This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d
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 10 04.1584 2461317.6584 10.37 20:52:42.25 +50:27:26.3
89.51154 3.76237 galactic Cyg Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.1854+50.4538 | 20:52:42.06 +50:27:28.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.138+/-0.034 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:52:42.25 +50:27:26.3: 11.41 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:52:42.25 +50:27:26.3: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.1854+50.4538,2461317.6584,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.1854+50.4538 20261004.1584 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SS Cyg,2461317.6584,8.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SS Cyg 20261004.1584 8.91CV 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 10 04.1584 2461317.6584 10.32 20:51:12.21 +50:12:01.2
89.16015 3.78360 galactic Cyg Second-epoch detections are separated by 1.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2169680970993939072 | 20:51:12.00 +50:12:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:12.21 +50:12:01.2: 11.23 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:12.21 +50:12:01.2: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2169680970993939072,2461317.6584,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2169680970993939072 20261004.1584 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 10.06 20:51:05.79 +50:26:41.7
89.33880 3.95195 galactic Cyg Second-epoch detections are separated by 0.2" and 5.9 pix
The object was found in VSX 0" Gaia DR3 2169699697060120192
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.890 G 10.910 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:05.79 +50:26:41.7: 11.05 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:05.79 +50:26:41.7: 11.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2169699697060120192,2461317.6584,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2169699697060120192 20261004.1584 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 10.11 20:49:46.41 +50:22:36.4
89.15226 4.07212 galactic Cyg Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168200817894985088 | 20:49:46.45 +50:22:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.030 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:46.41 +50:22:36.4: 11.00 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:46.41 +50:22:36.4: 11.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168200817894985088,2461317.6584,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168200817894985088 20261004.1584 10.11CV 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 10 04.1584 2461317.6584 10.02 20:49:37.51 +50:24:52.9
89.16681 4.11438 galactic Cyg Second-epoch detections are separated by 0.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168201161492368640 | 20:49:37.20 +50:24:55.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:37.51 +50:24:52.9: 10.95 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:37.51 +50:24:52.9: 10.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2168201161492368640,2461317.6584,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168201161492368640 20261004.1584 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 9.88 20:51:43.72 +50:27:45.2
89.41650 3.88540 galactic Cyg Second-epoch detections are separated by 1.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.9254+50.4681 | 20:51:43.72 +50:27:45.3 (Gaia DR3) | DBF (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.030 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:43.72 +50:27:45.2: 10.72 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:43.72 +50:27:45.2: 10.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J312.9254+50.4681,2461317.6584,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.9254+50.4681 20261004.1584 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 10.68 20:50:26.16 +49:13:24.7
88.32445 3.26036 galactic Cyg Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168068399764179968 | 20:50:26.17 +49:13:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:26.16 +49:13:24.7: 11.67 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:26.16 +49:13:24.7: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168068399764179968,2461317.6584,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168068399764179968 20261004.1584 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 10.40 20:49:45.71 +50:21:50.8
89.14123 4.06557 galactic Cyg Second-epoch detections are separated by 0.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168200817894985088 | 20:49:46.45 +50:22:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.378+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:45.71 +50:21:50.8: 11.44 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:45.71 +50:21:50.8: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168200817894985088,2461317.6584,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168200817894985088 20261004.1584 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 10.31 20:51:04.60 +50:25:11.0
89.31727 3.93842 galactic Cyg Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2169699387822469376 | 20:51:04.69 +50:25:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.095+/-0.029 (A)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:04.60 +50:25:11.0: 11.43 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:04.60 +50:25:11.0: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2169699387822469376,2461317.6584,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2169699387822469376 20261004.1584 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.47 21:41:45.97 +43:47:14.2
90.56296 -6.84641 galactic Cyg Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:45.97 +43:47:14.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.826+/-0.029 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:45.97 +43:47:14.2: 13.59 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:45.97 +43:47:14.2: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 12.45 21:41:11.98 +44:11:42.8
90.75722 -6.47281 galactic Cyg Second-epoch detections are separated by 2.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2995+44.1952 | 21:41:11.98 +44:11:42.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.691+/-0.027 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:11.98 +44:11:42.8: 13.60 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:11.98 +44:11:42.8: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2995+44.1952,2461317.6584,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2995+44.1952 20261004.1584 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.43 21:41:18.70 +43:48:56.3
90.51982 -6.77094 galactic Cyg Second-epoch detections are separated by 3.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:18.70 +43:48:56.3 (user input) | T | P | (position from user input) J-Ks=0.916+/-0.025 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:18.70 +43:48:56.3: 13.67 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:18.70 +43:48:56.3: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.43CV 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 10 04.1584 2461317.6584 10.56 20:51:00.98 +50:27:14.4
89.33774 3.96758 galactic Cyg Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2169699765779592704 | 20:51:00.75 +50:27:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:00.98 +50:27:14.4: 11.76 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:00.98 +50:27:14.4: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2169699765779592704,2461317.6584,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2169699765779592704 20261004.1584 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.15 21:39:57.12 +44:20:58.4
90.69176 -6.20925 galactic Cyg Second-epoch detections are separated by 0.7" and 6.5 pix
The object was found in VSX 1" ASASSN-V J213957.09+442059.2
Type: SR
# Max. Min./Amp. JD0 Period
13.500 g Y 0.270 g 2459384.90300 34.270000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:57.12 +44:20:58.4: 12.15 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:57.12 +44:20:58.4: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213957.09+442059.2,2461317.6584,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213957.09+442059.2 20261004.1584 11.15CV 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 10 04.1584 2461317.6584 10.97 20:49:50.79 +50:26:08.0
89.20533 4.10018 galactic Cyg Second-epoch detections are separated by 3.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168201402010537088 | 20:49:50.89 +50:26:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:50.79 +50:26:08.0: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:50.79 +50:26:08.0: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168201402010537088,2461317.6584,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168201402010537088 20261004.1584 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.40 21:40:38.14 +43:44:28.7
90.37817 -6.74588 galactic Cyg Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1591+43.7403 | 21:40:38.14 +43:44:28.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:38.14 +43:44:28.7: 12.31 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:38.14 +43:44:28.7: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1591+43.7403,2461317.6584,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1591+43.7403 20261004.1584 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.38 20:51:11.94 +49:04:19.5
88.28644 3.06784 galactic Cyg Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.8097+49.0718 | 20:51:12.10 +49:04:19.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.344+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:11.94 +49:04:19.5: 12.41 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:11.94 +49:04:19.5: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 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
ATO J312.8097+49.0718,2461317.6584,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.8097+49.0718 20261004.1584 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.29 20:50:14.79 +50:28:25.5
89.27533 4.07493 galactic Cyg Second-epoch detections are separated by 1.8" and 5.5 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 | 20:50:14.79 +50:28:25.5 (user input) | T | P | (position from user input) J-Ks=0.792+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:14.79 +50:28:25.5: 13.93 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:14.79 +50:28:25.5: 13.80 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.59 21:40:43.31 +43:49:30.5
90.44584 -6.69341 galactic Cyg Second-epoch detections are separated by 1.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1899+43.8192 | 21:40:43.30 +43:49:30.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.398+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:43.31 +43:49:30.5: 12.53 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:43.31 +43:49:30.5: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1899+43.8192,2461317.6584,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1899+43.8192 20261004.1584 11.59CV 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 10 04.1584 2461317.6584 11.72 21:41:43.92 +43:52:22.8
90.61528 -6.77794 galactic Cyg Second-epoch detections are separated by 1.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4271+43.8632 | 21:41:43.88 +43:52:23.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.177+/-0.035 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:43.92 +43:52:22.8: 12.66 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:43.92 +43:52:22.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.4271+43.8632,2461317.6584,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4271+43.8632 20261004.1584 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.68 20:51:13.15 +49:07:13.9
88.32601 3.09607 galactic Cyg Second-epoch detections are separated by 0.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.8047+49.1209 | 20:51:13.14 +49:07:15.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.903+/-0.029 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:13.15 +49:07:13.9: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:13.15 +49:07:13.9: 12.75 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.8047+49.1209,2461317.6584,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.8047+49.1209 20261004.1584 11.68CV 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 10 04.1584 2461317.6584 11.59 20:50:39.04 +49:01:04.8
88.18748 3.10297 galactic Cyg Second-epoch detections are separated by 1.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2167312584297593600 | 20:50:39.13 +49:01:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.364+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:39.04 +49:01:04.8: 12.73 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:39.04 +49:01:04.8: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2167312584297593600,2461317.6584,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2167312584297593600 20261004.1584 11.59CV 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 10 04.1584 2461317.6584 11.40 20:50:19.46 +50:24:28.8
89.23211 4.02377 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 20:50:19.46 +50:24:28.8 (user input) | T | P | (position from user input) J-Ks=0.229+/-0.034 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:19.46 +50:24:28.8: 12.76 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:19.46 +50:24:28.8: 12.86 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.89 21:40:10.81 +44:19:47.1
90.70924 -6.25114 galactic Cyg Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0457+44.3235 | 21:40:10.81 +44:19:47.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.563+/-0.036 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:10.81 +44:19:47.1: 12.78 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:10.81 +44:19:47.1: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0457+44.3235,2461317.6584,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0457+44.3235 20261004.1584 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.94 21:37:41.38 +44:16:34.7
90.33932 -5.99400 galactic Cyg Second-epoch detections are separated by 0.9" and 6.4 pix
The object was found in VSX 1" ZTF J213741.38+441635.2
Type: SR
# Max. Min./Amp. JD0 Period
14.060 g Y 0.144 g 2458367.86420 46.704633400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:37:41.38 +44:16:34.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:37:41.38 +44:16:34.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213741.38+441635.2,2461317.6584,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J213741.38+441635.2 20261004.1584 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.38 20:50:21.21 +50:26:08.3
89.25652 4.03764 galactic Cyg Second-epoch detections are separated by 1.2" and 5.8 pix
The object was found in VSX20" Gaia DR3 2169701724285317888
Type: ROT
# Max. Min./Amp. JD0 Period
15.480 G 15.500 G G
ATTENTION: measured mag 11.38 is 4.1 mag brighter than the VSX record maximum brightness 15.48 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:21.21 +50:26:08.3: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:21.21 +50:26:08.3: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2169701724285317888,2461317.6584,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2169701724285317888 20261004.1584 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.89 21:40:11.53 +43:33:30.8
90.19562 -6.82938 galactic Cyg Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1967703227601209600 | 21:40:11.53 +43:33:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.909+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:11.53 +43:33:30.8: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:11.53 +43:33:30.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1967703227601209600,2461317.6584,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1967703227601209600 20261004.1584 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.63 20:50:08.66 +49:09:12.8
88.23997 3.25297 galactic Cyg Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168067708267980928 | 20:50:08.52 +49:09:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:08.66 +49:09:12.8: 12.88 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:08.66 +49:09:12.8: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168067708267980928,2461317.6584,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168067708267980928 20261004.1584 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.71 20:50:23.96 +49:04:34.7
