:21.9
97.00535 0.88547 galactic Cyg Second-epoch detections are separated by 3.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:12.38 +53:50:21.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:12.38 +53:50:21.9: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:12.38 +53:50:21.9: 15.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.91 21:37:56.92 +49:49:27.9
94.08413 -1.89129 galactic Cyg Second-epoch detections are separated by 4.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1979110729472871424 | 21:37:54.54 +49:48:55.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:56.92 +49:49:27.9: 14.88 +/- 0.27 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:56.92 +49:49:27.9: 14.78 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1979110729472871424,2461211.9285,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1979110729472871424 20260620.4285 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.29 20:39:40.65 +56:25:44.7
93.02826 8.97732 galactic Cep Second-epoch detections are separated by 5.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:39:40.65 +56:25:44.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:39:40.65 +56:25:44.7: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:39:40.65 +56:25:44.7: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.22 20:41:31.86 +55:27:17.0
92.39757 8.18499 galactic Cep Second-epoch detections are separated by 3.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:31.86 +55:27:17.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:41:31.86 +55:27:17.0: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:41:31.86 +55:27:17.0: 15.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.22CV 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 06 20.4285 2461211.9285 14.18 20:57:24.43 +55:29:49.3
93.84745 6.45506 galactic Cep Second-epoch detections are separated by 3.8" and 4.7 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 J314.3394+55.5012 | 20:57:24.43 +55:29:49.3 (user input) | CBF (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:57:24.43 +55:29:49.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:57:24.43 +55:29:49.3: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J314.3394+55.5012,2461211.9285,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J314.3394+55.5012 20260620.4285 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.15 20:59:21.15 +49:49:50.4
89.72256 2.54468 galactic Cyg Second-epoch detections are separated by 6.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:21.15 +49:49:50.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:59:21.15 +49:49:50.4: 15.40 +/- 0.31 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:59:21.15 +49:49:50.4: 15.46 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.40 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.27 20:43:17.40 +53:43:39.8
91.16927 6.93403 galactic Cyg Second-epoch detections are separated by 6.7" and 5.6 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 | 20:43:17.40 +53:43:39.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:17.40 +53:43:39.8: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:17.40 +53:43:39.8: 15.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.27CV 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 06 20.4285 2461211.9285 14.24 20:42:33.19 +53:53:06.4
91.22816 7.11621 galactic Cyg Second-epoch detections are separated by 4.7" and 4.8 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 | 20:42:33.19 +53:53:06.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:42:33.19 +53:53:06.4: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:42:33.19 +53:53:06.4: 15.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.35 20:40:33.23 +57:27:26.2
93.93619 9.49536 galactic Cep Second-epoch detections are separated by 6.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:33.23 +57:27:26.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:40:33.23 +57:27:26.2: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:40:33.23 +57:27:26.2: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.35CV 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 06 20.4285 2461211.9285 14.04 21:37:03.49 +55:45:57.3
97.94539 2.62739 galactic Cep Second-epoch detections are separated by 5.4" and 4.1 pix
The object was found in VSX22" Gaia DR3 2177673458474154496
Type: ROT
# Max. Min./Amp. JD0 Period
15.650 G 15.690 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:03.49 +55:45:57.3: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:03.49 +55:45:57.3: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2177673458474154496,2461211.9285,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2177673458474154496 20260620.4285 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.20 20:47:50.67 +54:01:23.2
91.82019 6.58760 galactic Cyg Second-epoch detections are separated by 2.6" and 5.1 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 J311.9725+54.0204 | 20:47:50.67 +54:01:23.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:47:50.67 +54:01:23.2: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:47:50.67 +54:01:23.2: 15.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.9725+54.0204,2461211.9285,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.9725+54.0204 20260620.4285 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.81 21:37:58.28 +50:06:43.9
94.27847 -1.67893 galactic Cyg Second-epoch detections are separated by 4.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.4865+50.1182 | 21:37:58.28 +50:06:43.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:58.28 +50:06:43.9: 15.04 +/- 0.27 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:58.28 +50:06:43.9: 15.09 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.4865+50.1182,2461211.9285,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.4865+50.1182 20260620.4285 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.30 20:41:55.03 +54:15:24.5
91.46869 7.41610 galactic Cyg Second-epoch detections are separated by 5.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:55.03 +54:15:24.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:41:55.03 +54:15:24.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:41:55.03 +54:15:24.5: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.29 21:10:24.96 +57:40:50.1
96.68729 6.55538 galactic Cep Second-epoch detections are separated by 6.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:10:24.96 +57:40:50.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:10:24.96 +57:40:50.1: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:10:24.96 +57:40:50.1: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.15 21:17:50.06 +51:34:25.9
92.98820 1.57228 galactic Cyg Second-epoch detections are separated by 7.2" and 5.1 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 2172261421717706240 | 21:17:47.47 +51:34:53.7 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:17:50.06 +51:34:25.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:17:50.06 +51:34:25.9: 15.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2172261421717706240,2461211.9285,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2172261421717706240 20260620.4285 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.43 20:40:46.42 +57:06:56.9
93.67678 9.26737 galactic Cep Second-epoch detections are separated by 7.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:46.42 +57:06:56.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:40:46.42 +57:06:56.9: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:40:46.42 +57:06:56.9: 15.59 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.47 20:54:10.99 +57:58:40.4
95.48533 8.38175 galactic Cep Second-epoch detections are separated by 4.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.5494+57.9676 | 20:54:10.99 +57:58:40.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:54:10.99 +57:58:40.4: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:54:10.99 +57:58:40.4: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J313.5494+57.9676,2461211.9285,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J313.5494+57.9676 20260620.4285 14.47CV 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 06 20.4285 2461211.9285 14.43 20:48:50.36 +54:57:05.4
92.64223 7.05297 galactic Cyg Second-epoch detections are separated by 7.9" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:50.36 +54:57:05.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:48:50.36 +54:57:05.4: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:48:50.36 +54:57:05.4: 15.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.35 20:44:14.80 +51:12:14.1
89.25464 5.27070 galactic Cyg Second-epoch detections are separated by 7.7" and 5.1 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 J311.0606+51.1956 | 20:44:14.80 +51:12:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:44:14.80 +51:12:14.1: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:44:14.80 +51:12:14.1: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.0606+51.1956,2461211.9285,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.0606+51.1956 20260620.4285 14.35CV 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 06 20.4285 2461211.9285 14.11 21:37:04.77 +54:27:27.8
97.07319 1.65182 galactic Cyg Second-epoch detections are separated by 6.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:04.77 +54:27:27.8 (user input) | T | P | (position from user input) J-Ks=0.619+/-0.060 (K)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:04.77 +54:27:27.8: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:04.77 +54:27:27.8: 15.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.09 21:39:28.98 +55:45:40.8
98.19729 2.39714 galactic Cep Second-epoch detections are separated by 8.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:28.98 +55:45:40.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:28.98 +55:45:40.8: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:28.98 +55:45:40.8: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.18 20:50:08.35 +51:27:32.2
90.03084 4.71010 galactic Cyg Second-epoch detections are separated by 4.4" and 5.1 pix
The object was found in VSX17" Dauban V161
Type: M
# Max. Min./Amp. JD0 Period
17.942 g Y 3.645 g 2458310.80760 124.404956900000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:50:08.35 +51:27:32.2: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:50:08.35 +51:27:32.2: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Dauban V161,2461211.9285,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Dauban V161 20260620.4285 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.33 20:45:48.07 +54:31:17.5
92.02830 7.13047 galactic Cyg Second-epoch detections are separated by 3.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:45:48.07 +54:31:17.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:45:48.07 +54:31:17.5: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:45:48.07 +54:31:17.5: 15.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.06 21:38:31.39 +52:12:25.9
95.73565 -0.17101 galactic Cyg Second-epoch detections are separated by 8.3" and 4.7 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 J324.6178+52.1969 | 21:38:31.39 +52:12:25.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:31.39 +52:12:25.9: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:31.39 +52:12:25.9: 15.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.6178+52.1969,2461211.9285,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.6178+52.1969 20260620.4285 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.16 21:19:57.47 +54:31:30.9
95.31789 3.41502 galactic Cyg Second-epoch detections are separated by 4.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:19:57.47 +54:31:30.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:19:57.47 +54:31:30.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:19:57.47 +54:31:30.9: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.40 20:45:50.92 +50:43:17.4
89.03064 4.77415 galactic Cyg Second-epoch detections are separated by 8.1" and 5.3 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 J311.4583+50.7189 | 20:45:50.92 +50:43:17.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:45:50.92 +50:43:17.4: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:45:50.92 +50:43:17.4: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.4583+50.7189,2461211.9285,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.4583+50.7189 20260620.4285 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.27 20:54:06.71 +57:16:47.3
94.93388 7.94650 galactic Cep Second-epoch detections are separated by 3.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.5092+57.2794 | 20:54:06.71 +57:16:47.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:54:06.71 +57:16:47.3: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:54:06.71 +57:16:47.3: 15.41 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J313.5092+57.2794,2461211.9285,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J313.5092+57.2794 20260620.4285 14.27CV 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 06 20.4285 2461211.9285 14.46 20:44:18.87 +54:56:09.3
92.22523 7.55430 galactic Cyg Second-epoch detections are separated by 6.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.0964+54.9336 | 20:44:18.87 +54:56:09.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:44:18.87 +54:56:09.3: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:44:18.87 +54:56:09.3: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.0964+54.9336,2461211.9285,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.0964+54.9336 20260620.4285 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.09 21:39:34.42 +54:12:55.4
97.18387 1.22917 galactic Cyg Second-epoch detections are separated by 5.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:34.42 +54:12:55.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:34.42 +54:12:55.4: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:34.42 +54:12:55.4: 15.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.39 20:59:29.56 +56:44:47.1
94.99569 7.04257 galactic Cep Second-epoch detections are separated by 5.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:29.56 +56:44:47.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:59:29.56 +56:44:47.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:59:29.56 +56:44:47.1: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.32 20:43:56.36 +51:57:21.7
89.82076 5.77112 galactic Cyg Second-epoch detections are separated by 4.7" and 4.7 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 J310.9843+51.9612 | 20:43:56.36 +51:57:21.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:56.36 +51:57:21.7: 15.28 +/- 0.31 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:56.36 +51:57:21.7: 15.39 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J310.9843+51.9612,2461211.9285,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J310.9843+51.9612 20260620.4285 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.50 20:43:13.08 +56:20:13.3
93.25220 8.53053 galactic Cep Second-epoch detections are separated by 6.2" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:43:13.08 +56:20:13.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:13.08 +56:20:13.3: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:13.08 +56:20:13.3: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.50CV 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 06 20.4285 2461211.9285 14.50 20:43:11.75 +53:44:06.3
91.16658 6.94956 galactic Cyg Second-epoch detections are separated by 8.6" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J310.8010+53.7488 | 20:43:12.28 +53:44:44.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:11.75 +53:44:06.3: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:11.75 +53:44:06.3: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J310.8010+53.7488,2461211.9285,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J310.8010+53.7488 20260620.4285 14.50CV 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 06 20.4285 2461211.9285 14.62 20:52:14.53 +57:50:51.6
95.21875 8.49952 galactic Cep Second-epoch detections are separated by 6.9" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:52:14.53 +57:50:51.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:52:14.53 +57:50:51.6: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:52:14.53 +57:50:51.6: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.51 21:11:15.35 +57:22:19.0
96.53595 6.26324 galactic Cep Second-epoch detections are separated by 3.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:11:15.35 +57:22:19.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:11:15.35 +57:22:19.0: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:11:15.35 +57:22:19.0: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.51CV 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 06 20.4285 2461211.9285 14.51 20:38:50.94 +56:09:23.5
92.73735 8.90721 galactic Cyg Second-epoch detections are separated by 4.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:38:50.94 +56:09:23.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:38:50.94 +56:09:23.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:38:50.94 +56:09:23.5: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.51CV 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 06 20.4285 2461211.9285 14.48 20:45:35.17 +54:49:34.2
92.25098 7.34254 galactic Cyg Second-epoch detections are separated by 2.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.4110+54.8405 | 20:45:38.36 +54:49:41.8 (Gaia DR3) | CBF (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:45:35.17 +54:49:34.2: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:45:35.17 +54:49:34.2: 15.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.4110+54.8405,2461211.9285,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.4110+54.8405 20260620.4285 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.52 21:02:25.19 +57:15:09.4
95.64423 7.07127 galactic Cep Second-epoch detections are separated by 7.7" and 4.0 pix
The object was found in VSX 6" Gaia DR3 2189668340050717952
Type: S
# Max. Min./Amp. JD0 Period
16.890 G 17.790 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:02:25.19 +57:15:09.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:02:25.19 +57:15:09.4: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2189668340050717952,2461211.9285,14.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2189668340050717952 20260620.4285 14.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.36 21:41:11.83 +57:32:12.9
99.54793 3.57568 galactic Cep Second-epoch detections are separated by 5.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2903+57.5411 | 21:41:11.83 +57:32:12.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:11.83 +57:32:12.9: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:11.83 +57:32:12.9: 15.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.2903+57.5411,2461211.9285,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J325.2903+57.5411 20260620.4285 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.43 20:49:49.16 +54:17:47.6
92.21690 6.53269 galactic Cyg Second-epoch detections are separated by 3.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:49.16 +54:17:47.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:49:49.16 +54:17:47.6: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:49:49.16 +54:17:47.6: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.22 21:41:59.97 +56:24:24.7
98.88726 2.65168 galactic Cep Second-epoch detections are separated by 4.4" and 4.2 pix
The object was found in VSX13" Gaia DR3 2178091101091156864
Type: ROT
# Max. Min./Amp. JD0 Period
14.590 G 14.630 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:59.97 +56:24:24.7: 15.04 +/- 0.21 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:59.97 +56:24:24.7: 15.38 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2178091101091156864,2461211.9285,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2178091101091156864 20260620.4285 14.22CV 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 06 20.4285 2461211.9285 14.38 21:26:53.83 +56:11:51.2
97.19836 3.91171 galactic Cep Second-epoch detections are separated by 4.3" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:26:53.83 +56:11:51.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:26:53.83 +56:11:51.2: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:26:53.83 +56:11:51.2: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.57 20:42:49.38 +51:03:20.7
88.99941 5.35590 galactic Cyg Second-epoch detections are separated by 5.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J310.6950+51.0545 | 20:42:49.38 +51:03:20.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:42:49.38 +51:03:20.7: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:42:49.38 +51:03:20.7: 15.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J310.6950+51.0545,2461211.9285,14.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J310.6950+51.0545 20260620.4285 14.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.32 21:38:30.40 +56:01:58.5
98.27505 2.69117 galactic Cep Second-epoch detections are separated by 2.5" and 4.7 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 J324.6040+56.0315 | 21:38:30.40 +56:01:58.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:30.40 +56:01:58.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:30.40 +56:01:58.5: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.6040+56.0315,2461211.9285,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.6040+56.0315 20260620.4285 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.34 21:41:58.71 +57:00:58.7
99.28511 3.11379 galactic Cep Second-epoch detections are separated by 1.8" and 4.8 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 | 21:41:58.71 +57:00:58.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:58.71 +57:00:58.7: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:58.71 +57:00:58.7: 15.58 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.49 20:45:34.99 +50:55:55.9
89.17042 4.93771 galactic Cyg Second-epoch detections are separated by 7.0" and 5.3 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 J311.3970+50.9337 | 20:45:34.99 +50:55:55.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:45:34.99 +50:55:55.9: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:45:34.99 +50:55:55.9: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.3970+50.9337,2461211.9285,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.3970+50.9337 20260620.4285 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.39 20:48:31.64 +49:50:50.8
88.61389 3.89417 galactic Cyg Second-epoch detections are separated by 6.5" and 5.1 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 J312.1266+49.8517 | 20:48:28.48 +49:51:14.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.224+/- (M)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:48:31.64 +49:50:50.8: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:48:31.64 +49:50:50.8: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J312.1266+49.8517,2461211.9285,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J312.1266+49.8517 20260620.4285 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.67 20:55:57.40 +57:25:58.7
95.21305 7.85224 galactic Cep Second-epoch detections are separated by 8.3" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:57.40 +57:25:58.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:55:57.40 +57:25:58.7: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:55:57.40 +57:25:58.7: 15.68 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.24 21:38:09.72 +56:40:15.8
98.66436 3.19944 galactic Cep Second-epoch detections are separated by 5.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:38:09.72 +56:40:15.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:09.72 +56:40:15.8: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:09.72 +56:40:15.8: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.43 21:39:19.93 +53:34:33.7
96.73421 0.77319 galactic Cyg Second-epoch detections are separated by 6.7" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:19.93 +53:34:33.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:19.93 +53:34:33.7: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:19.93 +53:34:33.7: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.28 21:30:41.43 +54:20:47.2
96.31242 2.19833 galactic Cyg Second-epoch detections are separated by 5.8" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:41.43 +54:20:47.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:30:41.43 +54:20:47.2: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:30:41.43 +54:20:47.2: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.32 21:42:00.41 +56:03:58.6
98.66462 2.39375 galactic Cep Second-epoch detections are separated by 5.1" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:00.41 +56:03:58.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:42:00.41 +56:03:58.6: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:42:00.41 +56:03:58.6: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.52 20:43:56.34 +52:07:36.0
89.95606 5.87601 galactic Cyg Second-epoch detections are separated by 7.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:43:56.34 +52:07:36.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:43:56.34 +52:07:36.0: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:43:56.34 +52:07:36.0: 15.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.41 21:41:49.15 +57:27:48.5
99.56266 3.46542 galactic Cep Second-epoch detections are separated by 5.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:49.15 +57:27:48.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:49.15 +57:27:48.5: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:49.15 +57:27:48.5: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.47 21:40:43.97 +56:06:27.2
98.55766 2.54161 galactic Cep Second-epoch detections are separated by 8.5" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:43.97 +56:06:27.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:43.97 +56:06:27.2: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:43.97 +56:06:27.2: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.47CV 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 06 20.4285 2461211.9285 14.41 21:30:52.64 +55:04:37.4
96.83234 2.71282 galactic Cyg Second-epoch detections are separated by 6.4" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:52.64 +55:04:37.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:30:52.64 +55:04:37.4: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:30:52.64 +55:04:37.4: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.51 20:50:37.09 +51:04:23.8