88.20652 3.17177 galactic Cyg Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.5955+49.0666 | 20:50:23.96 +49:04:34.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.406+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:23.96 +49:04:34.7: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:23.96 +49:04:34.7: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 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
ATO J312.5955+49.0666,2461317.6584,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.5955+49.0666 20261004.1584 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.03 21:39:16.47 +44:34:15.5
90.74894 -5.96347 galactic Cyg Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.8145+44.5720 | 21:39:16.47 +44:34:15.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.165+/-0.037 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:16.47 +44:34:15.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:16.47 +44:34:15.5: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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
ATO J324.8145+44.5720,2461317.6584,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.8145+44.5720 20261004.1584 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.90 21:41:04.59 +43:42:38.9
90.41792 -6.82148 galactic Cyg Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2700+43.7134 | 21:41:04.59 +43:42:38.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.204+/-0.028 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:04.59 +43:42:38.9: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:04.59 +43:42:38.9: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2700+43.7134,2461317.6584,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2700+43.7134 20261004.1584 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.17 21:43:26.88 +44:08:01.8
91.02212 -6.78443 galactic Cyg Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1973748273804960896 | 21:43:26.88 +44:08:01.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.312+/-0.031 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:43:26.88 +44:08:01.8: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:43:26.88 +44:08:01.8: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1973748273804960896,2461317.6584,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1973748273804960896 20261004.1584 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.13 21:42:57.32 +43:54:22.5
90.80440 -6.89805 galactic Cyg Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:57.32 +43:54:22.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.872+/-0.025 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:57.32 +43:54:22.5: 13.02 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:57.32 +43:54:22.5: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.12 21:15:02.83 +50:17:58.7
91.76746 1.00047 galactic Cyg Second-epoch detections are separated by 0.6" and 6.2 pix
The object was found in VSX 2" ASASSN-V J211502.66+501800.3
Type: SR
# Max. Min./Amp. JD0 Period
15.160 g Y 0.350 g 2458223.96300 496.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:15:02.83 +50:17:58.7: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:15:02.83 +50:17:58.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211502.66+501800.3,2461317.6584,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211502.66+501800.3 20261004.1584 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.79 20:50:05.56 +49:13:57.8
88.29605 3.30958 galactic Cyg Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:05.56 +49:13:57.8 (user input) | T | P | (position from user input) J-Ks=0.762+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:05.56 +49:13:57.8: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:05.56 +49:13:57.8: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.79CV 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 10 04.1584 2461317.6584 12.09 21:39:48.96 +44:02:03.4
90.46272 -6.42872 galactic Cyg Second-epoch detections are separated by 0.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.9394+44.0313 | 21:39:48.96 +44:02:03.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.784+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:48.96 +44:02:03.4: 13.10 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:48.96 +44:02:03.4: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 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
ATO J324.9394+44.0313,2461317.6584,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.9394+44.0313 20261004.1584 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.13 21:27:55.72 +48:53:28.8
92.25171 -1.47021 galactic Cyg Second-epoch detections are separated by 2.9" and 6.7 pix
The object was found in VSX 1" Gaia DR3 2170778695936314880
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.970 G 13.000 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:27:55.72 +48:53:28.8: 13.12 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:27:55.72 +48:53:28.8: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2170778695936314880,2461317.6584,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2170778695936314880 20261004.1584 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.14 21:41:44.21 +43:49:09.6
90.58027 -6.81883 galactic Cyg Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4391+43.8259 | 21:41:45.93 +43:49:26.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:44.21 +43:49:09.6: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:44.21 +43:49:09.6: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 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
ATO J325.4391+43.8259,2461317.6584,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4391+43.8259 20261004.1584 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.00 21:23:05.05 +48:55:25.7
91.70300 -0.89248 galactic Cyg Second-epoch detections are separated by 1.7" and 6.4 pix
The object was found in VSX 1" ASASSN-V J212305.01+485526.7
Type: SR
# Max. Min./Amp. JD0 Period
13.510 V 13.690 V 2457297.86900 46.550000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:23:05.05 +48:55:25.7: 13.10 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:23:05.05 +48:55:25.7: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212305.01+485526.7,2461317.6584,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212305.01+485526.7 20261004.1584 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.21 21:42:38.88 +43:59:12.5
90.81573 -6.80098 galactic Cyg Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:38.88 +43:59:12.5 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.025 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:38.88 +43:59:12.5: 13.13 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:38.88 +43:59:12.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.12 21:41:46.94 +44:03:58.9
90.75060 -6.63862 galactic Cyg Second-epoch detections are separated by 2.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4468+44.0688 | 21:41:46.94 +44:03:58.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.182+/-0.031 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:46.94 +44:03:58.9: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:46.94 +44:03:58.9: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.4468+44.0688,2461317.6584,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4468+44.0688 20261004.1584 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.27 21:45:40.60 +45:38:54.6
92.31677 -5.89319 galactic Cyg Second-epoch detections are separated by 2.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:40.60 +45:38:54.6 (user input) | T | P | (position from user input) J-Ks=0.756+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:45:40.60 +45:38:54.6: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:45:40.60 +45:38:54.6: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.24 21:41:21.18 +43:31:18.1
90.32970 -6.99640 galactic Cyg Second-epoch detections are separated by 1.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3385+43.5217 | 21:41:21.18 +43:31:18.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.414+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:21.18 +43:31:18.1: 13.20 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:21.18 +43:31:18.1: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.3385+43.5217,2461317.6584,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3385+43.5217 20261004.1584 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.24 21:28:06.13 +48:20:54.6
91.89745 -1.88264 galactic Cyg Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J322.0249+48.3568 | 21:28:06.13 +48:20:54.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.884+/-0.032 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:28:06.13 +48:20:54.6: 13.23 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:28:06.13 +48:20:54.6: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J322.0249+48.3568,2461317.6584,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J322.0249+48.3568 20261004.1584 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.26 21:42:48.44 +44:08:08.0
90.93592 -6.70769 galactic Cyg Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.7003+44.1368 | 21:42:48.44 +44:08:08.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:48.44 +44:08:08.0: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:48.44 +44:08:08.0: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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
ATO J325.7003+44.1368,2461317.6584,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.7003+44.1368 20261004.1584 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 10 04.1584 2461317.6584 12.26 21:42:02.02 +43:38:59.8
90.50828 -6.98150 galactic Cyg Second-epoch detections are separated by 1.5" and 6.3 pix
The object was found in VSX16" Gaia DR3 1972961053545548288
Type: S
# Max. Min./Amp. JD0 Period
16.470 G 17.240 G F
ATTENTION: measured mag 12.26 is 4.2 mag brighter than the VSX record maximum brightness 16.47 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:02.02 +43:38:59.8: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:02.02 +43:38:59.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972961053545548288,2461317.6584,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972961053545548288 20261004.1584 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 10 04.1584 2461317.6584 12.40 21:28:31.62 +48:19:14.0
91.92930 -1.95158 galactic Cyg Second-epoch detections are separated by 2.1" and 6.4 pix
The object was found in VSX19" Gaia DR3 1978598799414045184
Type: RS
# Max. Min./Amp. JD0 Period
18.320 G 18.570 G
ATTENTION: measured mag 12.40 is 5.9 mag brighter than the VSX record maximum brightness 18.32 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:28:31.62 +48:19:14.0: 13.34 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:28:31.62 +48:19:14.0: 13.41 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1978598799414045184,2461317.6584,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1978598799414045184 20261004.1584 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.30 20:52:07.65 +48:52:24.5
88.23014 2.82391 galactic Cyg Second-epoch detections are separated by 3.2" 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 | ATO J313.0283+48.8732 | 20:52:07.65 +48:52:24.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.314+/-0.033 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:52:07.65 +48:52:24.5: 13.36 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:52:07.65 +48:52:24.5: 13.48 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.0283+48.8732,2461317.6584,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.0283+48.8732 20261004.1584 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.85 20:52:01.94 +50:26:37.7
89.43281 3.83618 galactic Cyg Second-epoch detections are separated by 1.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:52:01.94 +50:26:37.7 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.034 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:52:01.94 +50:26:37.7: 13.35 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:52:01.94 +50:26:37.7: 13.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 12.41 21:28:36.73 +48:15:41.1
91.89878 -2.00419 galactic Cyg Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:28:36.73 +48:15:41.1 (user input) | T | P | (position from user input) J-Ks=0.783+/-0.025 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:28:36.73 +48:15:41.1: 13.39 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:28:36.73 +48:15:41.1: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.30 21:40:45.67 +43:31:46.6
90.25398 -6.91944 galactic Cyg Second-epoch detections are separated by 2.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1866+43.5258 | 21:40:45.67 +43:31:46.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:45.67 +43:31:46.6: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:45.67 +43:31:46.6: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 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
ATO J325.1866+43.5258,2461317.6584,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1866+43.5258 20261004.1584 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.39 21:39:52.23 +43:50:53.7
90.34566 -6.57424 galactic Cyg Second-epoch detections are separated by 2.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.9582+43.8533 | 21:39:52.23 +43:50:53.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.082+/-0.027 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:52.23 +43:50:53.7: 13.42 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:52.23 +43:50:53.7: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.9582+43.8533,2461317.6584,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.9582+43.8533 20261004.1584 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.23 21:38:55.14 +44:28:22.9
90.63583 -5.99434 galactic Cyg Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:38:55.14 +44:28:22.9 (user input) | T | P | (position from user input) J-Ks=0.713+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:38:55.14 +44:28:22.9: 13.44 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:38:55.14 +44:28:22.9: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.26 21:41:08.31 +44:17:24.1
90.81202 -6.39443 galactic Cyg Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2843+44.2903 | 21:41:08.31 +44:17:24.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.304+/-0.030 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:08.31 +44:17:24.1: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:08.31 +44:17:24.1: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2843+44.2903,2461317.6584,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2843+44.2903 20261004.1584 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 10 04.1584 2461317.6584 12.37 21:40:26.91 +43:54:44.3
90.46688 -6.59549 galactic Cyg Second-epoch detections are separated by 0.5" and 6.4 pix
The object was found in VSX 5" Gaia DR3 1973727657968858368
Type: ROT
# Max. Min./Amp. JD0 Period
14.540 G 14.570 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:26.91 +43:54:44.3: 13.53 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:26.91 +43:54:44.3: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973727657968858368,2461317.6584,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973727657968858368 20261004.1584 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 10 04.1584 2461317.6584 12.48 21:38:35.60 +44:25:10.0
90.55635 -5.99552 galactic Cyg Second-epoch detections are separated by 2.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:38:35.60 +44:25:10.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.975+/-0.034 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:38:35.60 +44:25:10.0: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:38:35.60 +44:25:10.0: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.88 20:49:30.79 +50:27:22.5
89.18789 4.15442 galactic Cyg Second-epoch detections are separated by 1.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.3793+50.4450 | 20:49:30.79 +50:27:22.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.414+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:30.79 +50:27:22.5: 13.52 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:30.79 +50:27:22.5: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.3793+50.4450,2461317.6584,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.3793+50.4450 20261004.1584 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.45 21:40:16.53 +43:41:28.6
90.29572 -6.74015 galactic Cyg Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0661+43.6949 | 21:40:16.53 +43:41:28.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.411+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:16.53 +43:41:28.6: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:16.53 +43:41:28.6: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0661+43.6949,2461317.6584,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0661+43.6949 20261004.1584 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.32 21:41:40.87 +43:34:42.4