89.77838 4.40841 galactic Cyg Second-epoch detections are separated by 5.2" and 4.8 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 | 20:50:37.09 +51:04:23.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:50:37.09 +51:04:23.8: 15.49 +/- 0.32 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:50:37.09 +51:04:23.8: 15.57 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.49 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.51CV 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 06 20.4285 2461211.9285 14.56 20:54:05.86 +50:31:45.1
89.70901 3.63804 galactic Cyg Second-epoch detections are separated by 6.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:05.86 +50:31:45.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:54:05.86 +50:31:45.1: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:54:05.86 +50:31:45.1: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.29 21:37:20.87 +50:45:30.8
94.63514 -1.13074 galactic Cyg Second-epoch detections are separated by 3.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:20.87 +50:45:30.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:37:20.87 +50:45:30.8: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:37:20.87 +50:45:30.8: 15.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.31 21:35:45.80 +50:08:17.4
94.03247 -1.42311 galactic Cyg Second-epoch detections are separated by 5.4" and 4.8 pix
The object was found in VSX22" Gaia DR3 1979180067427326720
Type: VAR
# Max. Min./Amp. JD0 Period
14.640 G 14.750 G 0.017542800000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:45.80 +50:08:17.4: 15.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:45.80 +50:08:17.4: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979180067427326720,2461211.9285,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979180067427326720 20260620.4285 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.57 20:45:22.70 +49:38:30.2
88.13443 4.16318 galactic Cyg Second-epoch detections are separated by 7.1" and 5.3 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 J311.3389+49.6353 | 20:45:22.70 +49:38:30.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:45:22.70 +49:38:30.2: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:45:22.70 +49:38:30.2: 15.37 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J311.3389+49.6353,2461211.9285,14.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J311.3389+49.6353 20260620.4285 14.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.48 21:41:13.24 +56:41:17.9
98.99118 2.93444 galactic Cep Second-epoch detections are separated by 2.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:13.24 +56:41:17.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:13.24 +56:41:17.9: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:13.24 +56:41:17.9: 15.43 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.43 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.46 21:39:28.98 +54:00:15.8
97.03434 1.07968 galactic Cyg Second-epoch detections are separated by 3.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:28.98 +54:00:15.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:39:28.98 +54:00:15.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:39:28.98 +54:00:15.8: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.41 21:35:44.23 +50:54:20.2
94.54446 -0.85131 galactic Cyg Second-epoch detections are separated by 4.2" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J323.9353+50.8947 | 21:35:44.23 +50:54:20.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: PN 1972A&A....16..291K PN K 3-83
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:44.23 +50:54:20.2: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:44.23 +50:54:20.2: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J323.9353+50.8947,2461211.9285,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J323.9353+50.8947 20260620.4285 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.50 21:13:15.26 +56:37:38.0
96.17522 5.55619 galactic Cep Second-epoch detections are separated by 4.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:13:15.26 +56:37:38.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:13:15.26 +56:37:38.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:13:15.26 +56:37:38.0: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.50CV 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 06 20.4285 2461211.9285 14.52 20:58:22.98 +50:33:49.9
90.17664 3.14131 galactic Cyg Second-epoch detections are separated by 5.7" and 4.7 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 J314.5960+50.5712 | 20:58:22.98 +50:33:49.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:58:22.98 +50:33:49.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:58:22.98 +50:33:49.9: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J314.5960+50.5712,2461211.9285,14.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J314.5960+50.5712 20260620.4285 14.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.61 20:47:08.15 +49:51:02.7
88.47564 4.07110 galactic Cyg Second-epoch detections are separated by 5.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:47:08.15 +49:51:02.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:47:08.15 +49:51:02.7: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:47:08.15 +49:51:02.7: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.34 21:31:23.43 +49:50:50.4
93.31800 -1.16177 galactic Cyg Second-epoch detections are separated by 6.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.8480+49.8519 | 21:31:23.43 +49:50:50.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:31:23.43 +49:50:50.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:31:23.43 +49:50:50.4: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J322.8480+49.8519,2461211.9285,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.8480+49.8519 20260620.4285 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.69 21:24:31.95 +55:13:08.2
96.27536 3.44248 galactic Cyg Second-epoch detections are separated by 6.1" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:24:31.95 +55:13:08.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:24:31.95 +55:13:08.2: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:24:31.95 +55:13:08.2: 15.69 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.41 21:21:16.67 +53:23:52.0
94.65460 2.48223 galactic Cyg Second-epoch detections are separated by 4.3" and 4.7 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 J320.3185+53.3939 | 21:21:16.67 +53:23:52.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:21:16.67 +53:23:52.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:21:16.67 +53:23:52.0: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J320.3185+53.3939,2461211.9285,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J320.3185+53.3939 20260620.4285 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.34 21:40:57.14 +55:44:06.9
98.33553 2.24112 galactic Cep Second-epoch detections are separated by 4.1" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2175034493126155520 | 21:40:53.91 +55:44:26.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:40:57.14 +55:44:06.9: 15.24 +/- 0.27 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:40:57.14 +55:44:06.9: 15.47 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2175034493126155520,2461211.9285,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2175034493126155520 20260620.4285 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.55 21:41:28.83 +57:46:01.0
99.72814 3.72402 galactic Cep Second-epoch detections are separated by 5.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:28.83 +57:46:01.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:28.83 +57:46:01.0: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:28.83 +57:46:01.0: 15.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.61 21:41:46.40 +57:27:56.1
99.55939 3.47105 galactic Cep Second-epoch detections are separated by 6.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:46.40 +57:27:56.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:41:46.40 +57:27:56.1: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:41:46.40 +57:27:56.1: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.45 21:36:50.91 +53:59:43.1
96.73906 1.33027 galactic Cyg Second-epoch detections are separated by 7.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:50.91 +53:59:43.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:36:50.91 +53:59:43.1: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:36:50.91 +53:59:43.1: 15.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.46 21:29:48.10 +49:50:15.8
93.12453 -0.99358 galactic Cyg Second-epoch detections are separated by 7.4" and 5.4 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 | 21:29:48.10 +49:50:15.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:29:48.10 +49:50:15.8: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:29:48.10 +49:50:15.8: 15.41 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.31 21:38:45.74 +54:03:51.3
96.99471 1.19461 galactic Cyg Second-epoch detections are separated by 4.9" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.7067+54.0715 | 21:38:45.74 +54:03:51.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:45.74 +54:03:51.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:45.74 +54:03:51.3: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.7067+54.0715,2461211.9285,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J324.7067+54.0715 20260620.4285 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.49 21:30:11.85 +54:48:00.8
96.57135 2.57792 galactic Cyg Second-epoch detections are separated by 7.1" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:30:11.85 +54:48:00.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:30:11.85 +54:48:00.8: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:30:11.85 +54:48:00.8: 15.65 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.40 21:29:36.22 +51:19:25.2
94.12123 0.10900 galactic Cyg Second-epoch detections are separated by 4.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.3965+51.3283 | 21:29:36.22 +51:19:25.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:29:36.22 +51:19:25.2: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:29:36.22 +51:19:25.2: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J322.3965+51.3283,2461211.9285,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J322.3965+51.3283 20260620.4285 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.26 21:38:24.11 +50:09:53.6
94.36507 -1.68544 galactic Cyg Second-epoch detections are separated by 4.0" and 4.8 pix
The object was found in VSX16" Gaia DR3 1979169205446151424
Type: ROT
# Max. Min./Amp. JD0 Period
16.800 G 16.850 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:24.11 +50:09:53.6: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:24.11 +50:09:53.6: 15.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1979169205446151424,2461211.9285,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1979169205446151424 20260620.4285 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 14.44 21:38:01.31 +50:44:21.6
94.70187 -1.21609 galactic Cyg Second-epoch detections are separated by 1.3" and 4.8 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 | 21:38:01.31 +50:44:21.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:38:01.31 +50:44:21.6: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:38:01.31 +50:44:21.6: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461211.9285,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260620.4285 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.4285 2461211.9285 13.12 20:49:21.47 +50:31:43.3
89.22870 4.21924 galactic Cyg Second-epoch detections are separated by 5.1" and 4.8 pix
The object was found in VSX 8" V0750 Cyg
Type: M
# Max. Min./Amp. JD0 Period
11.200 V 16.400 V 2450201.00000 432.900000000000 M5ea
The object was not found in astcheck.
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:49:21.47 +50:31:43.3: 14.18 +/- 0.10 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:49:21.47 +50:31:43.3: 13.99 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.07 +/- 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
V0750 Cyg,2461211.9285,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0750 Cyg 20260620.4285 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461171.90353176 11.05.2026 09:40:55.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
First image: 2461171.90353176 11.05.2026 09:40:55.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Last image: 2461211.92878670 20.06.2026 10:17:17.171 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23466
Objects passed selection criteria: 23357
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 17514.2
Average stars matched: 15242.2 (87.0277 %)
Memory usage VmPeak: 125092 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 20 06:51:03 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461171.90353176 11.05.2026 09:40:55.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
First image: 2461171.90353176 11.05.2026 09:40:55.144 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Last image: 2461211.92878670 20.06.2026 10:17:17.171 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 479
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 227 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 166619
Objects passed selection criteria: 166042
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 129627
Average stars matched: 112896 (87.0927 %)
Memory usage VmPeak: 1933828 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 20 07:23:27 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.cat to cache
SExtractor catalog cache: saved Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.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/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.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: 2461211.92814424
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits'
wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits exists and is non-empty
Saving wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits to local_wcs_cache/
'wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits' -> 'local_wcs_cache/wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits'
wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits exists and is non-empty
Saving wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits to local_wcs_cache/
'wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits' -> 'local_wcs_cache/wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits (1st reference image)
verification OK: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Image size: 937.5'x624.1' 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: 21:10:39.370 +54:00:06.17 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_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits (1st new image)
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
Image size: 939.5'x622.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 21:10:35.552 +53:59:23.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:10:39.370 +54:00:06.17
Second-epoch image center 21:10:35.552 +53:59:23.23
Angular distance between the image centers 0.0152 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits (2nd new image)
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
Image size: 939.5'x622.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 21:10:32.706 +53:59:33.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:10:39.370 +54:00:06.17
Second-epoch image center 21:10:32.706 +53:59:33.83
Angular distance between the image centers 0.0186 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 21:10:35.552 +53:59:23.23
Second-epoch second image center 21:10:32.706 +53:59:33.83
Angular distance between the image centers 0.00757 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits &> /tmp/tmp.meJGAcDdS3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits &> /tmp/tmp.R5XTmAd1qu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits &> /tmp/tmp.BfWC5GvJDr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits &> /tmp/tmp.c1V7cITdGE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
Found non-empty wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits and wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
The reference image (wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits) and catalog (wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat) found
'wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat' -> 'wcsmag.cat'
Read 25074 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6809 to 332.6436 deg, Dec +48.1331 to +59.2551 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 302.6809 to 332.6436 deg, Dec 48.1331 to 59.2551 deg
Loaded 20051 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): 12364 out of 13307 total matches.
Matched with Tycho-2 13307 out of 25074 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.604000
a=0.000000 b=1.000000 c=22.604000
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 25074 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6809 to 332.6436 deg, Dec +48.1331 to +59.2551 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 302.6809 to 332.6436 deg, Dec 48.1331 to 59.2551 deg
Loaded 20051 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): 12364 out of 13307 total matches.
Matched with Tycho-2 13307 out of 25074 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits:
Forced-photometry filter: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits -> calib.txt_param_ref_wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits (aperture=6.5)
Read 23932 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 302.6813 to 332.6439 deg, Dec +48.1787 to +59.2616 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 302.6813 to 332.6439 deg, Dec 48.1787 to 59.2616 deg
Loaded 19971 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): 12294 out of 13147 total matches.
Matched with Tycho-2 13147 out of 23932 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits:
Forced-photometry filter: calibrated wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits -> calib.txt_param_ref_wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.6 pix Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
2.6 pix Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
2.4 pix fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
2.5 pix fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
2.6 pix wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
2.6 pix wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Limiting magnitude estimates:
14.9 mag. Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
14.8 mag. Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
14.9 mag. fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
14.8 mag. fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.meJGAcDdS3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits' -> 'wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2300, passed=25074
Got 25074 stars (including 22754 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat
util/solve_plate_with_UCAC5 got 25074 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 24212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits N_match=967 sigma_overall_arcsec=0.764 sigma_q1_arcsec=0.542 sigma_q2_arcsec=0.833 sigma_q3_arcsec=0.622 sigma_q4_arcsec=0.875 n_q1=190 n_q2=331 n_q3=174 n_q4=272 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits -region wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.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.R5XTmAd1qu (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits' -> 'wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS_IMAGE_NAME=wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS-calibrated image found: wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
Checking if the catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits alredy exist and is non-empty...
Catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat corresponding to the image wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits
WCS catalog name: wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2110, passed=23932
Got 23932 stars (including 21798 good ones) from the SExtractor catalog wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat
util/solve_plate_with_UCAC5 got 23932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 23180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 23180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 23180 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits N_match=967 sigma_overall_arcsec=0.770 sigma_q1_arcsec=0.579 sigma_q2_arcsec=0.827 sigma_q3_arcsec=0.679 sigma_q4_arcsec=0.930 n_q1=190 n_q2=327 n_q3=179 n_q4=271 worst_quadrant_to_overall_ratio=1.207
The image catalog is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits -region wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.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.BfWC5GvJDr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2819, passed=25248
Got 25248 stars (including 22396 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat
util/solve_plate_with_UCAC5 got 25248 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.5'
Seting catalog search parameters based on the expected field of view 939.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013049 (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 0.010439 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 320 matched stars entering correct_measured_positions(), 8754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.85"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 456 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 380 matched stars entering correct_measured_positions(), 8780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.79"
Accuracy estimation diagnostic: 374 matched stars entering correct_measured_positions(), 9542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.67"
Excluding outliers - 374 stars left (next iteration limit 352)
WCS_QUALITY_DIAG: file=fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits N_match=374 sigma_overall_arcsec=5.745 sigma_q1_arcsec=25.514 sigma_q2_arcsec=33.280 sigma_q3_arcsec=5.989 sigma_q4_arcsec=4.232 n_q1=28 n_q2=18 n_q3=151 n_q4=177 worst_quadrant_to_overall_ratio=5.793
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.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.c1V7cITdGE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
WCS-calibrated image found: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2796, passed=24993
Got 24993 stars (including 22170 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat
util/solve_plate_with_UCAC5 got 24993 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.5'
Seting catalog search parameters based on the expected field of view 939.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013049 (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 0.010439 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 386 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 317 matched stars entering correct_measured_positions(), 8210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 456 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 401 matched stars entering correct_measured_positions(), 8253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.84"
Accuracy estimation diagnostic: 397 matched stars entering correct_measured_positions(), 10262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.96"
Excluding outliers - 397 stars left (next iteration limit 348)
WCS_QUALITY_DIAG: file=fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits N_match=397 sigma_overall_arcsec=5.839 sigma_q1_arcsec=26.511 sigma_q2_arcsec=27.686 sigma_q3_arcsec=7.153 sigma_q4_arcsec=4.442 n_q1=28 n_q2=20 n_q3=165 n_q4=184 worst_quadrant_to_overall_ratio=4.742
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.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=Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits sigma_overall=0.764 worst_q_ratio=1.146
ref2=Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits sigma_overall=0.770 worst_q_ratio=1.207
new1=fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits sigma_overall=5.745 worst_q_ratio=5.793
new2=fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits sigma_overall=5.839 worst_q_ratio=4.742
reference average sigma_overall=0.767 worst_q_ratio=1.1765
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits) flagged: sigma=5.745 (ref avg 0.767), ratio=5.793 (ref avg 1.1765), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/lib/make_outxyls_for_astrometric_calibration found 23973 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out3835881.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3835881.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
log-odds ratio 36.2694 (5.64425e+15), 27 match, 0 conflict, 80 distractors, 186 index.
RA,Dec = (317.708,54.0404), pixel scale 5.90979 arcsec/pix.
Hit/miss: Hit/miss: -++--+++------------++---++---+----------++--+++-------------++--++---+---------++--------+---------
Field 1: solved with index index-4113.fits.
Field 1 solved: writing to file ./out3835881.solved to indicate this.
Field: out3835881.xyls
Field center: (RA,Dec) = (317.648646, 54.014236) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:10:35.675, +54:00:51.251).
Field size: 15.7319 x 10.5338 degrees
Field rotation angle: up is -179.25 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits' -> 'fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jun 20 07:02 fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
-rw-r--r-- 1 apache apache 12K Jun 20 07:02 out3835881.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits for reading... done!
Creating new image file (wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits (fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out3835881.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3835881.axy"...
Only searching for solutions within 15.6667 degrees of RA,Dec (317.647,54.0134)
log-odds ratio 60.6119 (2.10571e+26), 8 match, 0 conflict, 11 distractors, 23 index.
RA,Dec = (317.662,53.9909), pixel scale 5.93476 arcsec/pix.
Hit/miss: Hit/miss: +--+-+---+--+++---+(best)---------------------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out3835881.solved to indicate this.
Field: out3835881.xyls
Field center: (RA,Dec) = (317.649558, 53.990597) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:10:35.894, +53:59:26.149).
Field size: 15.7237 x 10.4772 degrees
Field rotation angle: up is -179.217 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jun 20 07:02 fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
-rw-r--r-- 1 apache apache 8.5K Jun 20 07:02 out3835881.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits for reading... done!
Creating new image file (wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 100000 sources.
Solving...
Reading file "./wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.axy"...
Verifying WCS using indices with quads of size [63.1854, 947.188] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 3.97254
Verifying WCS using indices with quads of size [63.1854, 947.188] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 3.97254
Got 0 solutions.
Field 1 did not solve (index index-5203-47.fits, field objects 1-10).
Field 1 did not solve (index index-5203-46.fits, field objects 1-10).
Field 1 did not solve (index index-5203-45.fits, field objects 1-10).
Field 1 did not solve (index index-5203-44.fits, field objects 1-10).
Field 1 did not solve (index index-5203-43.fits, field objects 1-10).
Field 1 did not solve (index index-5203-42.fits, field objects 1-10).
Field 1 did not solve (index index-5203-41.fits, field objects 1-10).
Field 1 did not solve (index index-5203-40.fits, field objects 1-10).
Field 1 did not solve (index index-5203-39.fits, field objects 1-10).
Field 1 did not solve (index index-5203-38.fits, field objects 1-10).
Field 1 did not solve (index index-5203-37.fits, field objects 1-10).
Field 1 did not solve (index index-5203-36.fits, field objects 1-10).
Field 1 did not solve (index index-5203-35.fits, field objects 1-10).
Field 1 did not solve (index index-5203-34.fits, field objects 1-10).
Field 1 did not solve (index index-5203-33.fits, field objects 1-10).
Field 1 did not solve (index index-5203-32.fits, field objects 1-10).
Field 1 did not solve (index index-5203-31.fits, field objects 1-10).
Field 1 did not solve (index index-5203-30.fits, field objects 1-10).
Field 1 did not solve (index index-5203-29.fits, field objects 1-10).
Field 1 did not solve (index index-5203-28.fits, field objects 1-10).
Field 1 did not solve (index index-5203-27.fits, field objects 1-10).
Field 1 did not solve (index index-5203-26.fits, field objects 1-10).
Field 1 did not solve (index index-5203-25.fits, field objects 1-10).
Field 1 did not solve (index index-5203-24.fits, field objects 1-10).
Field 1 did not solve (index index-5203-23.fits, field objects 1-10).
Field 1 did not solve (index index-5203-22.fits, field objects 1-10).
Field 1 did not solve (index index-5203-21.fits, field objects 1-10).
Field 1 did not solve (index index-5203-20.fits, field objects 1-10).
Field 1 did not solve (index index-5203-19.fits, field objects 1-10).
Field 1 did not solve (index index-5203-18.fits, field objects 1-10).
Field 1 did not solve (index index-5203-17.fits, field objects 1-10).
Field 1 did not solve (index index-5203-16.fits, field objects 1-10).
Field 1 did not solve (index index-5203-15.fits, field objects 1-10).
Field 1 did not solve (index index-5203-14.fits, field objects 1-10).
Field 1 did not solve (index index-5203-13.fits, field objects 1-10).
Field 1 did not solve (index index-5203-12.fits, field objects 1-10).
Field 1 did not solve (index index-5203-11.fits, field objects 1-10).
Field 1 did not solve (index index-5203-10.fits, field objects 1-10).
Field 1 did not solve (index index-5203-09.fits, field objects 1-10).
Field 1 did not solve (index index-5203-08.fits, field objects 1-10).
Field 1 did not solve (index index-5203-07.fits, field objects 1-10).
Field 1 did not solve (index index-5203-06.fits, field objects 1-10).
Field 1 did not solve (index index-5203-05.fits, field objects 1-10).
Field 1 did not solve (index index-5203-04.fits, field objects 1-10).
Field 1 did not solve (index index-5203-03.fits, field objects 1-10).
Field 1 did not solve (index index-5203-02.fits, field objects 1-10).
Field 1 did not solve (index index-5203-01.fits, field objects 1-10).
Field 1 did not solve (index index-5203-00.fits, field objects 1-10).
Field 1 did not solve (index index-5005-11.fits, field objects 1-10).
Field 1 did not solve (index index-5005-10.fits, field objects 1-10).
Field 1 did not solve (index index-5005-09.fits, field objects 1-10).
Field 1 did not solve (index index-5005-08.fits, field objects 1-10).
Field 1 did not solve (index index-5005-07.fits, field objects 1-10).
Field 1 did not solve (index index-5005-06.fits, field objects 1-10).
Field 1 did not solve (index index-5005-05.fits, field objects 1-10).
Field 1 did not solve (index index-5005-04.fits, field objects 1-10).
Field 1 did not solve (index index-5005-03.fits, field objects 1-10).
Field 1 did not solve (index index-5005-02.fits, field objects 1-10).
Field 1 did not solve (index index-5005-01.fits, field objects 1-10).
Field 1 did not solve (index index-5005-00.fits, field objects 1-10).
Field 1 did not solve (index index-4206-11.fits, field objects 1-10).
Field 1 did not solve (index index-4206-10.fits, field objects 1-10).
Field 1 did not solve (index index-4206-09.fits, field objects 1-10).
Field 1 did not solve (index index-4206-08.fits, field objects 1-10).
Field 1 did not solve (index index-4206-07.fits, field objects 1-10).
Field 1 did not solve (index index-4206-06.fits, field objects 1-10).
Field 1 did not solve (index index-4206-05.fits, field objects 1-10).
Field 1 did not solve (index index-4206-04.fits, field objects 1-10).
Field 1 did not solve (index index-4206-03.fits, field objects 1-10).
Field 1 did not solve (index index-4206-02.fits, field objects 1-10).
Field 1 did not solve (index index-4206-01.fits, field objects 1-10).
Field 1 did not solve (index index-4206-00.fits, field objects 1-10).
Field 1 did not solve (index index-4205-11.fits, field objects 1-10).
Field 1 did not solve (index index-4205-10.fits, field objects 1-10).
Field 1 did not solve (index index-4205-09.fits, field objects 1-10).
Field 1 did not solve (index index-4205-08.fits, field objects 1-10).
Field 1 did not solve (index index-4205-07.fits, field objects 1-10).
Field 1 did not solve (index index-4205-06.fits, field objects 1-10).
Field 1 did not solve (index index-4205-05.fits, field objects 1-10).
Field 1 did not solve (index index-4205-04.fits, field objects 1-10).
Field 1 did not solve (index index-4205-03.fits, field objects 1-10).
Field 1 did not solve (index index-4205-02.fits, field objects 1-10).
Field 1 did not solve (index index-4205-01.fits, field objects 1-10).
Field 1 did not solve (index index-4205-00.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4107.fits, field objects 1-10).
Field 1 did not solve (index index-204-11.fits, field objects 1-10).
Field 1 did not solve (index index-204-10.fits, field objects 1-10).
Field 1 did not solve (index index-204-09.fits, field objects 1-10).
Field 1 did not solve (index index-204-08.fits, field objects 1-10).
Field 1 did not solve (index index-204-07.fits, field objects 1-10).
Field 1 did not solve (index index-204-06.fits, field objects 1-10).
Field 1 did not solve (index index-204-05.fits, field objects 1-10).
Field 1 did not solve (index index-204-04.fits, field objects 1-10).
Field 1 did not solve (index index-204-03.fits, field objects 1-10).
Field 1 did not solve (index index-204-02.fits, field objects 1-10).
Field 1 did not solve (index index-204-01.fits, field objects 1-10).
Field 1 did not solve (index index-204-00.fits, field objects 1-10).
Field 1 did not solve (index index-5203-47.fits, field objects 11-20).
Field 1 did not solve (index index-5203-46.fits, field objects 11-20).
Field 1 did not solve (index index-5203-45.fits, field objects 11-20).
Field 1 did not solve (index index-5203-44.fits, field objects 11-20).
Field 1 did not solve (index index-5203-43.fits, field objects 11-20).
Field 1 did not solve (index index-5203-42.fits, field objects 11-20).
Field 1 did not solve (index index-5203-41.fits, field objects 11-20).
Field 1 did not solve (index index-5203-40.fits, field objects 11-20).
Field 1 did not solve (index index-5203-39.fits, field objects 11-20).
Field 1 did not solve (index index-5203-38.fits, field objects 11-20).
Field 1 did not solve (index index-5203-37.fits, field objects 11-20).
Field 1 did not solve (index index-5203-36.fits, field objects 11-20).
Field 1 did not solve (index index-5203-35.fits, field objects 11-20).
Field 1 did not solve (index index-5203-34.fits, field objects 11-20).
Field 1 did not solve (index index-5203-33.fits, field objects 11-20).
Field 1 did not solve (index index-5203-32.fits, field objects 11-20).
Field 1 did not solve (index index-5203-31.fits, field objects 11-20).
Field 1 did not solve (index index-5203-30.fits, field objects 11-20).
Field 1 did not solve (index index-5203-29.fits, field objects 11-20).
Field 1 did not solve (index index-5203-28.fits, field objects 11-20).
Field 1 did not solve (index index-5203-27.fits, field objects 11-20).
Field 1 did not solve (index index-5203-26.fits, field objects 11-20).
Field 1 did not solve (index index-5203-25.fits, field objects 11-20).
Field 1 did not solve (index index-5203-24.fits, field objects 11-20).
Field 1 did not solve (index index-5203-23.fits, field objects 11-20).
Field 1 did not solve (index index-5203-22.fits, field objects 11-20).
Field 1 did not solve (index index-5203-21.fits, field objects 11-20).
Field 1 did not solve (index index-5203-20.fits, field objects 11-20).
Field 1 did not solve (index index-5203-19.fits, field objects 11-20).
Field 1 did not solve (index index-5203-18.fits, field objects 11-20).
Field 1 did not solve (index index-5203-17.fits, field objects 11-20).
Field 1 did not solve (index index-5203-16.fits, field objects 11-20).
Field 1 did not solve (index index-5203-15.fits, field objects 11-20).
Field 1 did not solve (index index-5203-14.fits, field objects 11-20).
Field 1 did not solve (index index-5203-13.fits, field objects 11-20).
Field 1 did not solve (index index-5203-12.fits, field objects 11-20).
Field 1 did not solve (index index-5203-11.fits, field objects 11-20).
Field 1 did not solve (index index-5203-10.fits, field objects 11-20).
Field 1 did not solve (index index-5203-09.fits, field objects 11-20).
Field 1 did not solve (index index-5203-08.fits, field objects 11-20).
Field 1 did not solve (index index-5203-07.fits, field objects 11-20).
Field 1 did not solve (index index-5203-06.fits, field objects 11-20).
Field 1 did not solve (index index-5203-05.fits, field objects 11-20).
Field 1 did not solve (index index-5203-04.fits, field objects 11-20).
Field 1 did not solve (index index-5203-03.fits, field objects 11-20).
Field 1 did not solve (index index-5203-02.fits, field objects 11-20).
Field 1 did not solve (index index-5203-01.fits, field objects 11-20).
Field 1 did not solve (index index-5203-00.fits, field objects 11-20).
Field 1 did not solve (index index-5005-11.fits, field objects 11-20).
Field 1 did not solve (index index-5005-10.fits, field objects 11-20).
Field 1 did not solve (index index-5005-09.fits, field objects 11-20).
Field 1 did not solve (index index-5005-08.fits, field objects 11-20).
Field 1 did not solve (index index-5005-07.fits, field objects 11-20).
Field 1 did not solve (index index-5005-06.fits, field objects 11-20).
Field 1 did not solve (index index-5005-05.fits, field objects 11-20).
Field 1 did not solve (index index-5005-04.fits, field objects 11-20).
Field 1 did not solve (index index-5005-03.fits, field objects 11-20).
Field 1 did not solve (index index-5005-02.fits, field objects 11-20).
Field 1 did not solve (index index-5005-01.fits, field objects 11-20).
Field 1 did not solve (index index-5005-00.fits, field objects 11-20).
Field 1 did not solve (index index-4206-11.fits, field objects 11-20).
Field 1 did not solve (index index-4206-10.fits, field objects 11-20).
Field 1 did not solve (index index-4206-09.fits, field objects 11-20).
Field 1 did not solve (index index-4206-08.fits, field objects 11-20).
Field 1 did not solve (index index-4206-07.fits, field objects 11-20).
Field 1 did not solve (index index-4206-06.fits, field objects 11-20).
Field 1 did not solve (index index-4206-05.fits, field objects 11-20).
Field 1 did not solve (index index-4206-04.fits, field objects 11-20).
Field 1 did not solve (index index-4206-03.fits, field objects 11-20).
Field 1 did not solve (index index-4206-02.fits, field objects 11-20).
Field 1 did not solve (index index-4206-01.fits, field objects 11-20).
Field 1 did not solve (index index-4206-00.fits, field objects 11-20).
Field 1 did not solve (index index-4205-11.fits, field objects 11-20).
Field 1 did not solve (index index-4205-10.fits, field objects 11-20).
Field 1 did not solve (index index-4205-09.fits, field objects 11-20).
Field 1 did not solve (index index-4205-08.fits, field objects 11-20).
Field 1 did not solve (index index-4205-07.fits, field objects 11-20).
Field 1 did not solve (index index-4205-06.fits, field objects 11-20).
Field 1 did not solve (index index-4205-05.fits, field objects 11-20).
Field 1 did not solve (index index-4205-04.fits, field objects 11-20).
Field 1 did not solve (index index-4205-03.fits, field objects 11-20).
Field 1 did not solve (index index-4205-02.fits, field objects 11-20).
Field 1 did not solve (index index-4205-01.fits, field objects 11-20).
Field 1 did not solve (index index-4205-00.fits, field objects 11-20).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
Field 1 did not solve (index index-4115.fits, field objects 11-20).
Field 1 did not solve (index index-4114.fits, field objects 11-20).
Field 1 did not solve (index index-4113.fits, field objects 11-20).
Field 1 did not solve (index index-4112.fits, field objects 11-20).
Field 1 did not solve (index index-4111.fits, field objects 11-20).
Field 1 did not solve (index index-4110.fits, field objects 11-20).
Field 1 did not solve (index index-4109.fits, field objects 11-20).
Field 1 did not solve (index index-4108.fits, field objects 11-20).
Field 1 did not solve (index index-4107.fits, field objects 11-20).
Field 1 did not solve (index index-204-11.fits, field objects 11-20).
Field 1 did not solve (index index-204-10.fits, field objects 11-20).
Field 1 did not solve (index index-204-09.fits, field objects 11-20).
Field 1 did not solve (index index-204-08.fits, field objects 11-20).
Field 1 did not solve (index index-204-07.fits, field objects 11-20).
Field 1 did not solve (index index-204-06.fits, field objects 11-20).
Field 1 did not solve (index index-204-05.fits, field objects 11-20).
Field 1 did not solve (index index-204-04.fits, field objects 11-20).
Field 1 did not solve (index index-204-03.fits, field objects 11-20).
Field 1 did not solve (index index-204-02.fits, field objects 11-20).
Field 1 did not solve (index index-204-01.fits, field objects 11-20).
Field 1 did not solve (index index-204-00.fits, field objects 11-20).
Field 1 did not solve (index index-5203-47.fits, field objects 21-30).
Field 1 did not solve (index index-5203-46.fits, field objects 21-30).
Field 1 did not solve (index index-5203-45.fits, field objects 21-30).
Field 1 did not solve (index index-5203-44.fits, field objects 21-30).
Field 1 did not solve (index index-5203-43.fits, field objects 21-30).
Field 1 did not solve (index index-5203-42.fits, field objects 21-30).
Field 1 did not solve (index index-5203-41.fits, field objects 21-30).
Field 1 did not solve (index index-5203-40.fits, field objects 21-30).
Field 1 did not solve (index index-5203-39.fits, field objects 21-30).
Field 1 did not solve (index index-5203-38.fits, field objects 21-30).
Field 1 did not solve (index index-5203-37.fits, field objects 21-30).
Field 1 did not solve (index index-5203-36.fits, field objects 21-30).
Field 1 did not solve (index index-5203-35.fits, field objects 21-30).
Field 1 did not solve (index index-5203-34.fits, field objects 21-30).
Field 1 did not solve (index index-5203-33.fits, field objects 21-30).
Field 1 did not solve (index index-5203-32.fits, field objects 21-30).
Field 1 did not solve (index index-5203-31.fits, field objects 21-30).
Field 1 did not solve (index index-5203-30.fits, field objects 21-30).
Field 1 did not solve (index index-5203-29.fits, field objects 21-30).
Field 1 did not solve (index index-5203-28.fits, field objects 21-30).
Field 1 did not solve (index index-5203-27.fits, field objects 21-30).
Field 1 did not solve (index index-5203-26.fits, field objects 21-30).
Field 1 did not solve (index index-5203-25.fits, field objects 21-30).
Field 1 did not solve (index index-5203-24.fits, field objects 21-30).
Field 1 did not solve (index index-5203-23.fits, field objects 21-30).
Field 1 did not solve (index index-5203-22.fits, field objects 21-30).
Field 1 did not solve (index index-5203-21.fits, field objects 21-30).
Field 1 did not solve (index index-5203-20.fits, field objects 21-30).
Field 1 did not solve (index index-5203-19.fits, field objects 21-30).
Field 1 did not solve (index index-5203-18.fits, field objects 21-30).
Field 1 did not solve (index index-5203-17.fits, field objects 21-30).
Field 1 did not solve (index index-5203-16.fits, field objects 21-30).
Field 1 did not solve (index index-5203-15.fits, field objects 21-30).
Field 1 did not solve (index index-5203-14.fits, field objects 21-30).
Field 1 did not solve (index index-5203-13.fits, field objects 21-30).
Field 1 did not solve (index index-5203-12.fits, field objects 21-30).
Field 1 did not solve (index index-5203-11.fits, field objects 21-30).
Field 1 did not solve (index index-5203-10.fits, field objects 21-30).