90.41245 -6.99311 galactic Cyg Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:40.87 +43:34:42.4 (user input) | T | P | (position from user input) J-Ks=0.765+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:40.87 +43:34:42.4: 13.51 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:40.87 +43:34:42.4: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.32CV 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 10 04.1584 2461317.6584 12.44 21:40:59.63 +44:00:04.8
90.60025 -6.59380 galactic Cyg Second-epoch detections are separated by 2.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2516+44.0050 | 21:40:59.63 +44:00:04.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.857+/-0.029 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:59.63 +44:00:04.8: 13.51 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:59.63 +44:00:04.8: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2516+44.0050,2461317.6584,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2516+44.0050 20261004.1584 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.41 21:39:07.45 +43:49:17.0
90.22656 -6.50471 galactic Cyg Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.7815+43.8214 | 21:39:07.45 +43:49:17.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.139+/-0.032 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:07.45 +43:49:17.0: 13.53 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:07.45 +43:49:17.0: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.7815+43.8214,2461317.6584,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.7815+43.8214 20261004.1584 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.34 21:42:37.29 +43:32:25.6
90.51627 -7.13399 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1972957106476556672 | 21:42:38.17 +43:31:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.420+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:37.29 +43:32:25.6: 13.52 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:37.29 +43:32:25.6: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972957106476556672,2461317.6584,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972957106476556672 20261004.1584 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.07 20:50:40.80 +48:59:01.0
88.16390 3.07745 galactic Cyg Second-epoch detections are separated by 0.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:40.80 +48:59:01.0 (user input) | T | P | (position from user input) J-Ks=0.689+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:40.80 +48:59:01.0: 13.52 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:40.80 +48:59:01.0: 13.39 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.28 21:42:21.99 +43:41:44.1
90.58419 -6.98684 galactic Cyg Second-epoch detections are separated by 2.2" and 6.3 pix
The object was found in VSX14" Gaia DR3 1972961985559508352
Type: ROT
# Max. Min./Amp. JD0 Period
16.550 G 16.600 G K
ATTENTION: measured mag 12.28 is 4.3 mag brighter than the VSX record maximum brightness 16.55 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:21.99 +43:41:44.1: 13.51 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:21.99 +43:41:44.1: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1972961985559508352,2461317.6584,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972961985559508352 20261004.1584 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.29 21:41:25.95 +43:55:28.2
90.60873 -6.70364 galactic Cyg Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3671+43.9241 | 21:41:25.95 +43:55:28.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.693+/- (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:25.95 +43:55:28.2: 13.49 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:25.95 +43:55:28.2: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.3671+43.9241,2461317.6584,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3671+43.9241 20261004.1584 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.39 21:41:41.43 +43:48:23.6
90.56545 -6.82291 galactic Cyg Second-epoch detections are separated by 3.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:41.43 +43:48:23.6 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:41.43 +43:48:23.6: 13.47 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:41.43 +43:48:23.6: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.24 21:40:38.90 +44:05:14.7
90.61079 -6.48818 galactic Cyg Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1783+44.0824 | 21:40:38.90 +44:05:14.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.904+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:38.90 +44:05:14.7: 13.42 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:38.90 +44:05:14.7: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1783+44.0824,2461317.6584,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1783+44.0824 20261004.1584 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.32 21:42:25.60 +43:51:20.1
90.69855 -6.87357 galactic Cyg Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:25.60 +43:51:20.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.334+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:25.60 +43:51:20.1: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:25.60 +43:51:20.1: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.32CV 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 10 04.1584 2461317.6584 12.11 21:41:48.82 +44:10:05.6
90.82249 -6.56577 galactic Cyg Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:48.82 +44:10:05.6 (user input) | T | P | (position from user input) J-Ks=0.772+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:48.82 +44:10:05.6: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:48.82 +44:10:05.6: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.11CV 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 10 04.1584 2461317.6584 12.29 21:39:56.69 +44:39:34.3
90.89773 -5.97657 galactic Cyg Second-epoch detections are separated by 2.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.9831+44.6552 | 21:39:56.69 +44:39:34.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.459+/-0.027 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:56.69 +44:39:34.3: 13.41 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:56.69 +44:39:34.3: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.9831+44.6552,2461317.6584,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.9831+44.6552 20261004.1584 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.36 21:40:43.45 +43:39:25.9
90.33409 -6.81946 galactic Cyg Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1830+43.6596 | 21:40:42.08 +43:38:53.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.851+/-0.029 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:43.45 +43:39:25.9: 13.39 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:43.45 +43:39:25.9: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 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
ATO J325.1830+43.6596,2461317.6584,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1830+43.6596 20261004.1584 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 10 04.1584 2461317.6584 12.30 21:41:25.84 +44:13:55.0
90.81291 -6.47260 galactic Cyg Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:25.84 +44:13:55.0 (user input) | T | P | (position from user input) J-Ks=1.003+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:25.84 +44:13:55.0: 13.42 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:25.84 +44:13:55.0: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.33 21:12:01.13 +50:30:46.6
91.58938 1.49708 galactic Cyg Second-epoch detections are separated by 1.4" and 6.0 pix
The object was found in VSX22" ZTF J211201.70+503107.4
Type: SR
# Max. Min./Amp. JD0 Period
14.344 r Y 0.083 r 2458355.72190 22.532506600000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:12:01.13 +50:30:46.6: 13.40 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:12:01.13 +50:30:46.6: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J211201.70+503107.4,2461317.6584,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J211201.70+503107.4 20261004.1584 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.34 21:40:12.92 +43:52:03.8
90.40546 -6.60097 galactic Cyg Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:12.92 +43:52:03.8 (user input) | T | P | (position from user input) J-Ks=0.496+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:12.92 +43:52:03.8: 13.42 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:12.92 +43:52:03.8: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.23 21:40:04.32 +44:10:32.7
90.59184 -6.35349 galactic Cyg Second-epoch detections are separated by 2.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.0184+44.1789 | 21:40:04.32 +44:10:32.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.802+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:04.32 +44:10:32.7: 13.38 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:04.32 +44:10:32.7: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.0184+44.1789,2461317.6584,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.0184+44.1789 20261004.1584 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.34 21:42:07.35 +44:09:55.1
90.86248 -6.60447 galactic Cyg Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5273+44.1675 | 21:42:07.35 +44:09:55.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:07.35 +44:09:55.1: 13.36 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:07.35 +44:09:55.1: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5273+44.1675,2461317.6584,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5273+44.1675 20261004.1584 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.36 21:40:23.49 +44:00:23.2
90.52199 -6.51822 galactic Cyg Second-epoch detections are separated by 4.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:23.49 +44:00:23.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:23.49 +44:00:23.2: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:23.49 +44:00:23.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 12.24 21:41:46.25 +44:26:44.8
91.00089 -6.35206 galactic Cyg Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:46.25 +44:26:44.8 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:46.25 +44:26:44.8: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:46.25 +44:26:44.8: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.31 21:40:48.22 +44:11:21.3
90.69967 -6.43034 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2036+44.1977 | 21:40:48.22 +44:11:21.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.730+/-0.027 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:48.22 +44:11:21.3: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:48.22 +44:11:21.3: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2036+44.1977,2461317.6584,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2036+44.1977 20261004.1584 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.36 21:26:55.09 +48:57:44.0
92.18090 -1.30419 galactic Cyg Second-epoch detections are separated by 2.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.7338+48.9656 | 21:26:55.36 +48:57:44.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:26:55.09 +48:57:44.0: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:26:55.09 +48:57:44.0: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.7338+48.9656,2461317.6584,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.7338+48.9656 20261004.1584 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 10 04.1584 2461317.6584 12.28 21:42:36.82 +43:55:55.5
90.77480 -6.83814 galactic Cyg Second-epoch detections are separated by 1.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.6413+43.9255 | 21:42:36.82 +43:55:55.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.388+/-0.026 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:36.82 +43:55:55.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:36.82 +43:55:55.5: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.6413+43.9255,2461317.6584,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6413+43.9255 20261004.1584 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.18 20:52:20.39 +49:05:57.2
88.42648 2.94107 galactic Cyg Second-epoch detections are separated by 2.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:52:20.39 +49:05:57.2 (user input) | T | P | (position from user input) J-Ks=0.225+/-0.033 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:52:20.39 +49:05:57.2: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:52:20.39 +49:05:57.2: 13.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.18CV 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 10 04.1584 2461317.6584 12.37 21:25:54.68 +49:22:23.7
92.34784 -0.89410 galactic Cyg Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.4799+49.3728 | 21:25:54.55 +49:22:24.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.428+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:25:54.68 +49:22:23.7: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:25:54.68 +49:22:23.7: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J321.4799+49.3728,2461317.6584,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.4799+49.3728 20261004.1584 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 10 04.1584 2461317.6584 12.33 21:42:30.77 +43:57:27.3
90.77793 -6.80699 galactic Cyg Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.6386+43.9517 | 21:42:30.77 +43:57:27.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.416+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:30.77 +43:57:27.3: 13.29 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:30.77 +43:57:27.3: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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
ATO J325.6386+43.9517,2461317.6584,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.6386+43.9517 20261004.1584 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.33 21:37:43.61 +43:44:13.7
89.98107 -6.39884 galactic Cyg Second-epoch detections are separated by 2.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.4312+43.7341 | 21:37:43.61 +43:44:13.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.456+/-0.056 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:37:43.61 +43:44:13.7: 13.31 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:37:43.61 +43:44:13.7: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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
ATO J324.4312+43.7341,2461317.6584,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.4312+43.7341 20261004.1584 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.26 21:41:19.20 +44:14:36.5
90.80559 -6.45085 galactic Cyg Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:19.20 +44:14:36.5 (user input) | T | P | (position from user input) J-Ks=0.818+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:19.20 +44:14:36.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:19.20 +44:14:36.5: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 12.20 21:41:35.44 +44:08:45.4
90.77744 -6.55612 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4127+44.1489 | 21:41:35.44 +44:08:45.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.854+/-0.027 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:35.44 +44:08:45.4: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:35.44 +44:08:45.4: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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
ATO J325.4127+44.1489,2461317.6584,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4127+44.1489 20261004.1584 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.27 21:44:14.84 +45:35:57.6
92.09378 -5.76805 galactic Cyg Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:44:14.84 +45:35:57.6 (user input) | T | P | (position from user input) J-Ks=0.499+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:44:14.84 +45:35:57.6: 13.26 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:44:14.84 +45:35:57.6: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.24 21:38:41.33 +43:51:44.8
90.19526 -6.42176 galactic Cyg Second-epoch detections are separated by 1.7" and 6.3 pix
The object was found in VSX 1" Gaia DR3 1967772118877925632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.250 G 13.290 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:38:41.33 +43:51:44.8: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:38:41.33 +43:51:44.8: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1967772118877925632,2461317.6584,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1967772118877925632 20261004.1584 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.19 21:42:10.34 +44:16:04.1