Field 1 did not solve (index index-5203-09.fits, field objects 21-30).
Field 1 did not solve (index index-5203-08.fits, field objects 21-30).
Field 1 did not solve (index index-5203-07.fits, field objects 21-30).
Field 1 did not solve (index index-5203-06.fits, field objects 21-30).
Field 1 did not solve (index index-5203-05.fits, field objects 21-30).
Field 1 did not solve (index index-5203-04.fits, field objects 21-30).
Field 1 did not solve (index index-5203-03.fits, field objects 21-30).
Field 1 did not solve (index index-5203-02.fits, field objects 21-30).
Field 1 did not solve (index index-5203-01.fits, field objects 21-30).
Field 1 did not solve (index index-5203-00.fits, field objects 21-30).
Field 1 did not solve (index index-5005-11.fits, field objects 21-30).
Field 1 did not solve (index index-5005-10.fits, field objects 21-30).
Field 1 did not solve (index index-5005-09.fits, field objects 21-30).
Field 1 did not solve (index index-5005-08.fits, field objects 21-30).
Field 1 did not solve (index index-5005-07.fits, field objects 21-30).
Field 1 did not solve (index index-5005-06.fits, field objects 21-30).
Field 1 did not solve (index index-5005-05.fits, field objects 21-30).
Field 1 did not solve (index index-5005-04.fits, field objects 21-30).
Field 1 did not solve (index index-5005-03.fits, field objects 21-30).
Field 1 did not solve (index index-5005-02.fits, field objects 21-30).
Field 1 did not solve (index index-5005-01.fits, field objects 21-30).
Field 1 did not solve (index index-5005-00.fits, field objects 21-30).
Field 1 did not solve (index index-4206-11.fits, field objects 21-30).
Field 1 did not solve (index index-4206-10.fits, field objects 21-30).
Field 1 did not solve (index index-4206-09.fits, field objects 21-30).
Field 1 did not solve (index index-4206-08.fits, field objects 21-30).
Field 1 did not solve (index index-4206-07.fits, field objects 21-30).
Field 1 did not solve (index index-4206-06.fits, field objects 21-30).
Field 1 did not solve (index index-4206-05.fits, field objects 21-30).
Field 1 did not solve (index index-4206-04.fits, field objects 21-30).
Field 1 did not solve (index index-4206-03.fits, field objects 21-30).
Field 1 did not solve (index index-4206-02.fits, field objects 21-30).
Field 1 did not solve (index index-4206-01.fits, field objects 21-30).
Field 1 did not solve (index index-4206-00.fits, field objects 21-30).
Field 1 did not solve (index index-4205-11.fits, field objects 21-30).
Field 1 did not solve (index index-4205-10.fits, field objects 21-30).
Field 1 did not solve (index index-4205-09.fits, field objects 21-30).
Field 1 did not solve (index index-4205-08.fits, field objects 21-30).
Field 1 did not solve (index index-4205-07.fits, field objects 21-30).
Field 1 did not solve (index index-4205-06.fits, field objects 21-30).
Field 1 did not solve (index index-4205-05.fits, field objects 21-30).
Field 1 did not solve (index index-4205-04.fits, field objects 21-30).
Field 1 did not solve (index index-4205-03.fits, field objects 21-30).
Field 1 did not solve (index index-4205-02.fits, field objects 21-30).
Field 1 did not solve (index index-4205-01.fits, field objects 21-30).
Field 1 did not solve (index index-4205-00.fits, field objects 21-30).
Field 1 did not solve (index index-4119.fits, field objects 21-30).
Field 1 did not solve (index index-4118.fits, field objects 21-30).
Field 1 did not solve (index index-4117.fits, field objects 21-30).
Field 1 did not solve (index index-4116.fits, field objects 21-30).
Field 1 did not solve (index index-4115.fits, field objects 21-30).
Field 1 did not solve (index index-4114.fits, field objects 21-30).
Field 1 did not solve (index index-4113.fits, field objects 21-30).
Total CPU time limit reached!
Field 1 did not solve (index index-4112.fits, field objects 21-30).
Field: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
Did not solve (or no WCS file was written).
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
Generating wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat from image00003.cat
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits created.
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
Image size: 939.5'x622.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 21:10:35.552 +53:59:23.23 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 25248 stars ###
'wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/correct_sextractor_wcs_catalog_usingxy2sky3982838.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2819, passed=25248
Got 25248 stars (including 22396 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat
util/solve_plate_with_UCAC5 got 25248 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.5'
Seting catalog search parameters based on the expected field of view 939.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013049 (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 0.010439 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 320 matched stars entering correct_measured_positions(), 8754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.85"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 456 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 380 matched stars entering correct_measured_positions(), 8780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.79"
Accuracy estimation diagnostic: 374 matched stars entering correct_measured_positions(), 9542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.67"
Excluding outliers - 374 stars left (next iteration limit 352)
WCS_QUALITY_DIAG: file=fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits N_match=374 sigma_overall_arcsec=5.745 sigma_q1_arcsec=25.514 sigma_q2_arcsec=33.280 sigma_q3_arcsec=5.989 sigma_q4_arcsec=4.232 n_q1=28 n_q2=18 n_q3=151 n_q4=177 worst_quadrant_to_overall_ratio=5.793
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits): sigma 5.745->5.745, ratio 5.793->5.793; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits) flagged: sigma=5.839 (ref avg 0.767), ratio=4.742 (ref avg 1.1765), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/lib/make_outxyls_for_astrometric_calibration found 23665 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out3984822.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3984822.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
log-odds ratio 36.3178 (5.92381e+15), 15 match, 0 conflict, 33 distractors, 186 index.
RA,Dec = (317.696,54.0434), pixel scale 5.90985 arcsec/pix.
Hit/miss: Hit/miss: -++--+++------------++---++---+----------++--+++(best)-------------++--++---+---------++--------+---------
Field 1: solved with index index-4113.fits.
Field 1 solved: writing to file ./out3984822.solved to indicate this.
Field: out3984822.xyls
Field center: (RA,Dec) = (317.636840, 54.017235) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:10:32.842, +54:01:02.045).
Field size: 15.7319 x 10.5338 degrees
Field rotation angle: up is -179.25 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits' -> 'fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jun 20 07:11 fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
-rw-r--r-- 1 apache apache 12K Jun 20 07:11 out3984822.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits for reading... done!
Creating new image file (wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits (fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out3984822.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3984822.axy"...
Only searching for solutions within 15.6667 degrees of RA,Dec (317.635,54.0164)
log-odds ratio 60.247 (1.462e+26), 8 match, 0 conflict, 11 distractors, 23 index.
RA,Dec = (317.65,53.9939), pixel scale 5.93478 arcsec/pix.
Hit/miss: Hit/miss: ---+++---+--+++---+(best)---------------------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out3984822.solved to indicate this.
Field: out3984822.xyls
Field center: (RA,Dec) = (317.637699, 53.993541) deg.
Field center: (RA H:M:S, Dec D:M:S) = (21:10:33.048, +53:59:36.749).
Field size: 15.7238 x 10.4772 degrees
Field rotation angle: up is -179.217 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jun 20 07:11 fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
-rw-r--r-- 1 apache apache 8.5K Jun 20 07:11 out3984822.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits for reading... done!
Creating new image file (wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 100000 sources.
Solving...
Reading file "./wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.axy"...
Verifying WCS using indices with quads of size [63.1856, 947.19] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0.105503
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0.62158
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 13.2457
Verifying WCS using indices with quads of size [63.1856, 947.19] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
--> log-odds 0.105503
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
--> log-odds 0.62158
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
--> log-odds 13.2457
Got 0 solutions.
Field 1 did not solve (index index-5203-47.fits, field objects 1-10).
Field 1 did not solve (index index-5203-46.fits, field objects 1-10).
Field 1 did not solve (index index-5203-45.fits, field objects 1-10).
Field 1 did not solve (index index-5203-44.fits, field objects 1-10).
Field 1 did not solve (index index-5203-43.fits, field objects 1-10).
Field 1 did not solve (index index-5203-42.fits, field objects 1-10).
Field 1 did not solve (index index-5203-41.fits, field objects 1-10).
Field 1 did not solve (index index-5203-40.fits, field objects 1-10).
Field 1 did not solve (index index-5203-39.fits, field objects 1-10).
Field 1 did not solve (index index-5203-38.fits, field objects 1-10).
Field 1 did not solve (index index-5203-37.fits, field objects 1-10).
Field 1 did not solve (index index-5203-36.fits, field objects 1-10).
Field 1 did not solve (index index-5203-35.fits, field objects 1-10).
Field 1 did not solve (index index-5203-34.fits, field objects 1-10).
Field 1 did not solve (index index-5203-33.fits, field objects 1-10).
Field 1 did not solve (index index-5203-32.fits, field objects 1-10).
Field 1 did not solve (index index-5203-31.fits, field objects 1-10).
Field 1 did not solve (index index-5203-30.fits, field objects 1-10).
Field 1 did not solve (index index-5203-29.fits, field objects 1-10).
Field 1 did not solve (index index-5203-28.fits, field objects 1-10).
Field 1 did not solve (index index-5203-27.fits, field objects 1-10).
Field 1 did not solve (index index-5203-26.fits, field objects 1-10).
Field 1 did not solve (index index-5203-25.fits, field objects 1-10).
Field 1 did not solve (index index-5203-24.fits, field objects 1-10).
Field 1 did not solve (index index-5203-23.fits, field objects 1-10).
Field 1 did not solve (index index-5203-22.fits, field objects 1-10).
Field 1 did not solve (index index-5203-21.fits, field objects 1-10).
Field 1 did not solve (index index-5203-20.fits, field objects 1-10).
Field 1 did not solve (index index-5203-19.fits, field objects 1-10).
Field 1 did not solve (index index-5203-18.fits, field objects 1-10).
Field 1 did not solve (index index-5203-17.fits, field objects 1-10).
Field 1 did not solve (index index-5203-16.fits, field objects 1-10).
Field 1 did not solve (index index-5203-15.fits, field objects 1-10).
Field 1 did not solve (index index-5203-14.fits, field objects 1-10).
Field 1 did not solve (index index-5203-13.fits, field objects 1-10).
Field 1 did not solve (index index-5203-12.fits, field objects 1-10).
Field 1 did not solve (index index-5203-11.fits, field objects 1-10).
Field 1 did not solve (index index-5203-10.fits, field objects 1-10).
Field 1 did not solve (index index-5203-09.fits, field objects 1-10).
Field 1 did not solve (index index-5203-08.fits, field objects 1-10).
Field 1 did not solve (index index-5203-07.fits, field objects 1-10).
Field 1 did not solve (index index-5203-06.fits, field objects 1-10).
Field 1 did not solve (index index-5203-05.fits, field objects 1-10).
Field 1 did not solve (index index-5203-04.fits, field objects 1-10).
Field 1 did not solve (index index-5203-03.fits, field objects 1-10).
Field 1 did not solve (index index-5203-02.fits, field objects 1-10).
Field 1 did not solve (index index-5203-01.fits, field objects 1-10).
Field 1 did not solve (index index-5203-00.fits, field objects 1-10).
Field 1 did not solve (index index-5005-11.fits, field objects 1-10).
Field 1 did not solve (index index-5005-10.fits, field objects 1-10).
Field 1 did not solve (index index-5005-09.fits, field objects 1-10).
Field 1 did not solve (index index-5005-08.fits, field objects 1-10).
Field 1 did not solve (index index-5005-07.fits, field objects 1-10).
Field 1 did not solve (index index-5005-06.fits, field objects 1-10).
Field 1 did not solve (index index-5005-05.fits, field objects 1-10).
Field 1 did not solve (index index-5005-04.fits, field objects 1-10).
Field 1 did not solve (index index-5005-03.fits, field objects 1-10).
Field 1 did not solve (index index-5005-02.fits, field objects 1-10).
Field 1 did not solve (index index-5005-01.fits, field objects 1-10).
Field 1 did not solve (index index-5005-00.fits, field objects 1-10).
Field 1 did not solve (index index-4206-11.fits, field objects 1-10).
Field 1 did not solve (index index-4206-10.fits, field objects 1-10).
Field 1 did not solve (index index-4206-09.fits, field objects 1-10).
Field 1 did not solve (index index-4206-08.fits, field objects 1-10).
Field 1 did not solve (index index-4206-07.fits, field objects 1-10).
Field 1 did not solve (index index-4206-06.fits, field objects 1-10).
Field 1 did not solve (index index-4206-05.fits, field objects 1-10).
Field 1 did not solve (index index-4206-04.fits, field objects 1-10).
Field 1 did not solve (index index-4206-03.fits, field objects 1-10).
Field 1 did not solve (index index-4206-02.fits, field objects 1-10).
Field 1 did not solve (index index-4206-01.fits, field objects 1-10).
Field 1 did not solve (index index-4206-00.fits, field objects 1-10).
Field 1 did not solve (index index-4205-11.fits, field objects 1-10).
Field 1 did not solve (index index-4205-10.fits, field objects 1-10).
Field 1 did not solve (index index-4205-09.fits, field objects 1-10).
Field 1 did not solve (index index-4205-08.fits, field objects 1-10).
Field 1 did not solve (index index-4205-07.fits, field objects 1-10).
Field 1 did not solve (index index-4205-06.fits, field objects 1-10).
Field 1 did not solve (index index-4205-05.fits, field objects 1-10).
Field 1 did not solve (index index-4205-04.fits, field objects 1-10).
Field 1 did not solve (index index-4205-03.fits, field objects 1-10).
Field 1 did not solve (index index-4205-02.fits, field objects 1-10).
Field 1 did not solve (index index-4205-01.fits, field objects 1-10).
Field 1 did not solve (index index-4205-00.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4107.fits, field objects 1-10).
Field 1 did not solve (index index-204-11.fits, field objects 1-10).
Field 1 did not solve (index index-204-10.fits, field objects 1-10).
Field 1 did not solve (index index-204-09.fits, field objects 1-10).
Field 1 did not solve (index index-204-08.fits, field objects 1-10).
Field 1 did not solve (index index-204-07.fits, field objects 1-10).
Field 1 did not solve (index index-204-06.fits, field objects 1-10).
Field 1 did not solve (index index-204-05.fits, field objects 1-10).
Field 1 did not solve (index index-204-04.fits, field objects 1-10).
Field 1 did not solve (index index-204-03.fits, field objects 1-10).
Field 1 did not solve (index index-204-02.fits, field objects 1-10).
Field 1 did not solve (index index-204-01.fits, field objects 1-10).
Field 1 did not solve (index index-204-00.fits, field objects 1-10).
Field 1 did not solve (index index-5203-47.fits, field objects 11-20).
Field 1 did not solve (index index-5203-46.fits, field objects 11-20).
Field 1 did not solve (index index-5203-45.fits, field objects 11-20).
Field 1 did not solve (index index-5203-44.fits, field objects 11-20).
Field 1 did not solve (index index-5203-43.fits, field objects 11-20).
Field 1 did not solve (index index-5203-42.fits, field objects 11-20).
Field 1 did not solve (index index-5203-41.fits, field objects 11-20).
Field 1 did not solve (index index-5203-40.fits, field objects 11-20).
Field 1 did not solve (index index-5203-39.fits, field objects 11-20).
Field 1 did not solve (index index-5203-38.fits, field objects 11-20).
Field 1 did not solve (index index-5203-37.fits, field objects 11-20).
Field 1 did not solve (index index-5203-36.fits, field objects 11-20).
Field 1 did not solve (index index-5203-35.fits, field objects 11-20).
Field 1 did not solve (index index-5203-34.fits, field objects 11-20).
Field 1 did not solve (index index-5203-33.fits, field objects 11-20).
Field 1 did not solve (index index-5203-32.fits, field objects 11-20).
Field 1 did not solve (index index-5203-31.fits, field objects 11-20).
Field 1 did not solve (index index-5203-30.fits, field objects 11-20).
Field 1 did not solve (index index-5203-29.fits, field objects 11-20).
Field 1 did not solve (index index-5203-28.fits, field objects 11-20).
Field 1 did not solve (index index-5203-27.fits, field objects 11-20).
Field 1 did not solve (index index-5203-26.fits, field objects 11-20).
Field 1 did not solve (index index-5203-25.fits, field objects 11-20).
Field 1 did not solve (index index-5203-24.fits, field objects 11-20).
Field 1 did not solve (index index-5203-23.fits, field objects 11-20).
Field 1 did not solve (index index-5203-22.fits, field objects 11-20).
Field 1 did not solve (index index-5203-21.fits, field objects 11-20).
Field 1 did not solve (index index-5203-20.fits, field objects 11-20).
Field 1 did not solve (index index-5203-19.fits, field objects 11-20).
Field 1 did not solve (index index-5203-18.fits, field objects 11-20).
Field 1 did not solve (index index-5203-17.fits, field objects 11-20).
Field 1 did not solve (index index-5203-16.fits, field objects 11-20).
Field 1 did not solve (index index-5203-15.fits, field objects 11-20).
Field 1 did not solve (index index-5203-14.fits, field objects 11-20).
Field 1 did not solve (index index-5203-13.fits, field objects 11-20).
Field 1 did not solve (index index-5203-12.fits, field objects 11-20).
Field 1 did not solve (index index-5203-11.fits, field objects 11-20).
Field 1 did not solve (index index-5203-10.fits, field objects 11-20).
Field 1 did not solve (index index-5203-09.fits, field objects 11-20).
Field 1 did not solve (index index-5203-08.fits, field objects 11-20).
Field 1 did not solve (index index-5203-07.fits, field objects 11-20).
Field 1 did not solve (index index-5203-06.fits, field objects 11-20).
Field 1 did not solve (index index-5203-05.fits, field objects 11-20).
Field 1 did not solve (index index-5203-04.fits, field objects 11-20).
Field 1 did not solve (index index-5203-03.fits, field objects 11-20).
Field 1 did not solve (index index-5203-02.fits, field objects 11-20).
Field 1 did not solve (index index-5203-01.fits, field objects 11-20).
Field 1 did not solve (index index-5203-00.fits, field objects 11-20).
Field 1 did not solve (index index-5005-11.fits, field objects 11-20).
Field 1 did not solve (index index-5005-10.fits, field objects 11-20).
Field 1 did not solve (index index-5005-09.fits, field objects 11-20).
Field 1 did not solve (index index-5005-08.fits, field objects 11-20).
Field 1 did not solve (index index-5005-07.fits, field objects 11-20).
Field 1 did not solve (index index-5005-06.fits, field objects 11-20).
Field 1 did not solve (index index-5005-05.fits, field objects 11-20).
Field 1 did not solve (index index-5005-04.fits, field objects 11-20).
Field 1 did not solve (index index-5005-03.fits, field objects 11-20).
Field 1 did not solve (index index-5005-02.fits, field objects 11-20).
Field 1 did not solve (index index-5005-01.fits, field objects 11-20).
Field 1 did not solve (index index-5005-00.fits, field objects 11-20).
Field 1 did not solve (index index-4206-11.fits, field objects 11-20).
Field 1 did not solve (index index-4206-10.fits, field objects 11-20).
Field 1 did not solve (index index-4206-09.fits, field objects 11-20).
Field 1 did not solve (index index-4206-08.fits, field objects 11-20).
Field 1 did not solve (index index-4206-07.fits, field objects 11-20).
Field 1 did not solve (index index-4206-06.fits, field objects 11-20).
Field 1 did not solve (index index-4206-05.fits, field objects 11-20).
Field 1 did not solve (index index-4206-04.fits, field objects 11-20).
Field 1 did not solve (index index-4206-03.fits, field objects 11-20).
Field 1 did not solve (index index-4206-02.fits, field objects 11-20).
Field 1 did not solve (index index-4206-01.fits, field objects 11-20).
Field 1 did not solve (index index-4206-00.fits, field objects 11-20).
Field 1 did not solve (index index-4205-11.fits, field objects 11-20).
Field 1 did not solve (index index-4205-10.fits, field objects 11-20).
Field 1 did not solve (index index-4205-09.fits, field objects 11-20).
Field 1 did not solve (index index-4205-08.fits, field objects 11-20).
Field 1 did not solve (index index-4205-07.fits, field objects 11-20).
Field 1 did not solve (index index-4205-06.fits, field objects 11-20).
Field 1 did not solve (index index-4205-05.fits, field objects 11-20).
Field 1 did not solve (index index-4205-04.fits, field objects 11-20).
Field 1 did not solve (index index-4205-03.fits, field objects 11-20).
Field 1 did not solve (index index-4205-02.fits, field objects 11-20).
Field 1 did not solve (index index-4205-01.fits, field objects 11-20).
Field 1 did not solve (index index-4205-00.fits, field objects 11-20).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
Field 1 did not solve (index index-4115.fits, field objects 11-20).
Field 1 did not solve (index index-4114.fits, field objects 11-20).
Field 1 did not solve (index index-4113.fits, field objects 11-20).
Field 1 did not solve (index index-4112.fits, field objects 11-20).
Total CPU time limit reached!
Field 1 did not solve (index index-4111.fits, field objects 11-20).
Field: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
Did not solve (or no WCS file was written).
Checking if the catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
Generating wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat from image00004.cat
Catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat corresponding to the image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits created.
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
verification OK: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
Image size: 939.5'x622.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 21:10:32.706 +53:59:33.83 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 24993 stars ###
'wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/correct_sextractor_wcs_catalog_usingxy2sky365264.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
WCS catalog name: wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2796, passed=24993
Got 24993 stars (including 22170 good ones) from the SExtractor catalog wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat
util/solve_plate_with_UCAC5 got 24993 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.5'
Seting catalog search parameters based on the expected field of view 939.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013049 (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 0.010439 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 386 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 325 matched stars entering correct_measured_positions(), 257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 317 matched stars entering correct_measured_positions(), 8210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 456 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 401 matched stars entering correct_measured_positions(), 8253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.84"
Accuracy estimation diagnostic: 397 matched stars entering correct_measured_positions(), 10262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.96"
Excluding outliers - 397 stars left (next iteration limit 348)
WCS_QUALITY_DIAG: file=fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits N_match=397 sigma_overall_arcsec=5.839 sigma_q1_arcsec=26.511 sigma_q2_arcsec=27.686 sigma_q3_arcsec=7.153 sigma_q4_arcsec=4.442 n_q1=28 n_q2=20 n_q3=165 n_q4=184 worst_quadrant_to_overall_ratio=4.742
The image catalog is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits -region wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits): sigma 5.839->5.839, ratio 4.742->4.742; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=5.745 -- 7.49x the reference average (0.767); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=5.839 -- 7.61x the reference average (0.767); plate solution may be of low accuracy
WARNING: 1st new image has worst_quadrant_to_overall_ratio=5.793 -- 4.92x the reference average (1.1765); plate solution may be of low accuracy
WARNING: 2nd new image has worst_quadrant_to_overall_ratio=4.742 -- 4.03x the reference average (1.1765); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484_astrometric_residuals.png (967 matched stars from wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.65 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485_astrometric_residuals.png (967 matched stars from wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.69 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476_astrometric_residuals.png (374 matched stars from wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477_astrometric_residuals.png (397 matched stars from wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.87 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-16-21_20.00sec_5.00C_LIGHT_0476.fits'
Saving fully-calibrated image wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cyg-02-Q2b1x1_064507_TTUQ2b1x1_2653996_aJLo4rcr/wcs_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477.fits'
Preparing the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:09:14.63 +54:35:04.7: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:09.73 +50:13:30.7: 11.63 +/- 0.01 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:49:16.53 +52:43:15.4: 12.69 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:15:55.75 +54:48:14.3: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:27:40.11 +57:16:00.3: 14.78 +/- 0.23 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 20:58:44.50 +54:58:26.5: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:15:00.93 +52:48:20.7: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:20:24.89 +53:46:00.6: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:27:40.11 +57:16:00.3: 14.76 +/- 0.23 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:15:55.75 +54:48:14.3: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:09.73 +50:13:30.7: 11.63 +/- 0.01 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:49:16.53 +52:43:15.4: 12.69 +/- 0.03 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:09:14.63 +54:35:04.7: 15.58 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Forced photometry reference-image weighted average: 14.77 +/- 0.16
Forced photometry filter REJECTED candidate at 20:49:16.53 +52:43:15.4: ref_mag=12.69 +/- 0.02 new_mean_mag=11.9378 delta=0.75 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:35:09.73 +50:13:30.7: ref_mag=11.63 +/- 0.01 new_mean_mag=11.7705 delta=-0.14 (need > 0.90)
Forced photometry filter KEPT candidate at 21:27:40.11 +57:16:00.3: ref_mag=14.77 +/- 0.16 new_mean_mag=10.5151 delta=4.25 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:28:45.06 +52:13:13.3: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:26.37 +53:29:06.7: 15.16 +/- 0.34 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 20:58:44.50 +54:58:26.5: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:15:00.93 +52:48:20.7: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:20:24.89 +53:46:00.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:28:45.06 +52:13:13.3: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:26.37 +53:29:06.7: 15.22 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.16 +/- 0.34
Forced photometry filter KEPT candidate at 21:35:26.37 +53:29:06.7: ref_mag=15.16 +/- 0.34 new_mean_mag=12.0531 delta=3.11 (need > 0.90)
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-40-55_20.00sec_-4.90C_LIGHT_0484.fits at 21:35:51.53 +51:14:27.7: 12.46 +/- 0.02 detection
Forced photometry on wcs_Cyg-02-Q2b1x1_2026-05-11_04-41-39_20.00sec_-5.00C_LIGHT_0485.fits at 21:35:51.53 +51:14:27.7: 12.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Forced photometry filter KEPT candidate at 21:35:51.53 +51:14:27.7: ref_mag=12.51 +/- 0.02 new_mean_mag=10.8065 delta=1.70 (need > 0.90)
Adding exclusion_list_local.txt__out07816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36375.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 7s
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Considering the candidate 30801_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 30801_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 31372_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 31372_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (48.6") between the two second-epoch detections
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Considering the candidate 31842_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 31842_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 34307_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 34307_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (48.2") between the two second-epoch detections
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Considering the candidate 34746_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 34746_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 35071_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 35071_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 35139_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 35139_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 35379_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 35379_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 35453_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 35453_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 35500_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 35500_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 35592_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 35592_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (34.4") between the two second-epoch detections
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Considering the candidate 35712_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 35712_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 187858_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187858_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 187861_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187861_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187870_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187870_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187871_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187871_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 187897_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187897_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 187908_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187908_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 187911_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187911_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187913_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187913_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187917_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187917_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 187926_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187926_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 187934_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187934_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187938_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187938_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 187946_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187946_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 187952_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187952_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187953_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187953_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 187954_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187954_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187957_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187957_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187964_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187964_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 187967_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187967_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187970_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187970_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187971_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187971_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187972_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187972_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 187975_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187975_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187986_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187986_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187987_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187987_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187988_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187988_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187994_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 187994_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 187995_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187995_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187998_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187998_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 187999_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 187999_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188002_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188002_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 188007_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188007_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188012_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188012_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188021_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188021_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188027_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188027_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 188028_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188028_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188029_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188029_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188030_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188030_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188032_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188032_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188038_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188038_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188040_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188040_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 188042_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188042_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188043_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188043_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188049_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188049_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188050_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188050_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188059_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188059_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 188066_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188066_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188072_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188072_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 188078_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188078_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188079_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188079_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188082_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188082_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188083_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188083_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 188087_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188087_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 188092_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188092_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188096_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188096_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188099_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188099_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188100_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188100_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188101_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188101_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188102_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188102_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 188106_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188106_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188108_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188108_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188109_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188109_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 188112_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188112_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 188123_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188123_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188124_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188124_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188127_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188127_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188130_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188130_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188131_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188131_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188139_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188139_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
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Considering the candidate 188144_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188144_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188151_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188151_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 188154_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188154_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188156_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188156_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188162_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188162_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188163_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188163_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188165_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188165_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188168_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188168_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188169_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188169_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188171_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188171_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 188176_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188176_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188177_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188177_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