90.93720 -6.53322 galactic Cyg Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:10.34 +44:16:04.1 (user input) | T | P | (position from user input) J-Ks=0.719+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:10.34 +44:16:04.1: 13.26 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:10.34 +44:16:04.1: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 12.06 21:40:54.20 +43:55:55.0
90.54173 -6.63504 galactic Cyg Second-epoch detections are separated by 2.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:54.20 +43:55:55.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:54.20 +43:55:55.0: 13.08 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:54.20 +43:55:55.0: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 12.12 21:21:43.45 +48:41:45.6
91.38356 -0.89669 galactic Cyg Second-epoch detections are separated by 1.8" and 6.2 pix
The object was found in VSX 2" ASASSN-V J212143.42+484144.0
Type: L
# Max. Min./Amp. JD0 Period
13.950 V 14.570 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:21:43.45 +48:41:45.6: 13.20 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:21:43.45 +48:41:45.6: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J212143.42+484144.0,2461317.6584,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J212143.42+484144.0 20261004.1584 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.16 21:40:44.51 +44:04:07.0
90.61091 -6.51340 galactic Cyg Second-epoch detections are separated by 2.1" and 6.8 pix
The object was found in VSX19" Gaia DR3 1973735354550346880
Type: ROT
# Max. Min./Amp. JD0 Period
16.680 G 16.740 G G
ATTENTION: measured mag 12.16 is 4.5 mag brighter than the VSX record maximum brightness 16.68 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:44.51 +44:04:07.0: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:44.51 +44:04:07.0: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973735354550346880,2461317.6584,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973735354550346880 20261004.1584 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.23 21:39:04.37 +44:07:38.6
90.42482 -6.27041 galactic Cyg Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:04.37 +44:07:38.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.444+/-0.041 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:04.37 +44:07:38.6: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:04.37 +44:07:38.6: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.11 21:40:54.90 +43:57:59.3
90.56633 -6.61055 galactic Cyg Second-epoch detections are separated by 2.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2314+43.9609 | 21:40:54.90 +43:57:59.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.813+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:54.90 +43:57:59.3: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:54.90 +43:57:59.3: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 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
ATO J325.2314+43.9609,2461317.6584,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2314+43.9609 20261004.1584 12.11CV 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 10 04.1584 2461317.6584 12.12 21:39:59.14 +44:09:50.6
90.57238 -6.35196 galactic Cyg Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1973787203391124480 | 21:39:59.14 +44:09:50.6 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.757+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:59.14 +44:09:50.6: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:59.14 +44:09:50.6: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1973787203391124480,2461317.6584,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1973787203391124480 20261004.1584 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.12 21:42:01.92 +43:42:27.6
90.54640 -6.93791 galactic Cyg Second-epoch detections are separated by 0.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:01.92 +43:42:27.6 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:01.92 +43:42:27.6: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:01.92 +43:42:27.6: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.25 21:45:09.78 +45:43:57.9
92.30313 -5.77087 galactic Cyg Second-epoch detections are separated by 1.8" and 6.7 pix
The object was found in VSX17" Gaia DR3 1974171272252546816
Type: E
# Max. Min./Amp. JD0 Period
19.410 G 19.720 G 0.334512000000
ATTENTION: measured mag 12.25 is 7.2 mag brighter than the VSX record maximum brightness 19.41 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:45:09.78 +45:43:57.9: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:45:09.78 +45:43:57.9: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1974171272252546816,2461317.6584,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1974171272252546816 20261004.1584 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.30 21:43:07.46 +44:54:07.6
91.48510 -6.16640 galactic Cyg Second-epoch detections are separated by 2.2" and 6.5 pix
The object was found in VSX 1" Gaia DR3 1973921721774931456
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.980 G 13.010 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:43:07.46 +44:54:07.6: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:43:07.46 +44:54:07.6: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973921721774931456,2461317.6584,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973921721774931456 20261004.1584 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.21 21:42:38.05 +44:19:35.4
91.03871 -6.54339 galactic Cyg Second-epoch detections are separated by 4.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:38.05 +44:19:35.4 (user input) | T | P | (position from user input) J-Ks=0.719+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:38.05 +44:19:35.4: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:38.05 +44:19:35.4: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.69 20:51:01.44 +50:24:15.3
89.29994 3.93509 galactic Cyg Second-epoch detections are separated by 0.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J205058.12+502412.1 | 20:50:58.12 +50:24:12.1 (Gaia DR3) | EA (local) | 2.924200000000 (local) | Gaia3var=VARIABLE J-Ks=0.762+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:01.44 +50:24:15.3: 13.12 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:01.44 +50:24:15.3: 13.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205058.12+502412.1,2461317.6584,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205058.12+502412.1 20261004.1584 11.69CV 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 10 04.1584 2461317.6584 12.21 21:39:15.45 +44:15:53.0
90.54167 -6.19001 galactic Cyg Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:15.45 +44:15:53.0 (user input) | T | P | (position from user input) J-Ks=0.322+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:15.45 +44:15:53.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:15.45 +44:15:53.0: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.25 21:45:11.48 +45:25:21.5
92.10437 -6.00984 galactic Cyg Second-epoch detections are separated by 1.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:45:11.48 +45:25:21.5 (user input) | T | P | (position from user input) J-Ks=0.663+/-0.024 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:45:11.48 +45:25:21.5: 13.12 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:45:11.48 +45:25:21.5: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.04 21:41:27.90 +44:25:30.0
90.94582 -6.33166 galactic Cyg Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3571+44.4235 | 21:41:27.90 +44:25:30.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.376+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:27.90 +44:25:30.0: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:27.90 +44:25:30.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 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
ATO J325.3571+44.4235,2461317.6584,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3571+44.4235 20261004.1584 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 10 04.1584 2461317.6584 12.12 21:45:28.02 +44:12:35.8
91.34838 -6.96315 galactic Cyg Second-epoch detections are separated by 1.1" and 6.6 pix
The object was found in VSX23" Gaia DR3 1973089906865925248
Type: ROT
# Max. Min./Amp. JD0 Period
16.310 G 16.360 G G
ATTENTION: measured mag 12.12 is 4.2 mag brighter than the VSX record maximum brightness 16.31 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:45:28.02 +44:12:35.8: 13.08 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:45:28.02 +44:12:35.8: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973089906865925248,2461317.6584,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973089906865925248 20261004.1584 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.07 21:42:16.86 +44:05:41.1
90.83725 -6.67630 galactic Cyg Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:16.86 +44:05:41.1 (user input) | T | P | (position from user input) J-Ks=1.054+/-0.025 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:16.86 +44:05:41.1: 13.08 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:16.86 +44:05:41.1: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.87 20:50:35.73 +49:08:24.0
88.27625 3.18728 galactic Cyg Second-epoch detections are separated by 0.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:35.73 +49:08:24.0 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:35.73 +49:08:24.0: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:35.73 +49:08:24.0: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.15 21:40:55.30 +43:23:10.2
90.18019 -7.04618 galactic Cyg Second-epoch detections are separated by 0.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1972950951778584320 | 21:40:55.39 +43:23:10.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.228+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:55.30 +43:23:10.2: 13.08 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:55.30 +43:23:10.2: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972950951778584320,2461317.6584,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972950951778584320 20261004.1584 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.53 20:50:19.67 +50:31:03.9
89.31771 4.09271 galactic Cyg Second-epoch detections are separated by 2.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:19.67 +50:31:03.9 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:19.67 +50:31:03.9: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:19.67 +50:31:03.9: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.02 21:41:11.45 +43:47:54.2
90.49187 -6.76947 galactic Cyg Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2906+43.7896 | 21:41:11.45 +43:47:54.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.904+/-0.025 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:11.45 +43:47:54.2: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:11.45 +43:47:54.2: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.2906+43.7896,2461317.6584,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2906+43.7896 20261004.1584 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 10 04.1584 2461317.6584 12.06 21:41:44.75 +44:06:22.5
90.77213 -6.60432 galactic Cyg Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | PMAK V8 | 21:41:45.58 +44:05:49.3 (Gaia DR3) | SR (local) | 126.900000000000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:44.75 +44:06:22.5: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:44.75 +44:06:22.5: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
PMAK V8,2461317.6584,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PMAK V8 20261004.1584 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 10 04.1584 2461317.6584 11.86 20:50:26.01 +49:01:53.9
88.17545 3.13915 galactic Cyg Second-epoch detections are separated by 1.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168061798393044224 | 20:50:25.86 +49:01:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.976+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:26.01 +49:01:53.9: 13.05 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:26.01 +49:01:53.9: 12.98 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168061798393044224,2461317.6584,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168061798393044224 20261004.1584 11.86CV 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 10 04.1584 2461317.6584 12.10 21:39:44.02 +44:17:42.2
90.62598 -6.22405 galactic Cyg Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1973800500616163328 | 21:39:44.02 +44:17:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.989+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:44.02 +44:17:42.2: 13.04 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:44.02 +44:17:42.2: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973800500616163328,2461317.6584,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973800500616163328 20261004.1584 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.05 21:41:22.43 +44:21:27.6
90.88878 -6.37147 galactic Cyg Second-epoch detections are separated by 0.4" and 6.4 pix
The object was found in VSX22" Gaia DR3 1973810052624114944
Type: ROT
# Max. Min./Amp. JD0 Period
13.760 G 13.780 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:22.43 +44:21:27.6: 13.03 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:22.43 +44:21:27.6: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973810052624114944,2461317.6584,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973810052624114944 20261004.1584 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 10 04.1584 2461317.6584 12.04 21:42:39.01 +44:06:48.7
90.89994 -6.70576 galactic Cyg Second-epoch detections are separated by 0.7" and 6.5 pix
The object was found in VSX10" Gaia DR3 1973745589452733696
Type: ROT
# Max. Min./Amp. JD0 Period
18.560 G 18.750 G
ATTENTION: measured mag 12.04 is 6.5 mag brighter than the VSX record maximum brightness 18.56 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:39.01 +44:06:48.7: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:39.01 +44:06:48.7: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973745589452733696,2461317.6584,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973745589452733696 20261004.1584 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 10 04.1584 2461317.6584 12.09 21:41:19.21 +44:04:16.1
90.69101 -6.58022 galactic Cyg Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:19.21 +44:04:16.1 (user input) | T | P | (position from user input) J-Ks=0.765+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:19.21 +44:04:16.1: 13.02 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:19.21 +44:04:16.1: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.15 21:39:07.89 +43:21:35.7
89.91778 -6.84954 galactic Cyg Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:39:07.89 +43:21:35.7 (user input) | T | P | (position from user input) J-Ks=0.238+/-0.031 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:07.89 +43:21:35.7: 13.02 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:07.89 +43:21:35.7: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.06 21:41:36.67 +44:02:03.5
90.70604 -6.64241 galactic Cyg Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:36.67 +44:02:03.5 (user input) | T | P | (position from user input) J-Ks=0.862+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:36.67 +44:02:03.5: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:36.67 +44:02:03.5: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 12.21 21:42:09.79 +44:45:56.8
91.26579 -6.15729 galactic Cyg Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1973837093738503424 | 21:42:12.31 +44:45:26.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.812+/-0.024 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:09.79 +44:45:56.8: 13.00 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:09.79 +44:45:56.8: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973837093738503424,2461317.6584,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973837093738503424 20261004.1584 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.09 21:43:14.68 +43:36:25.5
90.64614 -7.15797 galactic Cyg Second-epoch detections are separated by 0.8" and 6.5 pix
The object was found in VSX 2" Gaia DR3 1972969372904277888
Type: E
# Max. Min./Amp. JD0 Period
17.540 G 17.630 G 0.254395000000
ATTENTION: measured mag 12.09 is 5.4 mag brighter than the VSX record maximum brightness 17.54 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:43:14.68 +43:36:25.5: 13.01 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:43:14.68 +43:36:25.5: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972969372904277888,2461317.6584,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972969372904277888 20261004.1584 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.95 21:40:42.41 +43:57:37.8
90.53409 -6.59022 galactic Cyg Second-epoch detections are separated by 1.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1782+43.9635 | 21:40:42.41 +43:57:37.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.369+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:42.41 +43:57:37.8: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:42.41 +43:57:37.8: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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
ATO J325.1782+43.9635,2461317.6584,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1782+43.9635 20261004.1584 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.09 21:44:43.54 +45:30:10.4
92.09449 -5.89577 galactic Cyg Second-epoch detections are separated by 2.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J326.1792+45.5054 | 21:44:43.54 +45:30:10.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.853+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:44:43.54 +45:30:10.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:44:43.54 +45:30:10.4: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J326.1792+45.5054,2461317.6584,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J326.1792+45.5054 20261004.1584 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.12 21:40:51.19 +44:36:41.5
90.98746 -6.11959 galactic Cyg Second-epoch detections are separated by 0.9" and 6.3 pix
The object was found in VSX 2" ASASSN-V J214051.35+443641.4
Type: DSCT
# Max. Min./Amp. JD0 Period
13.110 V 13.180 V 2457853.10900 0.120910000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:51.19 +44:36:41.5: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:51.19 +44:36:41.5: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214051.35+443641.4,2461317.6584,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214051.35+443641.4 20261004.1584 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.83 20:50:49.44 +49:04:34.0
88.25051 3.11785 galactic Cyg Second-epoch detections are separated by 0.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.7065+49.0759 | 20:50:49.44 +49:04:34.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.056+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:49.44 +49:04:34.0: 13.01 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:49.44 +49:04:34.0: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7065+49.0759,2461317.6584,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.7065+49.0759 20261004.1584 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.95 21:42:05.20 +43:28:02.8
90.39427 -7.12501 galactic Cyg Second-epoch detections are separated by 0.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:05.20 +43:28:02.8 (user input) | T | P | (position from user input) J-Ks=0.409+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:05.20 +43:28:02.8: 12.98 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:05.20 +43:28:02.8: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.86 21:41:09.73 +43:47:22.3
90.48206 -6.77269 galactic Cyg Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2906+43.7896 | 21:41:09.73 +43:47:22.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.247+/-0.028 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:09.73 +43:47:22.3: 12.97 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:09.73 +43:47:22.3: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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
ATO J325.2906+43.7896,2461317.6584,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2906+43.7896 20261004.1584 11.86CV 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 10 04.1584 2461317.6584 12.07 21:41:32.66 +44:31:33.9
91.02363 -6.26506 galactic Cyg Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1973816443535584512 | 21:41:35.16 +44:31:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.026 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:32.66 +44:31:33.9: 12.96 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:32.66 +44:31:33.9: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973816443535584512,2461317.6584,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973816443535584512 20261004.1584 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.96 21:42:52.08 +43:55:03.2
90.79994 -6.87919 galactic Cyg Second-epoch detections are separated by 2.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Vend4 | 21:42:53.84 +43:55:36.2 (Gaia DR3) | SR (local) | 461.286190900000 (local) | Gaia3var=VARIABLE SpType: F0 (LAMOST DR5) J-Ks=0.308+/-0.026 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:52.08 +43:55:03.2: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:52.08 +43:55:03.2: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Vend4,2461317.6584,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Vend4 20261004.1584 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 10 04.1584 2461317.6584 11.95 21:40:06.08 +44:22:23.2
90.72757 -6.20935 galactic Cyg Second-epoch detections are separated by 3.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:06.08 +44:22:23.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:06.08 +44:22:23.2: 12.92 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:06.08 +44:22:23.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.96 21:40:36.79 +44:07:30.9
90.63125 -6.45566 galactic Cyg Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:36.79 +44:07:30.9 (user input) | T | P | (position from user input) J-Ks=0.703+/-0.027 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:36.79 +44:07:30.9: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:36.79 +44:07:30.9: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 11.96 21:42:29.68 +44:06:23.5
90.87413 -6.69267 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 pix
The object was found in VSX 1" Gaia DR3 1973745731192006784
Type: ROT
# Max. Min./Amp. JD0 Period
12.810 G 12.840 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:29.68 +44:06:23.5: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:29.68 +44:06:23.5: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973745731192006784,2461317.6584,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973745731192006784 20261004.1584 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 10 04.1584 2461317.6584 11.92 21:42:02.75 +43:29:48.7
90.40821 -7.09802 galactic Cyg Second-epoch detections are separated by 3.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:42:02.75 +43:29:48.7 (user input) | T | P | (position from user input) J-Ks=1.107+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:02.75 +43:29:48.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:02.75 +43:29:48.7: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.76 20:50:57.80 +49:10:08.2
88.33686 3.15913 galactic Cyg Second-epoch detections are separated by 1.2" 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 | 20:50:57.80 +49:10:08.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:57.80 +49:10:08.2: 12.93 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:57.80 +49:10:08.2: 12.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.76CV 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 10 04.1584 2461317.6584 11.74 20:50:19.79 +49:19:18.5
88.38967 3.33598 galactic Cyg Second-epoch detections are separated by 1.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.5806+49.3109 | 20:50:19.79 +49:19:18.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.570+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:19.79 +49:19:18.5: 12.88 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:19.79 +49:19:18.5: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 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
ATO J312.5806+49.3109,2461317.6584,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.5806+49.3109 20261004.1584 11.74CV 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 10 04.1584 2461317.6584 11.88 21:40:24.93 +43:44:24.5
90.34742 -6.72038 galactic Cyg Second-epoch detections are separated by 2.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:24.93 +43:44:24.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.389+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:24.93 +43:44:24.5: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:24.93 +43:44:24.5: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.94 21:41:49.52 +44:14:22.6
90.87146 -6.51349 galactic Cyg Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4591+44.2380 | 21:41:49.52 +44:14:22.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.809+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:49.52 +44:14:22.6: 12.87 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:49.52 +44:14:22.6: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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
ATO J325.4591+44.2380,2461317.6584,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4591+44.2380 20261004.1584 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.68 20:50:36.51 +49:07:48.8
88.27003 3.17944 galactic Cyg Second-epoch detections are separated by 1.0" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:36.51 +49:07:48.8 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:36.51 +49:07:48.8: 12.86 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:36.51 +49:07:48.8: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.68CV 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 10 04.1584 2461317.6584 11.83 21:41:12.10 +44:19:42.7
90.84615 -6.37301 galactic Cyg Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3052+44.3339 | 21:41:12.09 +44:19:43.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.841+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:12.10 +44:19:42.7: 12.87 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:12.10 +44:19:42.7: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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
ATO J325.3052+44.3339,2461317.6584,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3052+44.3339 20261004.1584 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.86 21:40:29.65 +44:08:05.1
90.62150 -6.43440 galactic Cyg Second-epoch detections are separated by 0.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1242+44.1347 | 21:40:29.65 +44:08:05.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.273+/-0.050 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:29.65 +44:08:05.1: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:29.65 +44:08:05.1: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J325.1242+44.1347,2461317.6584,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1242+44.1347 20261004.1584 11.86CV 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 10 04.1584 2461317.6584 11.81 21:41:58.48 +44:11:35.6
90.86093 -6.56601 galactic Cyg Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5042+44.1894 | 21:42:01.01 +44:11:22.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.765+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:58.48 +44:11:35.6: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:58.48 +44:11:35.6: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5042+44.1894,2461317.6584,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5042+44.1894 20261004.1584 11.81CV 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 10 04.1584 2461317.6584 11.79 21:41:16.73 +44:07:02.1
90.71608 -6.54071 galactic Cyg Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:16.73 +44:07:02.1 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:16.73 +44:07:02.1: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:16.73 +44:07:02.1: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.79CV 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 10 04.1584 2461317.6584 11.63 20:50:08.10 +49:21:40.0
88.40004 3.38543 galactic Cyg Second-epoch detections are separated by 1.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:08.10 +49:21:40.0 (user input) | T | P | (position from user input) J-Ks=0.264+/-0.031 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:08.10 +49:21:40.0: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:08.10 +49:21:40.0: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.77 21:40:37.16 +43:48:47.5
90.42393 -6.69010 galactic Cyg Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:40:37.16 +43:48:47.5 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:37.16 +43:48:47.5: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:37.16 +43:48:47.5: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 11.93 21:40:26.78 +44:33:27.1
90.89690 -6.11211 galactic Cyg Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1113+44.5577 | 21:40:26.73 +44:33:27.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.696+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:26.78 +44:33:27.1: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:26.78 +44:33:27.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1113+44.5577,2461317.6584,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1113+44.5577 20261004.1584 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.71 21:41:08.78 +44:01:21.4
90.63512 -6.59599 galactic Cyg Second-epoch detections are separated by 1.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2735+44.0187 | 21:41:08.78 +44:01:21.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:08.78 +44:01:21.4: 12.81 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:08.78 +44:01:21.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2735+44.0187,2461317.6584,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2735+44.0187 20261004.1584 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.79 21:41:02.78 +44:23:06.9
90.86292 -6.31210 galactic Cyg Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2657+44.3875 | 21:41:02.78 +44:23:06.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:02.78 +44:23:06.9: 12.76 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:02.78 +44:23:06.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2657+44.3875,2461317.6584,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2657+44.3875 20261004.1584 11.79CV 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 10 04.1584 2461317.6584 11.78 21:41:20.31 +43:52:27.2
90.56247 -6.73018 galactic Cyg Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.3348+43.8742 | 21:41:20.31 +43:52:27.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.233+/-0.028 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:20.31 +43:52:27.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:20.31 +43:52:27.2: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.3348+43.8742,2461317.6584,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.3348+43.8742 20261004.1584 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.84 21:41:49.27 +43:52:18.3
90.62661 -6.78948 galactic Cyg Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:41:49.27 +43:52:18.3 (user input) | T | P | (position from user input) J-Ks=0.248+/-0.031 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:49.27 +43:52:18.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:49.27 +43:52:18.3: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.80 21:42:05.79 +43:56:24.1
90.70949 -6.77086 galactic Cyg Second-epoch detections are separated by 0.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.5240+43.9402 | 21:42:05.78 +43:56:25.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.863+/-0.029 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:05.79 +43:56:24.1: 12.73 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:05.79 +43:56:24.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.5240+43.9402,2461317.6584,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.5240+43.9402 20261004.1584 11.80CV 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 10 04.1584 2461317.6584 11.77 21:41:57.27 +43:40:45.4
90.51693 -6.95001 galactic Cyg Second-epoch detections are separated by 0.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1972961397141805312 | 21:41:57.28 +43:40:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.853+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:57.27 +43:40:45.4: 12.71 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:57.27 +43:40:45.4: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1972961397141805312,2461317.6584,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1972961397141805312 20261004.1584 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 10 04.1584 2461317.6584 11.72 21:42:01.66 +44:11:54.1
90.87153 -6.56840 galactic Cyg Second-epoch detections are separated by 0.9" and 6.6 pix