**** FOUND 21:13:22.31 +57:56:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 5.533 2189587938265900416 318.34411064325 +57.95093786082 14.8673 13.8797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188180_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188180_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 188182_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188182_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188189_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188189_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 188191_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188191_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188192_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188192_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 188194_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188194_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 188196_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188196_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 188206_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188206_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188210_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188210_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188215_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188215_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188216_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188216_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188218_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188218_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188226_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188226_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 188231_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188231_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188235_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188235_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188236_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188236_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188237_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188237_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188242_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188242_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188243_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188243_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188247_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188247_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188248_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188248_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188257_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188257_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188261_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188261_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 188263_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188263_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188264_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188264_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188266_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188266_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188276_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188276_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188280_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188280_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188281_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188281_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188283_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188283_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188285_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188285_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188288_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188288_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188291_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188291_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188294_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188294_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 188297_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188297_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188298_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188298_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188302_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188302_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 188303_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188303_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188305_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188305_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188310_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188310_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188312_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188312_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188315_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188315_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188317_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188317_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188318_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188318_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188321_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188321_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 188325_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188325_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188328_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188328_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188329_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188329_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
**** FOUND 21:36:58.12 +50:31:36.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 188330_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188330_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 188331_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188331_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188332_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188332_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188333_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188333_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188337_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188337_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188338_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 188338_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 188343_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188343_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188344_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188344_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 188820_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 188820_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 189304_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 189304_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (32.6") between the two second-epoch detections
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Considering the candidate 191705_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 191705_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 191985_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 191985_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 192418_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 192418_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 193147_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 193147_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 193652_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 193652_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 193952_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 193952_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 194603_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 194603_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 194643_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 194643_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 196362_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 196362_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 196504_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 196504_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 197614_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 197614_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 197883_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 197883_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 198114_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 198114_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 199625_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 199625_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 199857_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 199857_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 200295_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 200295_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 201642_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 201642_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 201646_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 201646_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 203328_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 203328_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 204864_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 204864_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 205064_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 205064_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 205202_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 205202_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 205714_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 205714_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 206047_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 206047_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 206557_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 206557_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 206710_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 206710_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 207322_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 207322_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 211469_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 211469_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 213428_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 213428_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 213531_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 213531_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 213567_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 213567_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 213605_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 213605_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (33.0") between the two second-epoch detections
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Considering the candidate 213656_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 213656_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 214795_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 214795_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 214826_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 214826_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 214912_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 214912_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 215517_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 215517_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 216083_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 216083_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 216321_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 216321_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 216653_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 216653_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 216826_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 216826_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (24.1") between the two second-epoch detections
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Considering the candidate 216940_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 216940_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 217766_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 217766_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 217848_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 217848_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 217876_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 217876_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 217934_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 217934_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 217972_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 217972_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 217979_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 217979_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218212_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218212_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218271_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218271_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218293_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 218293_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 218368_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218368_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218416_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218416_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218448_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218448_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218526_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218526_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218532_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 218532_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 218538_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 218538_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 218643_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218643_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218680_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218680_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218946_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 218946_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 218997_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 218997_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 219212_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 219212_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 219371_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 219371_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 219565_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 219565_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 219717_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 219717_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 219816_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 219816_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 219832_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 219832_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 219885_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 219885_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 219968_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 219968_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 220040_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 220040_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 220047_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 220047_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 220056_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 220056_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 220112_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 220112_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 220151_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 220151_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 220425_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 220425_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 220463_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 220463_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 220546_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 220546_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 220566_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 220566_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 220608_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 220608_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 220660_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 220660_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 220717_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 220717_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 220802_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 220802_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 220806_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 220806_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
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Considering the candidate 221077_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 221077_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 221102_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 221102_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 221129_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 221129_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 221146_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 221146_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 221536_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 221536_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 221552_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 221552_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 221639_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 221639_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 221659_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 221659_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 221671_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 221671_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 221954_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 221954_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222107_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222107_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222147_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 222147_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 222156_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 222156_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 222185_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222185_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222189_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222189_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222272_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 222272_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 222295_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 222295_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 222307_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222307_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222377_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 222377_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 222579_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222579_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222620_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222620_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222638_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222638_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222641_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222641_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 222842_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 222842_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 222978_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 222978_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223030_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223030_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 223045_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223045_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 223059_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223059_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 223078_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223078_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223104_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223104_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 223160_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223160_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 223234_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223234_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223238_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223238_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 223244_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223244_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 223261_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223261_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 223285_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223285_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 223384_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223384_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 223523_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223523_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223664_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223664_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223685_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223685_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223737_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223737_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223782_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223782_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223787_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223787_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 223795_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223795_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223812_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223812_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223846_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223846_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 223848_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223848_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 223896_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 223896_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 223985_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 223985_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 224003_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 224003_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 224095_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 224095_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 224115_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 224115_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 224158_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 224158_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 224236_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 224236_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 224480_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 224480_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 224496_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 224496_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 224525_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 224525_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 224694_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 224694_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 224783_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 224783_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
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Considering the candidate 224799_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 224799_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 224833_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 224833_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 224916_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 224916_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 224975_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 224975_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 225023_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225023_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225098_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225098_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225231_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225231_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225312_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225312_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225354_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 225354_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 225585_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225585_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225670_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225670_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225675_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 225675_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 225691_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225691_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225695_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225695_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225798_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225798_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225804_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225804_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
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Considering the candidate 225891_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225891_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225895_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225895_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225948_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 225948_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226015_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 226015_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226477_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 226477_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226497_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 226497_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226542_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 226542_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226643_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 226643_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 226738_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 226738_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226777_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 226777_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227133_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 227133_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227252_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 227252_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227503_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 227503_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227577_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 227577_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227653_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 227653_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227769_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 227769_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227841_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 227841_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 227925_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 227925_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228181_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 228181_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 228207_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 228207_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228312_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 228312_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228397_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 228397_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229012_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 229012_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229421_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 229421_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229872_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 229872_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34266_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