The object was found in VSX 1" ASASSN-V J214201.66+441155.0
Type: L
# Max. Min./Amp. JD0 Period
12.530 V 12.690 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:01.66 +44:11:54.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:01.66 +44:11:54.1: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214201.66+441155.0,2461317.6584,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214201.66+441155.0 20261004.1584 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.79 21:39:19.20 +44:00:46.3
90.38139 -6.38540 galactic Cyg Second-epoch detections are separated by 1.6" and 6.5 pix
The object was found in VSX 1" Gaia DR3 1973778957060114688
Type: E
# Max. Min./Amp. JD0 Period
12.660 G 12.950 G 3.532150000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:19.20 +44:00:46.3: 12.71 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:19.20 +44:00:46.3: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973778957060114688,2461317.6584,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973778957060114688 20261004.1584 11.79CV 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 10 04.1584 2461317.6584 11.29 20:49:55.60 +50:26:15.0
89.21492 4.09150 galactic Cyg Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2168201402010537088 | 20:49:50.89 +50:26:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.825+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:55.60 +50:26:15.0: 12.67 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:55.60 +50:26:15.0: 12.73 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2168201402010537088,2461317.6584,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168201402010537088 20261004.1584 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.63 21:41:02.22 +43:56:55.5
90.57109 -6.63837 galactic Cyg Second-epoch detections are separated by 0.7" and 6.4 pix
The object was found in VSX20" ASASSN-V J214101.17+435638.9
Type: L
# Max. Min./Amp. JD0 Period
13.070 V 13.330 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:02.22 +43:56:55.5: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:02.22 +43:56:55.5: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J214101.17+435638.9,2461317.6584,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J214101.17+435638.9 20261004.1584 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.76 21:40:54.19 +44:30:41.3
90.92761 -6.20052 galactic Cyg Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.2294+44.5199 | 21:40:54.18 +44:30:41.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.703+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:54.19 +44:30:41.3: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:54.19 +44:30:41.3: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.2294+44.5199,2461317.6584,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.2294+44.5199 20261004.1584 11.76CV 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 10 04.1584 2461317.6584 11.54 21:39:13.07 +48:41:33.9
93.48677 -2.87482 galactic Cyg Second-epoch detections are separated by 2.6" and 6.6 pix
The object was found in VSX 3" ASASSN-V J213913.01+484136.8
Type: L
# Max. Min./Amp. JD0 Period
12.220 V 12.940 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:39:13.07 +48:41:33.9: 12.60 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:39:13.07 +48:41:33.9: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J213913.01+484136.8,2461317.6584,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J213913.01+484136.8 20261004.1584 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.57 21:30:36.63 +49:51:16.9
93.23117 -1.07052 galactic Cyg Second-epoch detections are separated by 0.9" and 6.1 pix
The object was found in VSX 1" V2071 Cyg
Type: LB
# Max. Min./Amp. JD0 Period
12.900 V 13.800 V N
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:30:36.63 +49:51:16.9: 12.57 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:30:36.63 +49:51:16.9: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2071 Cyg,2461317.6584,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2071 Cyg 20261004.1584 11.57CV 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 10 04.1584 2461317.6584 11.45 20:50:56.12 +49:04:13.6
88.25771 3.10016 galactic Cyg Second-epoch detections are separated by 2.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.7285+49.0706 | 20:50:56.25 +49:04:13.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.459+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:56.12 +49:04:13.6: 12.60 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:56.12 +49:04:13.6: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.59 +/- 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
ATO J312.7285+49.0706,2461317.6584,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.7285+49.0706 20261004.1584 11.45CV 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 10 04.1584 2461317.6584 11.62 21:40:09.03 +44:10:03.6
90.59704 -6.36888 galactic Cyg Second-epoch detections are separated by 0.5" and 6.4 pix
The object was found in VSX 0" PMAK V17
Type: SRS
# Max. Min./Amp. JD0 Period
12.840 V 13.170 V 2457749.00000 27.600000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:09.03 +44:10:03.6: 12.57 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:09.03 +44:10:03.6: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
PMAK V17,2461317.6584,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PMAK V17 20261004.1584 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 10 04.1584 2461317.6584 11.62 21:41:49.42 +44:15:10.4
90.88004 -6.50331 galactic Cyg Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.4582+44.2524 | 21:41:49.42 +44:15:10.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:49.42 +44:15:10.4: 12.55 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:49.42 +44:15:10.4: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.4582+44.2524,2461317.6584,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.4582+44.2524 20261004.1584 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 10 04.1584 2461317.6584 11.14 20:50:58.13 +50:24:12.4
89.29373 3.94138 galactic Cyg Second-epoch detections are separated by 1.0" and 5.8 pix
The object was found in VSX 0" ASASSN-V J205058.12+502412.1
Type: EA
# Max. Min./Amp. JD0 Period
12.470 g Y 0.340 g 2458420.75800 2.924200000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:58.13 +50:24:12.4: 12.46 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:58.13 +50:24:12.4: 12.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205058.12+502412.1,2461317.6584,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205058.12+502412.1 20261004.1584 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.43 20:51:27.17 +49:04:07.0
88.31021 3.03354 galactic Cyg Second-epoch detections are separated by 0.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.8687+49.0756 | 20:51:27.13 +49:04:08.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.744+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:27.17 +49:04:07.0: 12.45 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:27.17 +49:04:07.0: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J312.8687+49.0756,2461317.6584,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J312.8687+49.0756 20261004.1584 11.43CV 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 10 04.1584 2461317.6584 11.46 20:50:47.20 +48:51:48.7
88.08205 2.98775 galactic Cyg Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.7016+48.8613 | 20:50:47.20 +48:51:49.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.435+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:47.20 +48:51:48.7: 12.47 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:47.20 +48:51:48.7: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7016+48.8613,2461317.6584,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.7016+48.8613 20261004.1584 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.51 21:41:21.14 +43:46:10.9
90.49478 -6.81027 galactic Cyg Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1973716177511328768 | 21:41:21.16 +43:46:10.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.666+/-0.025 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:21.14 +43:46:10.9: 12.46 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:21.14 +43:46:10.9: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973716177511328768,2461317.6584,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973716177511328768 20261004.1584 11.51CV 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 10 04.1584 2461317.6584 11.52 21:40:42.04 +43:38:53.2
90.32483 -6.82345 galactic Cyg Second-epoch detections are separated by 0.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J325.1830+43.6596 | 21:40:42.08 +43:38:53.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:40:42.04 +43:38:53.2: 12.44 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:40:42.04 +43:38:53.2: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J325.1830+43.6596,2461317.6584,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J325.1830+43.6596 20261004.1584 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.44 20:51:28.89 +49:03:48.5
88.30923 3.02665 galactic Cyg Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.8687+49.0756 | 20:51:27.13 +49:04:08.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.213+/-0.032 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:28.89 +49:03:48.5: 12.43 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:28.89 +49:03:48.5: 12.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 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
ATO J312.8687+49.0756,2461317.6584,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.8687+49.0756 20261004.1584 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.39 21:41:36.89 +43:39:11.3
90.45306 -6.92909 galactic Cyg Second-epoch detections are separated by 0.8" and 6.5 pix
The object was found in VSX 2" Gaia DR3 1973711543251798784
Type: ROT
# Max. Min./Amp. JD0 Period
12.070 G 12.120 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:36.89 +43:39:11.3: 12.32 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:36.89 +43:39:11.3: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973711543251798784,2461317.6584,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973711543251798784 20261004.1584 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.19 21:42:53.85 +43:55:35.8
90.80996 -6.87585 galactic Cyg Second-epoch detections are separated by 0.7" and 6.5 pix
The object was found in VSX 0" Vend4
Type: SR
# Max. Min./Amp. JD0 Period
12.500 V 13.500 V 2458342.82420 461.286190900000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:53.85 +43:55:35.8: 12.32 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:53.85 +43:55:35.8: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Vend4,2461317.6584,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Vend4 20261004.1584 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.23 20:50:55.70 +48:52:58.0
88.11175 2.98195 galactic Cyg Second-epoch detections are separated by 0.8" and 5.9 pix
The object was found in VSX 1" ASASSN-V J205055.80+485257.9
Type: EB
# Max. Min./Amp. JD0 Period
12.060 V 12.190 V 2457223.02100 2.580100000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:55.70 +48:52:58.0: 12.17 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:55.70 +48:52:58.0: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205055.80+485257.9,2461317.6584,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205055.80+485257.9 20261004.1584 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 11.12 20:50:38.65 +49:03:16.4
88.21512 3.12696 galactic Cyg Second-epoch detections are separated by 2.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.6609+49.0603 | 20:50:38.73 +49:03:16.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.479+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:38.65 +49:03:16.4: 12.10 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:38.65 +49:03:16.4: 12.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.6609+49.0603,2461317.6584,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.6609+49.0603 20261004.1584 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.43 21:24:01.99 +50:11:05.8
92.69693 -0.10106 galactic Cyg Second-epoch detections are separated by 0.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2171137407292873216 | 21:24:01.77 +50:11:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=2.074+/-0.037 (Very red!)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:24:01.99 +50:11:05.8: 13.83 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:24:01.99 +50:11:05.8: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2171137407292873216,2461317.6584,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2171137407292873216 20261004.1584 12.43CV 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 10 04.1584 2461317.6584 10.94 20:51:56.16 +48:53:47.5
88.22784 2.86286 galactic Cyg Second-epoch detections are separated by 1.1" and 6.0 pix
The object was found in VSX 3" ASASSN-V J205155.92+485349.0
Type: SR
# Max. Min./Amp. JD0 Period
13.270 g Y 0.130 g 2458601.92300 670.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:56.16 +48:53:47.5: 11.83 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:56.16 +48:53:47.5: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205155.92+485349.0,2461317.6584,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205155.92+485349.0 20261004.1584 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.04 20:51:48.04 +50:32:15.1
89.48180 3.92423 galactic Cyg Second-epoch detections are separated by 2.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:51:48.04 +50:32:15.1 (user input) | T | P | (position from user input) J-Ks=0.742+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:48.04 +50:32:15.1: 13.71 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:48.04 +50:32:15.1: 13.68 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461317.6584,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261004.1584 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 10 04.1584 2461317.6584 10.56 21:43:48.59 +45:37:49.7
92.05595 -5.69453 galactic Cyg Second-epoch detections are separated by 0.8" and 6.4 pix
The object was found in VSX 3" NSVS 5982217
Type: SR
# Max. Min./Amp. JD0 Period
13.251 g Y 0.371 g 2458334.86820 146.961757700000 M6
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:43:48.59 +45:37:49.7: 11.52 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:43:48.59 +45:37:49.7: 11.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5982217,2461317.6584,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5982217 20261004.1584 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SS Cyg,2461317.6584,8.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SS Cyg 20261004.1584 8.74CV 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 10 04.1584 2461317.6584 12.38 21:42:39.84 +44:00:47.6
90.83541 -6.78297 galactic Cyg Second-epoch detections are separated by 2.9" and 6.9 pix
The object was found in VSX 2" Gaia DR3 1973741367505281792
Type: SR|M
# Max. Min./Amp. JD0 Period
12.380 G 12.610 G 447.300000000000 M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:42:39.84 +44:00:47.6: 13.58 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:42:39.84 +44:00:47.6: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973741367505281792,2461317.6584,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973741367505281792 20261004.1584 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.39 21:41:20.62 +44:12:11.3
90.78198 -6.48393 galactic Cyg Second-epoch detections are separated by 1.3" and 6.6 pix
The object was found in VSX 1" Gaia DR3 1973761158714377472
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.480 G 13.520 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:41:20.62 +44:12:11.3: 13.66 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:41:20.62 +44:12:11.3: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1973761158714377472,2461317.6584,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1973761158714377472 20261004.1584 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 12.41 21:37:27.43 +43:34:41.6
89.83743 -6.48406 galactic Cyg Second-epoch detections are separated by 1.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.3655+43.5758 | 21:37:27.43 +43:34:41.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M1 (LAMOST DR5) J-Ks=1.273+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:37:27.43 +43:34:41.6: 13.60 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:37:27.43 +43:34:41.6: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J324.3655+43.5758,2461317.6584,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.3655+43.5758 20261004.1584 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.1584 2461317.6584 8.89 20:50:45.92 +50:29:43.7
89.34454 4.02475 galactic Cyg Second-epoch detections are separated by 0.2" and 5.9 pix
The object was found in VSX 2" Gaia DR3 2169700757912222848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
9.500 G 9.520 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:45.92 +50:29:43.7: 9.70 +/- 0.00 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:45.92 +50:29:43.7: 9.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.70 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2169700757912222848,2461317.6584,8.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2169700757912222848 20261004.1584 8.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461245.82532353 24.07.2026 07:48:17.953 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
First image: 2461245.82532353 24.07.2026 07:48:17.953 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Last image: 2461317.65872839 04.10.2026 03:48:24.133 /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
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: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 32305
Objects passed selection criteria: 32091
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 19856
Average stars matched: 19174.5 (96.5678 %)
Memory usage VmPeak: 256048 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Oct 3 04:56:41 CDT 2026
VaST build number 1.0rc89-231-g50972ca5
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 4 00:35:11 CDT 2026
Host name: tau
############################################################
ERROR: large change in astrometric-star counts between the two new images (q2: 1700 -> 2301, 26.119% > 20%; fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits vs fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
ERROR: large change in astrometric-star counts between the two new images (q4: 575 -> 439, 23.652% > 20%; fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits vs fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461245.82532353 24.07.2026 07:48:17.953 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
First image: 2461245.82532353 24.07.2026 07:48:17.953 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Last image: 2461317.65872839 04.10.2026 03:48:24.133 /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 293
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.07
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: 36 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 240262
Objects passed selection criteria: 239418
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 153793
Average stars matched: 147187 (95.7046 %)
Memory usage VmPeak: 696812 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Oct 3 04:56:41 CDT 2026
VaST build number 1.0rc89-231-g50972ca5
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 4 00:36:49 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
SExtractor catalog cache: saved Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.cat to cache
SExtractor catalog cache: saved Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.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-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461317.65802685
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'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits exists and is non-empty
wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits exists and is non-empty
wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits exists and is non-empty
wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits (1st reference image)
verification OK: wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Image size: 937.3'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: 21:36:03.270 +46:00:36.57 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-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits (1st new image)
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:36:00.976 +45:59:23.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:36:03.270 +46:00:36.57
Second-epoch image center 21:36:00.976 +45:59:23.51
Angular distance between the image centers 0.0214 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits (2nd new image)
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:35:59.068 +45:58:51.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:36:03.270 +46:00:36.57
Second-epoch image center 21:35:59.068 +45:58:51.01
Angular distance between the image centers 0.0317 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 21:36:00.976 +45:59:23.51
Second-epoch second image center 21:35:59.068 +45:58:51.01
Angular distance between the image centers 0.01058 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits &> /tmp/tmp.p6MVnS3o0a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits &> /tmp/tmp.t0ms94V8Tm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits &> /tmp/tmp.5mkPJEWfY8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits &> /tmp/tmp.KfoinHwIyf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.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-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits and wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.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-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits and wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
Found non-empty wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits and wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
The reference image (wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits) and catalog (wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat) found
'wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat' -> 'wcsmag.cat'
Read 34895 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 311.6628 to 336.3203 deg, Dec +40.3089 to +51.2694 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 311.6628 to 336.3203 deg, Dec 40.3089 to 51.2694 deg
Loaded 22786 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): 15376 out of 17092 total matches.
Matched with Tycho-2 17092 out of 34895 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.639650
a=0.000000 b=1.000000 c=22.639650
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34895 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 311.6628 to 336.3203 deg, Dec +40.3089 to +51.2694 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 311.6628 to 336.3203 deg, Dec 40.3089 to 51.2694 deg
Loaded 22786 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): 15376 out of 17092 total matches.
Matched with Tycho-2 17092 out of 34895 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Forced-photometry filter: calibrated wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits -> calib.txt_param_ref_wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits (aperture=6.3)
Read 34846 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 311.6977 to 336.3366 deg, Dec +40.3085 to +51.2755 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 311.6977 to 336.3366 deg, Dec 40.3085 to 51.2755 deg
Loaded 22774 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): 15460 out of 17160 total matches.
Matched with Tycho-2 17160 out of 34846 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
Forced-photometry filter: calibrated wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits -> calib.txt_param_ref_wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
2.2 pix Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
3.0 pix fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
3.3 pix fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
Limiting magnitude estimates:
15.3 mag. Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
15.2 mag. Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
12.0 mag. fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
12.9 mag. fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
All-image limiting magnitude estimate: 12.0 (SNR ) 10.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.p6MVnS3o0a (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.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-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits' -> 'wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Checking if the catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
WCS catalog name: wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4028, bad_region=0, passed=34895
Got 34895 stars (including 30831 good ones) from the SExtractor catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 34895 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 4927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 34895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 34895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 34895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4925 stars left (next iteration limit 5419)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits N_match=4925 sigma_overall_arcsec=0.629 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.750 sigma_q3_arcsec=0.574 sigma_q4_arcsec=0.725 n_q1=1127 n_q2=1072 n_q3=1228 n_q4=1498 worst_quadrant_to_overall_ratio=1.191
The image catalog is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits -region wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.t0ms94V8Tm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.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-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits' -> 'wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
WCS-calibrated image found: wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
Checking if the catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat corresponding to the image wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat corresponding to the image wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
WCS catalog name: wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3993, bad_region=0, passed=34846
Got 34846 stars (including 30830 good ones) from the SExtractor catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat
util/solve_plate_with_UCAC5 got 34846 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 4923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 34846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 34846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 34846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 4922 stars left (next iteration limit 5415)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits N_match=4922 sigma_overall_arcsec=0.616 sigma_q1_arcsec=0.460 sigma_q2_arcsec=0.738 sigma_q3_arcsec=0.548 sigma_q4_arcsec=0.693 n_q1=1113 n_q2=1072 n_q3=1245 n_q4=1492 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits -region wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.5mkPJEWfY8 (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_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.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_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
Checking if the catalog wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
WCS catalog name: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=149, bad_region=0, passed=4688
Got 4688 stars (including 4536 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat
util/solve_plate_with_UCAC5 got 4688 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4473 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4426 matched stars entering correct_measured_positions(), 4425 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4426 matched stars entering correct_measured_positions(), 4684 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4472 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4426 matched stars entering correct_measured_positions(), 4685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4426 matched stars entering correct_measured_positions(), 4685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4426 stars left (next iteration limit 4868)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4426 robust_rms=9.035 arcsec worst_region_rms=31.211 arcsec outer_annulus_rms=31.211 arcsec
SIP_REFIT: SIP order 3 trial: matched=4426 robust_rms=0.531 arcsec worst_region_rms=1.008 arcsec outer_annulus_rms=1.008 arcsec
SIP_REFIT: SIP order 5 trial: matched=4426 robust_rms=0.449 arcsec worst_region_rms=0.779 arcsec outer_annulus_rms=0.779 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4426 robust_rms_before=0.771 arcsec robust_rms_before_corrected=0.496 arcsec robust_rms_after=0.449 arcsec worst_region_rms_before=1.015 worst_region_rms_after=0.779 outer_annulus_rms_before=1.203 outer_annulus_rms_after=0.779
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:36:01.012 +45:59:23.52 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 4688 stars ###
'wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/correct_sextractor_wcs_catalog_usingxy2sky2885005.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.771 -> 0.449 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4426 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4212 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4212 pairs (4426 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4212 robust_rms=8.395 arcsec worst_region_rms=32.451 arcsec outer_annulus_rms=32.451 arcsec
SIP_REFIT: SIP order 3 trial: matched=4212 robust_rms=0.526 arcsec worst_region_rms=0.966 arcsec outer_annulus_rms=0.966 arcsec
SIP_REFIT: SIP order 5 trial: matched=4212 robust_rms=0.443 arcsec worst_region_rms=0.763 arcsec outer_annulus_rms=0.763 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4212 robust_rms_before=0.443 arcsec robust_rms_before_corrected=0.443 arcsec robust_rms_after=0.443 arcsec worst_region_rms_before=0.763 worst_region_rms_after=0.763 outer_annulus_rms_before=0.763 outer_annulus_rms_after=0.763
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-region 0.763 vs 0.763 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4212 matched stars entering correct_measured_positions(), 4683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4212 matched stars entering correct_measured_positions(), 4683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WCS_QUALITY_DIAG: file=fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits N_match=4212 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.487 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.422 n_q1=1084 n_q2=1700 n_q3=853 n_q4=575 worst_quadrant_to_overall_ratio=1.085
The image catalog is written to wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits -region wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.KfoinHwIyf (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_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.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_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
Checking if the catalog wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
WCS catalog name: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=185, bad_region=0, passed=5475
Got 5475 stars (including 5285 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat
util/solve_plate_with_UCAC5 got 5475 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 4883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 5469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.3)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 5469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 5469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 4884 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4884 robust_rms=13.087 arcsec worst_region_rms=16.991 arcsec outer_annulus_rms=16.991 arcsec
SIP_REFIT: SIP order 3 trial: matched=4884 robust_rms=0.599 arcsec worst_region_rms=1.002 arcsec outer_annulus_rms=1.002 arcsec
SIP_REFIT: SIP order 5 trial: matched=4884 robust_rms=0.455 arcsec worst_region_rms=0.869 arcsec outer_annulus_rms=0.869 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4884 robust_rms_before=0.828 arcsec robust_rms_before_corrected=0.563 arcsec robust_rms_after=0.455 arcsec worst_region_rms_before=0.998 worst_region_rms_after=0.869 outer_annulus_rms_before=1.168 outer_annulus_rms_after=0.869
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:35:59.104 +45:58:51.03 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5475 stars ###
'wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/correct_sextractor_wcs_catalog_usingxy2sky2885095.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.828 -> 0.455 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4884 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.3)
Done reading UCAC5 zone files...