Preparing report for the candidate 34266_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32574_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 32574_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47781_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477
The candidate 47781_fd_Cyg-02-Q2b1x1_2026-06-20_05-17-17_20.00sec_5.00C_LIGHT_0477 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 357s
Prepared the HTML report for the field Cyg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:35:51.53 +51:14:27.7
21:27:40.11 +57:16:00.3
21:15:55.75 +54:48:14.3
21:09:14.63 +54:35:04.7
20:58:44.50 +54:58:26.5
21:20:24.89 +53:46:00.6
21:15:00.93 +52:48:20.7
21:28:45.06 +52:13:13.3
21:35:26.37 +53:29:06.7
21:24:45.67 +54:10:57.0
21:31:17.47 +51:25:39.5
21:38:48.17 +54:12:18.2
21:34:28.21 +55:37:27.2
21:36:07.30 +52:33:31.8
21:26:29.43 +49:53:58.3
21:10:39.98 +55:32:47.6
21:35:23.50 +51:40:26.6
21:42:13.87 +57:07:35.2
21:30:23.78 +54:47:04.6
21:18:03.19 +54:36:11.6
21:31:58.61 +50:55:32.5
21:43:07.54 +57:55:26.0
21:18:31.91 +57:59:35.9
20:53:11.08 +49:55:09.3
21:15:33.37 +58:11:01.9
21:39:36.79 +56:01:25.9
20:43:10.69 +55:27:28.7
20:51:34.30 +58:10:50.6
21:41:38.76 +56:10:24.3
20:43:06.81 +53:39:55.0
21:41:58.93 +56:33:06.9
21:16:08.72 +56:47:44.5
21:35:59.50 +50:54:17.5
21:34:20.99 +51:20:57.2
21:37:46.83 +50:47:24.9
21:08:54.08 +57:28:41.9
21:43:00.71 +56:39:42.5
20:45:48.56 +53:45:55.1
20:42:10.48 +53:40:59.9
21:34:03.64 +55:19:03.4
21:25:55.47 +51:51:35.0
20:41:45.44 +57:14:15.4
20:47:48.00 +49:59:53.4
21:10:27.31 +56:35:47.1
20:43:14.80 +54:35:24.9
21:41:34.07 +57:47:39.9
21:37:28.07 +52:54:40.7
20:49:09.56 +54:26:00.7
20:47:43.46 +56:36:18.9
21:37:12.39 +52:31:38.5
21:40:14.50 +53:44:30.6
21:00:31.36 +55:52:32.7
21:28:12.72 +50:38:59.3
21:36:44.66 +55:43:08.2
21:41:17.12 +57:21:52.3
20:51:43.68 +53:51:01.1
21:30:50.18 +49:40:27.8
21:31:36.22 +55:52:52.6
20:45:29.19 +54:37:54.7
21:05:22.56 +54:01:53.9
20:47:42.43 +53:46:00.7
21:34:10.99 +51:07:14.8
20:55:02.11 +54:56:37.9
21:35:32.19 +53:42:41.3
21:37:28.32 +55:01:48.3
21:40:33.19 +53:58:50.4
21:41:26.28 +57:15:39.7
21:03:28.30 +56:47:41.6
21:34:57.10 +55:05:43.9
21:38:40.69 +53:42:12.9
21:35:48.50 +53:28:05.9
21:39:01.38 +56:54:02.1
21:40:14.46 +54:14:13.0
20:44:09.08 +55:47:28.0
20:54:07.45 +57:07:51.8
20:44:10.58 +55:47:53.1
20:50:07.38 +56:46:24.1
21:32:49.84 +51:49:55.0
21:40:16.97 +53:54:37.5
20:49:02.95 +54:34:53.1
21:01:39.26 +57:43:29.9
20:42:11.44 +54:10:24.0
21:33:53.98 +49:34:20.1
20:52:42.71 +57:09:44.3
21:01:36.62 +57:43:17.8
21:34:59.04 +55:36:39.3
20:54:29.12 +57:36:37.1
20:48:12.23 +55:48:05.4
21:12:52.25 +56:22:35.3
20:43:40.80 +54:05:52.8
21:01:45.07 +57:43:15.3
20:40:58.80 +55:28:52.2
21:40:12.38 +53:50:21.9
21:37:56.92 +49:49:27.9
20:39:40.65 +56:25:44.7
20:41:31.86 +55:27:17.0
20:57:24.43 +55:29:49.3
20:59:21.15 +49:49:50.4
20:43:17.40 +53:43:39.8
20:42:33.19 +53:53:06.4
20:40:33.23 +57:27:26.2
21:37:03.49 +55:45:57.3
20:47:50.67 +54:01:23.2
21:37:58.28 +50:06:43.9
20:41:55.03 +54:15:24.5
21:10:24.96 +57:40:50.1
21:17:50.06 +51:34:25.9
20:40:46.42 +57:06:56.9
20:54:10.99 +57:58:40.4
20:48:50.36 +54:57:05.4
20:44:14.80 +51:12:14.1
21:37:04.77 +54:27:27.8
21:39:28.98 +55:45:40.8
20:50:08.35 +51:27:32.2
20:45:48.07 +54:31:17.5
21:38:31.39 +52:12:25.9
21:19:57.47 +54:31:30.9
20:45:50.92 +50:43:17.4
20:54:06.71 +57:16:47.3
20:44:18.87 +54:56:09.3
21:39:34.42 +54:12:55.4
20:59:29.56 +56:44:47.1
20:43:56.36 +51:57:21.7
20:43:13.08 +56:20:13.3
20:43:11.75 +53:44:06.3
20:52:14.53 +57:50:51.6
21:11:15.35 +57:22:19.0
20:38:50.94 +56:09:23.5
20:45:35.17 +54:49:34.2
21:02:25.19 +57:15:09.4
21:41:11.83 +57:32:12.9
20:49:49.16 +54:17:47.6
21:41:59.97 +56:24:24.7
21:26:53.83 +56:11:51.2
20:42:49.38 +51:03:20.7
21:38:30.40 +56:01:58.5
21:41:58.71 +57:00:58.7
20:45:34.99 +50:55:55.9
20:48:31.64 +49:50:50.8
20:55:57.40 +57:25:58.7
21:38:09.72 +56:40:15.8
21:39:19.93 +53:34:33.7
21:30:41.43 +54:20:47.2
21:42:00.41 +56:03:58.6
20:43:56.34 +52:07:36.0
21:41:49.15 +57:27:48.5
21:40:43.97 +56:06:27.2
21:30:52.64 +55:04:37.4
20:50:37.09 +51:04:23.8
20:54:05.86 +50:31:45.1
21:37:20.87 +50:45:30.8
21:35:45.80 +50:08:17.4
20:45:22.70 +49:38:30.2
21:41:13.24 +56:41:17.9
21:39:28.98 +54:00:15.8
21:35:44.23 +50:54:20.2
21:13:15.26 +56:37:38.0
20:58:22.98 +50:33:49.9
20:47:08.15 +49:51:02.7
21:31:23.43 +49:50:50.4
21:24:31.95 +55:13:08.2
21:21:16.67 +53:23:52.0
21:40:57.14 +55:44:06.9
21:41:28.83 +57:46:01.0
21:41:46.40 +57:27:56.1
21:36:50.91 +53:59:43.1
21:29:48.10 +49:50:15.8
21:38:45.74 +54:03:51.3
21:30:11.85 +54:48:00.8
21:29:36.22 +51:19:25.2
21:38:24.11 +50:09:53.6
21:38:01.31 +50:44:21.6
20:49:21.47 +50:31:43.3
########### Completed Cyg-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
21:27:40.11 +57:16:00.3
21:15:55.75 +54:48:14.3
21:09:14.63 +54:35:04.7
20:58:44.50 +54:58:26.5
21:20:24.89 +53:46:00.6
21:15:00.93 +52:48:20.7
21:28:45.06 +52:13:13.3
21:35:26.37 +53:29:06.7
21:35:51.53 +51:14:27.7
21:24:45.67 +54:10:57.0
21:31:17.47 +51:25:39.5
21:38:48.17 +54:12:18.2
21:34:28.21 +55:37:27.2
21:36:07.30 +52:33:31.8
21:26:29.43 +49:53:58.3
21:10:39.98 +55:32:47.6
21:35:23.50 +51:40:26.6
21:42:13.87 +57:07:35.2
21:30:23.78 +54:47:04.6
21:18:03.19 +54:36:11.6
21:31:58.61 +50:55:32.5
21:43:07.54 +57:55:26.0
21:18:31.91 +57:59:35.9
20:53:11.08 +49:55:09.3
21:15:33.37 +58:11:01.9
21:39:36.79 +56:01:25.9
20:43:10.69 +55:27:28.7
20:51:34.30 +58:10:50.6
21:41:38.76 +56:10:24.3
20:43:06.81 +53:39:55.0
21:41:58.93 +56:33:06.9
21:16:08.72 +56:47:44.5
21:35:59.50 +50:54:17.5
21:34:20.99 +51:20:57.2
21:37:46.83 +50:47:24.9
21:08:54.08 +57:28:41.9
21:43:00.71 +56:39:42.5
20:45:48.56 +53:45:55.1
20:42:10.48 +53:40:59.9
21:34:03.64 +55:19:03.4
21:25:55.47 +51:51:35.0
20:41:45.44 +57:14:15.4
20:47:48.00 +49:59:53.4
21:10:27.31 +56:35:47.1
20:43:14.80 +54:35:24.9
21:41:34.07 +57:47:39.9
21:37:28.07 +52:54:40.7
20:49:09.56 +54:26:00.7
20:47:43.46 +56:36:18.9
21:37:12.39 +52:31:38.5
21:40:14.50 +53:44:30.6
21:00:31.36 +55:52:32.7
21:28:12.72 +50:38:59.3
21:36:44.66 +55:43:08.2
21:41:17.12 +57:21:52.3
20:51:43.68 +53:51:01.1
21:30:50.18 +49:40:27.8
21:31:36.22 +55:52:52.6
20:45:29.19 +54:37:54.7
21:05:22.56 +54:01:53.9
20:47:42.43 +53:46:00.7
21:34:10.99 +51:07:14.8
20:55:02.11 +54:56:37.9
21:35:32.19 +53:42:41.3
21:37:28.32 +55:01:48.3
21:40:33.19 +53:58:50.4
21:41:26.28 +57:15:39.7
21:03:28.30 +56:47:41.6
21:34:57.10 +55:05:43.9
21:38:40.69 +53:42:12.9
21:35:48.50 +53:28:05.9
21:39:01.38 +56:54:02.1
21:40:14.46 +54:14:13.0
20:44:09.08 +55:47:28.0
20:54:07.45 +57:07:51.8
20:44:10.58 +55:47:53.1
20:50:07.38 +56:46:24.1
21:32:49.84 +51:49:55.0
21:40:16.97 +53:54:37.5
20:49:02.95 +54:34:53.1
21:01:39.26 +57:43:29.9
20:42:11.44 +54:10:24.0
21:33:53.98 +49:34:20.1
20:52:42.71 +57:09:44.3
21:01:36.62 +57:43:17.8
21:34:59.04 +55:36:39.3
20:54:29.12 +57:36:37.1
20:48:12.23 +55:48:05.4
21:12:52.25 +56:22:35.3
20:43:40.80 +54:05:52.8
21:01:45.07 +57:43:15.3
20:40:58.80 +55:28:52.2
21:40:12.38 +53:50:21.9
21:37:56.92 +49:49:27.9
20:39:40.65 +56:25:44.7
20:41:31.86 +55:27:17.0
20:57:24.43 +55:29:49.3
20:59:21.15 +49:49:50.4
20:43:17.40 +53:43:39.8
20:42:33.19 +53:53:06.4
20:40:33.23 +57:27:26.2
21:37:03.49 +55:45:57.3
20:47:50.67 +54:01:23.2
21:37:58.28 +50:06:43.9
20:41:55.03 +54:15:24.5
21:10:24.96 +57:40:50.1
21:17:50.06 +51:34:25.9
20:40:46.42 +57:06:56.9
20:54:10.99 +57:58:40.4
20:48:50.36 +54:57:05.4
20:44:14.80 +51:12:14.1
21:37:04.77 +54:27:27.8
21:39:28.98 +55:45:40.8
20:50:08.35 +51:27:32.2
20:45:48.07 +54:31:17.5
21:38:31.39 +52:12:25.9
21:19:57.47 +54:31:30.9
20:45:50.92 +50:43:17.4
20:54:06.71 +57:16:47.3
20:44:18.87 +54:56:09.3
21:39:34.42 +54:12:55.4
20:59:29.56 +56:44:47.1
20:43:56.36 +51:57:21.7
20:43:13.08 +56:20:13.3
20:43:11.75 +53:44:06.3
20:52:14.53 +57:50:51.6
21:11:15.35 +57:22:19.0
20:38:50.94 +56:09:23.5
20:45:35.17 +54:49:34.2
21:02:25.19 +57:15:09.4
21:41:11.83 +57:32:12.9
20:49:49.16 +54:17:47.6
21:41:59.97 +56:24:24.7
21:26:53.83 +56:11:51.2
20:42:49.38 +51:03:20.7
21:38:30.40 +56:01:58.5
21:41:58.71 +57:00:58.7
20:45:34.99 +50:55:55.9
20:48:31.64 +49:50:50.8
20:55:57.40 +57:25:58.7
21:38:09.72 +56:40:15.8
21:39:19.93 +53:34:33.7
21:30:41.43 +54:20:47.2
21:42:00.41 +56:03:58.6
20:43:56.34 +52:07:36.0
21:41:49.15 +57:27:48.5
21:40:43.97 +56:06:27.2
21:30:52.64 +55:04:37.4
20:50:37.09 +51:04:23.8
20:54:05.86 +50:31:45.1
21:37:20.87 +50:45:30.8
21:35:45.80 +50:08:17.4
20:45:22.70 +49:38:30.2
21:41:13.24 +56:41:17.9
21:39:28.98 +54:00:15.8
21:35:44.23 +50:54:20.2
21:13:15.26 +56:37:38.0
20:58:22.98 +50:33:49.9
20:47:08.15 +49:51:02.7
21:31:23.43 +49:50:50.4
21:24:31.95 +55:13:08.2
21:21:16.67 +53:23:52.0
21:40:57.14 +55:44:06.9
21:41:28.83 +57:46:01.0
21:41:46.40 +57:27:56.1
21:36:50.91 +53:59:43.1
21:29:48.10 +49:50:15.8
21:38:45.74 +54:03:51.3
21:30:11.85 +54:48:00.8
21:29:36.22 +51:19:25.2
21:38:24.11 +50:09:53.6
21:38:01.31 +50:44:21.6
20:49:21.47 +50:31:43.3
###################################################################################
21:27:40.11 +57:16:00.3 -- not an asteroid (will add it to exclusion list)
21:15:55.75 +54:48:14.3 -- not an asteroid (will add it to exclusion list)
21:09:14.63 +54:35:04.7 -- not an asteroid (will add it to exclusion list)
20:58:44.50 +54:58:26.5 -- not an asteroid (will add it to exclusion list)
21:20:24.89 +53:46:00.6 -- not an asteroid (will add it to exclusion list)
21:15:00.93 +52:48:20.7 -- not an asteroid (will add it to exclusion list)
21:28:45.06 +52:13:13.3 -- not an asteroid (will add it to exclusion list)
21:35:26.37 +53:29:06.7 -- not an asteroid (will add it to exclusion list)
21:35:51.53 +51:14:27.7 -- not an asteroid (will add it to exclusion list)
21:24:45.67 +54:10:57.0 -- not an asteroid (will add it to exclusion list)
21:31:17.47 +51:25:39.5 -- not an asteroid (will add it to exclusion list)
21:38:48.17 +54:12:18.2 -- not an asteroid (will add it to exclusion list)
21:34:28.21 +55:37:27.2 -- not an asteroid (will add it to exclusion list)
21:36:07.30 +52:33:31.8 -- not an asteroid (will add it to exclusion list)
21:26:29.43 +49:53:58.3 -- not an asteroid (will add it to exclusion list)
21:10:39.98 +55:32:47.6 -- not an asteroid (will add it to exclusion list)
21:35:23.50 +51:40:26.6 -- not an asteroid (will add it to exclusion list)
21:42:13.87 +57:07:35.2 -- not an asteroid (will add it to exclusion list)
21:30:23.78 +54:47:04.6 -- not an asteroid (will add it to exclusion list)
21:18:03.19 +54:36:11.6 -- not an asteroid (will add it to exclusion list)
21:31:58.61 +50:55:32.5 -- not an asteroid (will add it to exclusion list)
21:43:07.54 +57:55:26.0 -- not an asteroid (will add it to exclusion list)
21:18:31.91 +57:59:35.9 -- not an asteroid (will add it to exclusion list)
20:53:11.08 +49:55:09.3 -- not an asteroid (will add it to exclusion list)
21:15:33.37 +58:11:01.9 -- not an asteroid (will add it to exclusion list)
21:39:36.79 +56:01:25.9 -- not an asteroid (will add it to exclusion list)
20:43:10.69 +55:27:28.7 -- not an asteroid (will add it to exclusion list)
20:51:34.30 +58:10:50.6 -- not an asteroid (will add it to exclusion list)
21:41:38.76 +56:10:24.3 -- not an asteroid (will add it to exclusion list)
20:43:06.81 +53:39:55.0 -- not an asteroid (will add it to exclusion list)
21:41:58.93 +56:33:06.9 -- not an asteroid (will add it to exclusion list)
21:16:08.72 +56:47:44.5 -- not an asteroid (will add it to exclusion list)
21:35:59.50 +50:54:17.5 -- not an asteroid (will add it to exclusion list)
21:34:20.99 +51:20:57.2 -- not an asteroid (will add it to exclusion list)
21:37:46.83 +50:47:24.9 -- not an asteroid (will add it to exclusion list)
21:08:54.08 +57:28:41.9 -- not an asteroid (will add it to exclusion list)
21:43:00.71 +56:39:42.5 -- not an asteroid (will add it to exclusion list)
20:45:48.56 +53:45:55.1 -- not an asteroid (will add it to exclusion list)
20:42:10.48 +53:40:59.9 -- not an asteroid (will add it to exclusion list)
21:34:03.64 +55:19:03.4 -- not an asteroid (will add it to exclusion list)
21:25:55.47 +51:51:35.0 -- not an asteroid (will add it to exclusion list)
20:41:45.44 +57:14:15.4 -- not an asteroid (will add it to exclusion list)
20:47:48.00 +49:59:53.4 -- not an asteroid (will add it to exclusion list)
21:10:27.31 +56:35:47.1 -- not an asteroid (will add it to exclusion list)
20:43:14.80 +54:35:24.9 -- not an asteroid (will add it to exclusion list)
21:41:34.07 +57:47:39.9 -- not an asteroid (will add it to exclusion list)
21:37:28.07 +52:54:40.7 -- not an asteroid (will add it to exclusion list)
20:49:09.56 +54:26:00.7 -- not an asteroid (will add it to exclusion list)
20:47:43.46 +56:36:18.9 -- not an asteroid (will add it to exclusion list)
21:37:12.39 +52:31:38.5 -- not an asteroid (will add it to exclusion list)
21:40:14.50 +53:44:30.6 -- not an asteroid (will add it to exclusion list)
21:00:31.36 +55:52:32.7 -- not an asteroid (will add it to exclusion list)
21:28:12.72 +50:38:59.3 -- not an asteroid (will add it to exclusion list)
21:36:44.66 +55:43:08.2 -- not an asteroid (will add it to exclusion list)
21:41:17.12 +57:21:52.3 -- not an asteroid (will add it to exclusion list)
20:51:43.68 +53:51:01.1 -- not an asteroid (will add it to exclusion list)
21:30:50.18 +49:40:27.8 -- not an asteroid (will add it to exclusion list)
21:31:36.22 +55:52:52.6 -- not an asteroid (will add it to exclusion list)
20:45:29.19 +54:37:54.7 -- not an asteroid (will add it to exclusion list)
21:05:22.56 +54:01:53.9 -- not an asteroid (will add it to exclusion list)
20:47:42.43 +53:46:00.7 -- not an asteroid (will add it to exclusion list)
21:34:10.99 +51:07:14.8 -- not an asteroid (will add it to exclusion list)
20:55:02.11 +54:56:37.9 -- not an asteroid (will add it to exclusion list)
21:35:32.19 +53:42:41.3 -- not an asteroid (will add it to exclusion list)
21:37:28.32 +55:01:48.3 -- not an asteroid (will add it to exclusion list)
21:40:33.19 +53:58:50.4 -- not an asteroid (will add it to exclusion list)
21:41:26.28 +57:15:39.7 -- not an asteroid (will add it to exclusion list)
21:03:28.30 +56:47:41.6 -- not an asteroid (will add it to exclusion list)
21:34:57.10 +55:05:43.9 -- not an asteroid (will add it to exclusion list)
21:38:40.69 +53:42:12.9 -- not an asteroid (will add it to exclusion list)
21:35:48.50 +53:28:05.9 -- not an asteroid (will add it to exclusion list)
21:39:01.38 +56:54:02.1 -- not an asteroid (will add it to exclusion list)
21:40:14.46 +54:14:13.0 -- not an asteroid (will add it to exclusion list)
20:44:09.08 +55:47:28.0 -- not an asteroid (will add it to exclusion list)
20:54:07.45 +57:07:51.8 -- not an asteroid (will add it to exclusion list)
20:44:10.58 +55:47:53.1 -- not an asteroid (will add it to exclusion list)
20:50:07.38 +56:46:24.1 -- not an asteroid (will add it to exclusion list)
21:32:49.84 +51:49:55.0 -- not an asteroid (will add it to exclusion list)
21:40:16.97 +53:54:37.5 -- not an asteroid (will add it to exclusion list)
20:49:02.95 +54:34:53.1 -- not an asteroid (will add it to exclusion list)
21:01:39.26 +57:43:29.9 -- not an asteroid (will add it to exclusion list)
20:42:11.44 +54:10:24.0 -- not an asteroid (will add it to exclusion list)
21:33:53.98 +49:34:20.1 -- not an asteroid (will add it to exclusion list)
20:52:42.71 +57:09:44.3 -- not an asteroid (will add it to exclusion list)
21:01:36.62 +57:43:17.8 -- not an asteroid (will add it to exclusion list)
21:34:59.04 +55:36:39.3 -- not an asteroid (will add it to exclusion list)
20:54:29.12 +57:36:37.1 -- not an asteroid (will add it to exclusion list)
20:48:12.23 +55:48:05.4 -- not an asteroid (will add it to exclusion list)
21:12:52.25 +56:22:35.3 -- not an asteroid (will add it to exclusion list)
20:43:40.80 +54:05:52.8 -- not an asteroid (will add it to exclusion list)
21:01:45.07 +57:43:15.3 -- not an asteroid (will add it to exclusion list)
20:40:58.80 +55:28:52.2 -- not an asteroid (will add it to exclusion list)
21:40:12.38 +53:50:21.9 -- not an asteroid (will add it to exclusion list)
21:37:56.92 +49:49:27.9 -- not an asteroid (will add it to exclusion list)
20:39:40.65 +56:25:44.7 -- not an asteroid (will add it to exclusion list)
20:41:31.86 +55:27:17.0 -- not an asteroid (will add it to exclusion list)
20:57:24.43 +55:29:49.3 -- not an asteroid (will add it to exclusion list)
20:59:21.15 +49:49:50.4 -- not an asteroid (will add it to exclusion list)
20:43:17.40 +53:43:39.8 -- not an asteroid (will add it to exclusion list)
20:42:33.19 +53:53:06.4 -- not an asteroid (will add it to exclusion list)
20:40:33.23 +57:27:26.2 -- not an asteroid (will add it to exclusion list)
21:37:03.49 +55:45:57.3 -- not an asteroid (will add it to exclusion list)
20:47:50.67 +54:01:23.2 -- not an asteroid (will add it to exclusion list)
21:37:58.28 +50:06:43.9 -- not an asteroid (will add it to exclusion list)
20:41:55.03 +54:15:24.5 -- not an asteroid (will add it to exclusion list)
21:10:24.96 +57:40:50.1 -- not an asteroid (will add it to exclusion list)
21:17:50.06 +51:34:25.9 -- not an asteroid (will add it to exclusion list)
20:40:46.42 +57:06:56.9 -- not an asteroid (will add it to exclusion list)
20:54:10.99 +57:58:40.4 -- not an asteroid (will add it to exclusion list)
20:48:50.36 +54:57:05.4 -- not an asteroid (will add it to exclusion list)
20:44:14.80 +51:12:14.1 -- not an asteroid (will add it to exclusion list)
21:37:04.77 +54:27:27.8 -- not an asteroid (will add it to exclusion list)
21:39:28.98 +55:45:40.8 -- not an asteroid (will add it to exclusion list)
20:50:08.35 +51:27:32.2 -- not an asteroid (will add it to exclusion list)
20:45:48.07 +54:31:17.5 -- not an asteroid (will add it to exclusion list)
21:38:31.39 +52:12:25.9 -- not an asteroid (will add it to exclusion list)
21:19:57.47 +54:31:30.9 -- not an asteroid (will add it to exclusion list)
20:45:50.92 +50:43:17.4 -- not an asteroid (will add it to exclusion list)
20:54:06.71 +57:16:47.3 -- not an asteroid (will add it to exclusion list)
20:44:18.87 +54:56:09.3 -- not an asteroid (will add it to exclusion list)
21:39:34.42 +54:12:55.4 -- not an asteroid (will add it to exclusion list)
20:59:29.56 +56:44:47.1 -- not an asteroid (will add it to exclusion list)
20:43:56.36 +51:57:21.7 -- not an asteroid (will add it to exclusion list)
20:43:13.08 +56:20:13.3 -- not an asteroid (will add it to exclusion list)
20:43:11.75 +53:44:06.3 -- not an asteroid (will add it to exclusion list)
20:52:14.53 +57:50:51.6 -- not an asteroid (will add it to exclusion list)
21:11:15.35 +57:22:19.0 -- not an asteroid (will add it to exclusion list)
20:38:50.94 +56:09:23.5 -- not an asteroid (will add it to exclusion list)
20:45:35.17 +54:49:34.2 -- not an asteroid (will add it to exclusion list)
21:02:25.19 +57:15:09.4 -- not an asteroid (will add it to exclusion list)
21:41:11.83 +57:32:12.9 -- not an asteroid (will add it to exclusion list)
20:49:49.16 +54:17:47.6 -- not an asteroid (will add it to exclusion list)
21:41:59.97 +56:24:24.7 -- not an asteroid (will add it to exclusion list)
21:26:53.83 +56:11:51.2 -- not an asteroid (will add it to exclusion list)
20:42:49.38 +51:03:20.7 -- not an asteroid (will add it to exclusion list)
21:38:30.40 +56:01:58.5 -- not an asteroid (will add it to exclusion list)
21:41:58.71 +57:00:58.7 -- not an asteroid (will add it to exclusion list)
20:45:34.99 +50:55:55.9 -- not an asteroid (will add it to exclusion list)
20:48:31.64 +49:50:50.8 -- not an asteroid (will add it to exclusion list)
20:55:57.40 +57:25:58.7 -- not an asteroid (will add it to exclusion list)
21:38:09.72 +56:40:15.8 -- not an asteroid (will add it to exclusion list)
21:39:19.93 +53:34:33.7 -- not an asteroid (will add it to exclusion list)
21:30:41.43 +54:20:47.2 -- not an asteroid (will add it to exclusion list)
21:42:00.41 +56:03:58.6 -- not an asteroid (will add it to exclusion list)
20:43:56.34 +52:07:36.0 -- not an asteroid (will add it to exclusion list)
21:41:49.15 +57:27:48.5 -- not an asteroid (will add it to exclusion list)
21:40:43.97 +56:06:27.2 -- not an asteroid (will add it to exclusion list)
21:30:52.64 +55:04:37.4 -- not an asteroid (will add it to exclusion list)
20:50:37.09 +51:04:23.8 -- not an asteroid (will add it to exclusion list)
20:54:05.86 +50:31:45.1 -- not an asteroid (will add it to exclusion list)
21:37:20.87 +50:45:30.8 -- not an asteroid (will add it to exclusion list)
21:35:45.80 +50:08:17.4 -- not an asteroid (will add it to exclusion list)
20:45:22.70 +49:38:30.2 -- not an asteroid (will add it to exclusion list)
21:41:13.24 +56:41:17.9 -- not an asteroid (will add it to exclusion list)
21:39:28.98 +54:00:15.8 -- not an asteroid (will add it to exclusion list)
21:35:44.23 +50:54:20.2 -- not an asteroid (will add it to exclusion list)
21:13:15.26 +56:37:38.0 -- not an asteroid (will add it to exclusion list)
20:58:22.98 +50:33:49.9 -- not an asteroid (will add it to exclusion list)
20:47:08.15 +49:51:02.7 -- not an asteroid (will add it to exclusion list)
21:31:23.43 +49:50:50.4 -- not an asteroid (will add it to exclusion list)
21:24:31.95 +55:13:08.2 -- not an asteroid (will add it to exclusion list)
21:21:16.67 +53:23:52.0 -- not an asteroid (will add it to exclusion list)
21:40:57.14 +55:44:06.9 -- not an asteroid (will add it to exclusion list)
21:41:28.83 +57:46:01.0 -- not an asteroid (will add it to exclusion list)
21:41:46.40 +57:27:56.1 -- not an asteroid (will add it to exclusion list)
21:36:50.91 +53:59:43.1 -- not an asteroid (will add it to exclusion list)
21:29:48.10 +49:50:15.8 -- not an asteroid (will add it to exclusion list)
21:38:45.74 +54:03:51.3 -- not an asteroid (will add it to exclusion list)
21:30:11.85 +54:48:00.8 -- not an asteroid (will add it to exclusion list)
21:29:36.22 +51:19:25.2 -- not an asteroid (will add it to exclusion list)
21:38:24.11 +50:09:53.6 -- not an asteroid (will add it to exclusion list)
21:38:01.31 +50:44:21.6 -- not an asteroid (will add it to exclusion list)
20:49:21.47 +50:31:43.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:38:50.94 +56:09:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:40.65 +56:25:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:33.23 +57:27:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:46.42 +57:06:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:58.80 +55:28:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:31.86 +55:27:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:45.44 +57:14:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:55.03 +54:15:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:10.48 +53:40:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:11.44 +54:10:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:33.19 +53:53:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:49.38 +51:03:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:06.81 +53:39:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:10.69 +55:27:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:11.75 +53:44:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:13.08 +56:20:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:14.80 +54:35:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:17.40 +53:43:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:40.80 +54:05:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:56.34 +52:07:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:56.36 +51:57:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:09.08 +55:47:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:10.58 +55:47:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:14.80 +51:12:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:18.87 +54:56:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:22.70 +49:38:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:29.19 +54:37:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:34.99 +50:55:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:35.17 +54:49:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:48.07 +54:31:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:48.56 +53:45:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:50.92 +50:43:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:08.15 +49:51:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:42.43 +53:46:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:43.46 +56:36:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:48.00 +49:59:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:50.67 +54:01:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:12.23 +55:48:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:31.64 +49:50:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:50.36 +54:57:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:02.95 +54:34:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:09.56 +54:26:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:21.47 +50:31:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:49.16 +54:17:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:07.38 +56:46:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:08.35 +51:27:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:37.09 +51:04:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:34.30 +58:10:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:43.68 +53:51:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:14.53 +57:50:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:42.71 +57:09:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:11.08 +49:55:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:05.86 +50:31:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:06.71 +57:16:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:07.45 +57:07:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:10.99 +57:58:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:29.12 +57:36:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:02.11 +54:56:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:57.40 +57:25:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:24.43 +55:29:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:22.98 +50:33:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:44.50 +54:58:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:21.15 +49:49:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:29.56 +56:44:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:31.36 +55:52:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:36.62 +57:43:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:39.26 +57:43:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:45.07 +57:43:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:25.19 +57:15:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:28.30 +56:47:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:22.56 +54:01:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:54.08 +57:28:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:14.63 +54:35:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:24.96 +57:40:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:27.31 +56:35:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:10:39.98 +55:32:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:15.35 +57:22:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:52.25 +56:22:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:15.26 +56:37:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:00.93 +52:48:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:33.37 +58:11:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:55.75 +54:48:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:16:08.72 +56:47:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:17:50.06 +51:34:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:03.19 +54:36:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:18:31.91 +57:59:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:19:57.47 +54:31:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:20:24.89 +53:46:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:16.67 +53:23:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:31.95 +55:13:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:45.67 +54:10:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:55.47 +51:51:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:29.43 +49:53:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:53.83 +56:11:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:40.11 +57:16:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:12.72 +50:38:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:45.06 +52:13:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:36.22 +51:19:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:29:48.10 +49:50:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:11.85 +54:48:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:23.78 +54:47:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:41.43 +54:20:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:50.18 +49:40:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:52.64 +55:04:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:17.47 +51:25:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:23.43 +49:50:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:36.22 +55:52:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:31:58.61 +50:55:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:32:49.84 +51:49:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:33:53.98 +49:34:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:03.64 +55:19:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:10.99 +51:07:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:20.99 +51:20:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:28.21 +55:37:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:57.10 +55:05:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:59.04 +55:36:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:23.50 +51:40:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:26.37 +53:29:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:32.19 +53:42:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:44.23 +50:54:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:45.80 +50:08:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:48.50 +53:28:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:51.53 +51:14:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:59.50 +50:54:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:07.30 +52:33:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:44.66 +55:43:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:50.91 +53:59:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:03.49 +55:45:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:04.77 +54:27:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:12.39 +52:31:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:20.87 +50:45:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:28.07 +52:54:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:28.32 +55:01:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:46.83 +50:47:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:56.92 +49:49:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:58.28 +50:06:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:01.31 +50:44:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:09.72 +56:40:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:24.11 +50:09:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:30.40 +56:01:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:31.39 +52:12:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:40.69 +53:42:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:45.74 +54:03:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:48.17 +54:12:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:01.38 +56:54:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:19.93 +53:34:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:28.98 +54:00:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:28.98 +55:45:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:34.42 +54:12:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:36.79 +56:01:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:12.38 +53:50:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:14.46 +54:14:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:14.50 +53:44:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:16.97 +53:54:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:33.19 +53:58:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.97 +56:06:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:57.14 +55:44:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:11.83 +57:32:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:13.24 +56:41:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:17.12 +57:21:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:26.28 +57:15:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:28.83 +57:46:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:34.07 +57:47:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:38.76 +56:10:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:46.40 +57:27:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:49.15 +57:27:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:58.71 +57:00:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:58.93 +56:33:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:59.97 +56:24:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:00.41 +56:03:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:13.87 +57:07:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:00.71 +56:39:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:07.54 +57:55:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
20:38:50.94 +56:09:23.5 -- not a known variable star
20:39:40.65 +56:25:44.7 -- not a known variable star
20:40:33.23 +57:27:26.2 -- not a known variable star
20:40:46.42 +57:06:56.9 -- not a known variable star
20:40:58.80 +55:28:52.2 -- not a known variable star
20:41:31.86 +55:27:17.0 -- not a known variable star
20:41:45.44 +57:14:15.4 -- not a known variable star
20:41:55.03 +54:15:24.5 -- not a known variable star
20:42:10.48 +53:40:59.9 -- not a known variable star
20:42:11.44 +54:10:24.0 -- not a known variable star
20:42:33.19 +53:53:06.4 -- not a known variable star
20:42:49.38 +51:03:20.7 -- not a known variable star
20:43:06.81 +53:39:55.0 -- not a known variable star
20:43:10.69 +55:27:28.7 -- not a known variable star
20:43:11.75 +53:44:06.3 -- not a known variable star
20:43:13.08 +56:20:13.3 -- not a known variable star
20:43:14.80 +54:35:24.9 -- a known variable star
20:43:17.40 +53:43:39.8 -- not a known variable star
20:43:40.80 +54:05:52.8 -- not a known variable star
20:43:56.34 +52:07:36.0 -- not a known variable star
20:43:56.36 +51:57:21.7 -- not a known variable star
20:44:09.08 +55:47:28.0 -- not a known variable star
20:44:10.58 +55:47:53.1 -- not a known variable star
20:44:14.80 +51:12:14.1 -- not a known variable star
20:44:18.87 +54:56:09.3 -- not a known variable star
20:45:22.70 +49:38:30.2 -- not a known variable star
20:45:29.19 +54:37:54.7 -- not a known variable star
20:45:34.99 +50:55:55.9 -- not a known variable star
20:45:35.17 +54:49:34.2 -- not a known variable star
20:45:48.07 +54:31:17.5 -- not a known variable star
20:45:48.56 +53:45:55.1 -- not a known variable star
20:45:50.92 +50:43:17.4 -- not a known variable star
20:47:08.15 +49:51:02.7 -- not a known variable star
20:47:42.43 +53:46:00.7 -- not a known variable star
20:47:43.46 +56:36:18.9 -- not a known variable star
20:47:48.00 +49:59:53.4 -- a known variable star
20:47:50.67 +54:01:23.2 -- not a known variable star
20:48:12.23 +55:48:05.4 -- not a known variable star
20:48:31.64 +49:50:50.8 -- not a known variable star
20:48:50.36 +54:57:05.4 -- not a known variable star
20:49:02.95 +54:34:53.1 -- not a known variable star
20:49:09.56 +54:26:00.7 -- not a known variable star
20:49:21.47 +50:31:43.3 -- a known variable star
20:49:49.16 +54:17:47.6 -- not a known variable star
20:50:07.38 +56:46:24.1 -- not a known variable star
20:50:08.35 +51:27:32.2 -- a known variable star
20:50:37.09 +51:04:23.8 -- not a known variable star
20:51:34.30 +58:10:50.6 -- a known variable star
20:51:43.68 +53:51:01.1 -- not a known variable star
20:52:14.53 +57:50:51.6 -- not a known variable star
20:52:42.71 +57:09:44.3 -- not a known variable star
20:53:11.08 +49:55:09.3 -- not a known variable star
20:54:05.86 +50:31:45.1 -- not a known variable star
20:54:06.71 +57:16:47.3 -- not a known variable star
20:54:07.45 +57:07:51.8 -- not a known variable star
20:54:10.99 +57:58:40.4 -- not a known variable star
20:54:29.12 +57:36:37.1 -- not a known variable star
20:55:02.11 +54:56:37.9 -- not a known variable star
20:55:57.40 +57:25:58.7 -- not a known variable star
20:57:24.43 +55:29:49.3 -- not a known variable star
20:58:22.98 +50:33:49.9 -- not a known variable star
20:58:44.50 +54:58:26.5 -- not a known variable star
20:59:21.15 +49:49:50.4 -- not a known variable star
20:59:29.56 +56:44:47.1 -- not a known variable star
21:00:31.36 +55:52:32.7 -- not a known variable star
21:01:36.62 +57:43:17.8 -- not a known variable star
21:01:39.26 +57:43:29.9 -- not a known variable star
21:01:45.07 +57:43:15.3 -- not a known variable star
21:02:25.19 +57:15:09.4 -- a known variable star
21:03:28.30 +56:47:41.6 -- a known variable star
21:05:22.56 +54:01:53.9 -- not a known variable star
21:08:54.08 +57:28:41.9 -- not a known variable star
21:09:14.63 +54:35:04.7 -- not a known variable star
21:10:24.96 +57:40:50.1 -- not a known variable star
21:10:27.31 +56:35:47.1 -- not a known variable star
21:10:39.98 +55:32:47.6 -- not a known variable star
21:11:15.35 +57:22:19.0 -- not a known variable star
21:12:52.25 +56:22:35.3 -- not a known variable star
21:13:15.26 +56:37:38.0 -- not a known variable star
21:15:00.93 +52:48:20.7 -- not a known variable star
21:15:33.37 +58:11:01.9 -- not a known variable star
21:15:55.75 +54:48:14.3 -- not a known variable star
21:16:08.72 +56:47:44.5 -- not a known variable star
21:17:50.06 +51:34:25.9 -- not a known variable star
21:18:03.19 +54:36:11.6 -- not a known variable star
21:18:31.91 +57:59:35.9 -- not a known variable star
21:19:57.47 +54:31:30.9 -- not a known variable star
21:20:24.89 +53:46:00.6 -- not a known variable star
21:21:16.67 +53:23:52.0 -- not a known variable star
21:24:31.95 +55:13:08.2 -- not a known variable star
21:24:45.67 +54:10:57.0 -- not a known variable star
21:25:55.47 +51:51:35.0 -- not a known variable star
21:26:29.43 +49:53:58.3 -- not a known variable star
21:26:53.83 +56:11:51.2 -- not a known variable star
21:27:40.11 +57:16:00.3 -- not a known variable star
21:28:12.72 +50:38:59.3 -- not a known variable star
21:28:45.06 +52:13:13.3 -- not a known variable star
21:29:36.22 +51:19:25.2 -- not a known variable star
21:29:48.10 +49:50:15.8 -- not a known variable star
21:30:11.85 +54:48:00.8 -- not a known variable star
21:30:23.78 +54:47:04.6 -- not a known variable star
21:30:41.43 +54:20:47.2 -- not a known variable star
21:30:50.18 +49:40:27.8 -- not a known variable star
21:30:52.64 +55:04:37.4 -- not a known variable star
21:31:17.47 +51:25:39.5 -- a known variable star
21:31:23.43 +49:50:50.4 -- not a known variable star
21:31:36.22 +55:52:52.6 -- not a known variable star
21:31:58.61 +50:55:32.5 -- not a known variable star
21:32:49.84 +51:49:55.0 -- not a known variable star
21:33:53.98 +49:34:20.1 -- not a known variable star
21:34:03.64 +55:19:03.4 -- not a known variable star
21:34:10.99 +51:07:14.8 -- not a known variable star
21:34:20.99 +51:20:57.2 -- a known variable star
21:34:28.21 +55:37:27.2 -- not a known variable star
21:34:57.10 +55:05:43.9 -- not a known variable star
21:34:59.04 +55:36:39.3 -- not a known variable star
21:35:23.50 +51:40:26.6 -- not a known variable star
21:35:26.37 +53:29:06.7 -- a known variable star
21:35:32.19 +53:42:41.3 -- not a known variable star
21:35:44.23 +50:54:20.2 -- not a known variable star
21:35:45.80 +50:08:17.4 -- a known variable star
21:35:48.50 +53:28:05.9 -- a known variable star
21:35:51.53 +51:14:27.7 -- a known variable star
21:35:59.50 +50:54:17.5 -- not a known variable star
21:36:07.30 +52:33:31.8 -- a known variable star
21:36:44.66 +55:43:08.2 -- not a known variable star
21:36:50.91 +53:59:43.1 -- not a known variable star
21:37:03.49 +55:45:57.3 -- a known variable star
21:37:04.77 +54:27:27.8 -- not a known variable star
21:37:12.39 +52:31:38.5 -- not a known variable star
21:37:20.87 +50:45:30.8 -- not a known variable star
21:37:28.07 +52:54:40.7 -- not a known variable star
21:37:28.32 +55:01:48.3 -- not a known variable star
21:37:46.83 +50:47:24.9 -- not a known variable star
21:37:56.92 +49:49:27.9 -- not a known variable star
21:37:58.28 +50:06:43.9 -- not a known variable star
21:38:01.31 +50:44:21.6 -- not a known variable star
21:38:09.72 +56:40:15.8 -- not a known variable star
21:38:24.11 +50:09:53.6 -- a known variable star
21:38:30.40 +56:01:58.5 -- not a known variable star
21:38:31.39 +52:12:25.9 -- not a known variable star
21:38:40.69 +53:42:12.9 -- not a known variable star
21:38:45.74 +54:03:51.3 -- not a known variable star
21:38:48.17 +54:12:18.2 -- not a known variable star
21:39:01.38 +56:54:02.1 -- not a known variable star
21:39:19.93 +53:34:33.7 -- not a known variable star
21:39:28.98 +54:00:15.8 -- not a known variable star
21:39:28.98 +55:45:40.8 -- not a known variable star
21:39:34.42 +54:12:55.4 -- not a known variable star
21:39:36.79 +56:01:25.9 -- not a known variable star
21:40:12.38 +53:50:21.9 -- not a known variable star
21:40:14.46 +54:14:13.0 -- not a known variable star
21:40:14.50 +53:44:30.6 -- not a known variable star
21:40:16.97 +53:54:37.5 -- not a known variable star
21:40:33.19 +53:58:50.4 -- not a known variable star
21:40:43.97 +56:06:27.2 -- not a known variable star
21:40:57.14 +55:44:06.9 -- not a known variable star
21:41:11.83 +57:32:12.9 -- not a known variable star
21:41:13.24 +56:41:17.9 -- not a known variable star
21:41:17.12 +57:21:52.3 -- not a known variable star
21:41:26.28 +57:15:39.7 -- not a known variable star
21:41:28.83 +57:46:01.0 -- not a known variable star
21:41:34.07 +57:47:39.9 -- not a known variable star
21:41:38.76 +56:10:24.3 -- a known variable star
21:41:46.40 +57:27:56.1 -- not a known variable star
21:41:49.15 +57:27:48.5 -- not a known variable star
21:41:58.71 +57:00:58.7 -- not a known variable star
21:41:58.93 +56:33:06.9 -- not a known variable star
21:41:59.97 +56:24:24.7 -- a known variable star
21:42:00.41 +56:03:58.6 -- not a known variable star
21:42:13.87 +57:07:35.2 -- not a known variable star
21:43:00.71 +56:39:42.5 -- not a known variable star
21:43:07.54 +57:55:26.0 -- not a known variable star
Found 155 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
173 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 173 (excluding asteroids and hot pixels, 155 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461211.92814424 -observatory V36
07:37:52.61 +21:39:38.3 Mercury (0.9mag)
08:42:42.86 +20:15:47.1 Venus (-4.0mag)
03:25:21.14 +18:15:48.5 Mars (1.3mag)
07:58:53.10 +21:03:58.0 Jupiter (-1.8mag)
00:52:29.73 +03:05:10.3 Saturn (0.8mag)
04:03:03.04 +20:33:32.3 Uranus (5.8mag)
00:16:43.09 +00:19:51.0 Neptune (7.8mag)
20:32:34.24 -23:09:23.9 Pluto (14.5mag)
10:46:21.65 +06:11:28.0 Moon (-9.9mag)
-rw-r--r-- 1 apache apache 361 Jun 20 06:51 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461211.92814424:
07:58:50.76 +21:04:07.6 Io (6.2mag)
07:58:58.95 +21:03:37.9 Europa (6.3mag)
07:59:00.77 +21:03:29.0 Ganymede (5.6mag)
07:59:16.13 +21:02:48.8 Callisto (6.9mag)
07:58:27.20 +20:41:56.1 Himalia (15.6mag)
07:58:56.85 +21:03:45.4 Thebe (16.6mag)
07:58:06.83 +20:52:21.5 Elara (17.6mag)
08:01:39.36 +21:08:58.4 Pasiphae (17.8mag)
08:04:54.16 +21:06:42.6 Carme (18.9mag)
00:52:23.99 +03:05:39.1 Titan (8.6mag)
00:52:34.25 +03:05:14.3 Rhea (9.9mag)
00:52:43.53 +03:07:33.0 Iapetus (11.3mag)
00:52:33.03 +03:05:38.7 Hyperion (14.6mag)
00:52:56.62 +03:05:19.9 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jun 20 06:51 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461211.92814424:
17:28:20.70 -35:29:45.8 JWST
18:34:23.74 +21:02:07.0 Chandra
04:29:43.86 +53:16:57.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 20 06:51 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461211.92814424 -observatory V36
18:34:14.67 -33:28:20.7 13.6mag P/2010 H2 (Vales)
06:05:38.60 -67:59:41.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:53:35.43 +32:08:08.7 17.6mag C/2017 K2 (PANSTARRS)
17:09:53.83 +15:49:48.9 17.9mag C/2021 G2 (ATLAS)
23:13:46.10 -35:56:26.8 15.9mag P/2021 N1 (ZTF)
23:09:04.61 +31:59:52.5 17.2mag C/2022 E2 (ATLAS)
05:48:56.26 +27:00:44.4 16.6mag C/2022 N2 (PANSTARRS)
09:38:57.42 +30:37:31.1 16.7mag C/2022 QE78 (ATLAS)
08:57:25.53 +04:26:48.8 17.7mag C/2022 R6 (PANSTARRS)
18:20:07.01 +21:42:10.0 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:15:27.08 -11:04:21.8 17.6mag P/2023 B1 (PANSTARRS)
22:08:14.29 +67:11:02.0 17.8mag C/2023 H5 (Lemmon)
17:15:58.04 -07:56:46.7 13.7mag C/2023 R1 (PANSTARRS)
13:17:39.01 +80:07:09.8 18.0mag C/2023 X2 (Lemmon)
07:28:14.65 +64:45:58.3 17.8mag C/2024 A1 (ATLAS)
07:05:22.70 +28:48:36.3 14.0mag C/2024 E1 (Wierzchos)
15:28:12.12 +14:26:44.4 17.4mag C/2024 G6 (ATLAS)
20:03:21.73 +34:38:30.0 13.9mag C/2024 J3 (ATLAS)
04:30:15.23 -14:58:22.5 15.9mag C/2024 T5 (ATLAS)
06:17:11.43 +32:23:53.1 17.9mag C/2025 J1 (Borisov)
11:32:04.42 +52:00:01.3 17.8mag C/2025 L1 (ATLAS)
06:58:03.75 -11:28:37.2 15.2mag C/2025 R3 (PANSTARRS)
09:35:01.52 +23:06:27.5 17.8mag C/2025 V2 (Rankin)
12:40:13.40 +04:33:12.4 17.1mag C/2025 Y1 (ATLAS)
17:48:10.01 +77:23:36.8 17.7mag C/2026 A2 (Bok)
02:20:31.12 +44:12:54.9 16.3mag C/2026 B2 (Sun-Gao)
11:15:03.75 +00:05:14.9 16.7mag A/2026 E1
20:45:31.32 -09:58:16.6 8.1mag 10P/Tempel
11:05:28.23 -01:12:37.0 16.0mag 29P/Schwassmann-Wachmann
03:30:31.53 +27:13:36.4 17.7mag 47P/Ashbrook-Jackson
09:26:03.14 +20:11:03.5 16.9mag 63P/Wild
00:36:37.78 -05:41:17.1 15.6mag 65P/Gunn
07:23:12.70 +34:17:51.4 17.2mag 76P/West-Kohoutek-Ikemura
03:38:53.55 +18:37:26.1 13.8mag 78P/Gehrels
01:46:12.72 +07:20:14.3 15.8mag 88P/Howell
05:33:52.07 +30:54:01.5 15.4mag 93P/Lovas
03:18:38.21 +29:23:03.7 17.3mag 114P/Wiseman-Skiff
07:20:01.52 +32:25:46.4 15.5mag 123P/West-Hartley
10:11:46.14 +09:26:30.0 16.6mag 124P/Mrkos
04:19:13.31 +19:59:11.9 16.3mag 128P/Shoemaker-Holt
04:57:46.52 +19:31:28.1 17.8mag 131P/Mueller
06:47:41.61 +16:55:46.0 16.2mag 141P/Machholz
06:51:17.22 +17:52:18.2 16.1mag 141P-A/Machholz
05:53:18.35 +17:17:32.9 13.0mag 141P-D/Machholz
03:05:56.31 -23:07:37.0 16.4mag 161P/Hartley-IRAS
04:22:41.89 +28:21:11.7 15.0mag 162P/SidingSpring
19:32:29.09 +05:44:59.6 16.2mag 169P/NEAT
00:50:51.31 +04:43:16.1 17.8mag 220P/McNaught
16:43:40.37 -08:05:59.5 16.6mag 235P/LINEAR
08:02:05.13 +34:51:00.6 17.7mag 240P/NEAT
01:04:47.04 +02:53:18.0 16.1mag 260P/McNaught
04:38:21.64 +34:30:45.6 17.5mag 295P/LINEAR
00:55:42.40 +03:22:15.8 17.9mag 320P/McNaught
15:10:28.63 +07:31:58.1 17.5mag 391P/Kowalski
08:17:11.57 +20:23:44.6 17.9mag 450P/LONEOS
07:19:53.32 +40:47:54.3 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 20 06:51 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
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
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:49:13.39 +25:17:59.20 2026-06-15.39 15.93
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:49:13.39 +25:17:59.20 2026-06-15.39 15.93
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.68 -22:39:32.70 ASASSN-26cm 2026-04-4.27 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
-rw-r--r-- 1 apache apache 5.6K Jun 20 06:51 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
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
-rw-r--r-- 1 apache apache 189K Jun 20 06:51 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:46:06.891 +33:41:13.54 AT 2026oyn 2026-06-03.92 19.91
22:04:59.426 +17:15:40.14 AT 2026oym 2026-06-09.20 19.68
15:19:51.792 +48:33:17.32 AT 2026oyl 2026-06-09.90 20.47
21:06:36.637 +12:42:18.62 AT 2026oyk 2026-06-10.12 19.64
13:35:55.780 +35:23:15.20 AT 2026oyj 2026-05-24.78 21.27
18:33:47.510 +37:36:07.65 AT 2026oyi 2026-05-10.79 21.55
18:14:44.150 +51:46:11.54 AT 2026oyh 2026-05-08.79 22.03
15:07:33.090 +20:01:11.55 AT 2026oyg 2026-05-07.82 21.15
13:35:40.460 -01:57:01.30 AT 2026oyf 2026-05-22.68 22.32
10:26:08.380 +04:26:57.22 AT 2026oye 2026-05-22.61 21.23
14:00:27.900 -01:28:05.40 AT 2026oyd 2026-06-02.72 21
13:47:00.850 +01:08:03.86 AT 2026oyc 2026-06-02.72 20.42
14:34:07.980 +03:43:00.64 AT 2026oyb 2026-05-25.68 21.54
13:48:38.410 +04:03:32.72 AT 2026oya 2026-05-09.68 22.13
00:38:19.802 -05:15:31.84 AT 2026oxz 2026-06-08.47 19.6034
14:39:23.496 +35:21:27.84 AT 2026oxy 2026-06-04.97 20.13
23:44:57.556 +04:18:42.85 SN 2026oxx 2026-06-11.15 19.97
15:19:13.587 +27:52:58.57 SN 2026oxw 2026-06-11.02 19.96
09:53:09.311 +42:13:35.56 AT 2026oxv 2026-06-10.17 19.7446
20:30:02.168 +37:49:06.79 AT 2026oxu 2026-06-10.94 19.78
-rw-r--r-- 1 apache apache 30K Jun 20 06:51 tns_transients_list.txt