Matched 4660 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4660 pairs (4884 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4660 robust_rms=12.802 arcsec worst_region_rms=17.314 arcsec outer_annulus_rms=17.314 arcsec
SIP_REFIT: SIP order 3 trial: matched=4660 robust_rms=0.588 arcsec worst_region_rms=0.956 arcsec outer_annulus_rms=0.956 arcsec
SIP_REFIT: SIP order 5 trial: matched=4660 robust_rms=0.446 arcsec worst_region_rms=0.813 arcsec outer_annulus_rms=0.813 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4660 robust_rms_before=0.446 arcsec robust_rms_before_corrected=0.446 arcsec robust_rms_after=0.446 arcsec worst_region_rms_before=0.815 worst_region_rms_after=0.813 outer_annulus_rms_before=0.815 outer_annulus_rms_after=0.813
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:35:59.105 +45:58:51.02 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5475 stars ###
'wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/correct_sextractor_wcs_catalog_usingxy2sky2885198.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.446 -> 0.446 arcsec)
Accuracy estimation diagnostic: 4660 matched stars entering correct_measured_positions(), 5469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4660 matched stars entering correct_measured_positions(), 5468 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
WCS_QUALITY_DIAG: file=fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits N_match=4660 sigma_overall_arcsec=0.504 sigma_q1_arcsec=0.458 sigma_q2_arcsec=0.549 sigma_q3_arcsec=0.385 sigma_q4_arcsec=0.470 n_q1=944 n_q2=2301 n_q3=976 n_q4=439 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits -region wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits to local_wcs_cache/
'wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits'
Saving the final (post-refit) wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits to local_wcs_cache/
'wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits'
Saving the final (post-refit) wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits'
Saving the final (post-refit) wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits sigma_overall=0.629 worst_q_ratio=1.191
ref2=Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits sigma_overall=0.616 worst_q_ratio=1.197
new1=fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits sigma_overall=0.459 worst_q_ratio=1.085
new2=fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits sigma_overall=0.504 worst_q_ratio=1.088
reference average sigma_overall=0.6225 worst_q_ratio=1.194
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: large change in astrometric-star counts between the two new images (q2: 1700 -> 2301, 26.119% > 20%; fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits vs fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
ERROR: large change in astrometric-star counts between the two new images (q4: 575 -> 439, 23.652% > 20%; fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits vs fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132_astrometric_residuals.png (4925 matched stars from wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133_astrometric_residuals.png (4922 matched stars from wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034_astrometric_residuals.png (4212 matched stars from wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035_astrometric_residuals.png (4660 matched stars from wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-03_CI_Cyg-04-Q1b1x1_224924_TTUQ1b1x1_3413026_d2qdGK5d/wcs_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits'
Preparing the HTML report for the field Cyg-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:46.41 +50:22:36.4: 11.00 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:45.71 +50:21:50.8: 11.44 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:05.79 +50:26:41.7: 11.05 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:43.72 +50:27:45.2: 10.72 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:50:26.16 +49:13:24.7: 11.67 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:49:37.51 +50:24:52.9: 10.95 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:12.21 +50:12:01.2: 11.23 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:52:42.25 +50:27:26.3: 11.41 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:50:26.16 +49:13:24.7: 11.65 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:43.72 +50:27:45.2: 10.79 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:05.79 +50:26:41.7: 11.01 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:45.71 +50:21:50.8: 11.41 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:46.41 +50:22:36.4: 11.01 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:12.21 +50:12:01.2: 11.22 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:49:37.51 +50:24:52.9: 10.95 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:52:42.25 +50:27:26.3: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Forced photometry reference-image weighted average: 11.03 +/- 0.01
Forced photometry reference-image weighted average: 10.75 +/- 0.00
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:51:04.60 +50:25:11.0: 11.43 +/- 0.01 detection
Forced photometry filter KEPT candidate at 20:50:26.16 +49:13:24.7: ref_mag=11.66 +/- 0.01 new_mean_mag=10.6882 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 11.43 +/- 0.01
Forced photometry filter KEPT candidate at 20:51:05.79 +50:26:41.7: ref_mag=11.03 +/- 0.01 new_mean_mag=9.9950 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 20:51:43.72 +50:27:45.2: ref_mag=10.75 +/- 0.00 new_mean_mag=9.8107 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 11.01 +/- 0.01
Forced photometry reference-image weighted average: 11.23 +/- 0.01
Forced photometry filter KEPT candidate at 20:49:45.71 +50:21:50.8: ref_mag=11.43 +/- 0.01 new_mean_mag=10.3056 delta=1.12 (need > 0.90)
Forced photometry filter KEPT candidate at 20:49:46.41 +50:22:36.4: ref_mag=11.01 +/- 0.01 new_mean_mag=9.9977 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 10.95 +/- 0.01
Forced photometry reference-image weighted average: 11.39 +/- 0.01
Forced photometry filter KEPT candidate at 20:51:12.21 +50:12:01.2: ref_mag=11.23 +/- 0.01 new_mean_mag=10.1799 delta=1.05 (need > 0.90)
Forced photometry filter KEPT candidate at 20:49:37.51 +50:24:52.9: ref_mag=10.95 +/- 0.01 new_mean_mag=9.9137 delta=1.04 (need > 0.90)
Forced photometry filter KEPT candidate at 20:52:42.25 +50:27:26.3: ref_mag=11.39 +/- 0.01 new_mean_mag=10.2371 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:51:04.60 +50:25:11.0: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Forced photometry filter KEPT candidate at 20:51:04.60 +50:25:11.0: ref_mag=11.42 +/- 0.01 new_mean_mag=10.2504 delta=1.17 (need > 0.90)
Adding exclusion_list_local.txt__out29640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34585.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
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: 4s
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Considering the candidate 34042_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 34042_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 07557_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 07557_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 34585_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 34585_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 34012_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 34012_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 33958_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 33958_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 33885_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 33885_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 28707_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 28707_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 299572_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 299572_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:41:59.34 +45:47:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299780_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 299780_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:42:11.87 +45:44:10.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 299808_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 299808_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:08:33.73 +47:15:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299834_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 299834_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 299926_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 299926_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:10:39.66 +47:41:52.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 299984_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 299984_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 20:51:37.08 +47:09:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300149_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 300149_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:22:41.61 +49:28:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300203_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 300203_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:15:43.88 +47:57:20.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 300270_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 300270_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 300273_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 300273_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:30:25.99 +50:09:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60207_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 60207_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 69890_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 69890_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 60821_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 60821_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 255472_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 255472_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 74216_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 74216_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 255796_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 255796_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 59345_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 59345_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 237533_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 237533_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 255825_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 255825_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 61286_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 61286_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 62599_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 62599_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 236900_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 236900_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 238581_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 238581_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 257925_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 257925_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 73256_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 73256_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 72092_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 72092_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 255344_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 255344_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 55130_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 55130_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 234982_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 234982_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 237960_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 237960_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 79072_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 79072_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 58665_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 58665_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68524_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68524_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 63123_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 63123_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 218865_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 218865_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 233474_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 233474_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 66119_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 66119_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 207740_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 207740_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 60947_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 60947_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 209947_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 209947_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 61071_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 61071_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 64981_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 64981_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 66849_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 66849_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 109506_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 109506_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 54160_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 54160_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 192268_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 192268_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68588_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68588_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 57138_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 57138_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 191305_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 191305_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 243339_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 243339_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 232067_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 232067_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (36.4") between the two second-epoch detections
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Considering the candidate 256524_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 256524_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 189529_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 189529_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 54309_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 54309_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 61570_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 61570_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 76621_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 76621_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 72194_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 72194_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 62993_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 62993_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 75170_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 75170_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 227556_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 227556_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (38.4") between the two second-epoch detections
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Considering the candidate 254446_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 254446_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 57993_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 57993_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 55451_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 55451_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 65370_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 65370_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 60841_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 60841_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 217963_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 217963_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:16:50.98 +50:23:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54676_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 54676_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 240161_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 240161_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 58185_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 58185_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 257980_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 257980_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (36.0") between the two second-epoch detections
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Considering the candidate 63353_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 63353_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 89887_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 89887_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:42:03.44 +44:57:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60605_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 60605_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 67188_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 67188_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 61836_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 61836_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 69176_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 69176_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 81097_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 81097_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 57342_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 57342_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 70842_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 70842_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 263025_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 263025_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 86794_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 86794_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 62226_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 62226_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 173865_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 173865_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 69380_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 69380_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 69137_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 69137_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 192966_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 192966_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (37.2") between the two second-epoch detections
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Considering the candidate 65305_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 65305_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 112834_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 112834_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (38.1") between the two second-epoch detections
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Considering the candidate 76035_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 76035_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 69666_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 69666_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 209902_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 209902_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 63656_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 63656_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 13257_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 13257_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (38.6") between the two second-epoch detections
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Considering the candidate 237939_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 237939_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 244871_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 244871_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 64247_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 64247_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 59003_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 59003_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 280858_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 280858_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (34.6") between the two second-epoch detections
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Considering the candidate 70991_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 70991_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68642_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68642_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 107819_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 107819_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 23043_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 23043_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (38.2") between the two second-epoch detections
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Considering the candidate 61794_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 61794_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 71745_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 71745_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 63488_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 63488_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 203463_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 203463_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 125153_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 125153_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (37.9") between the two second-epoch detections
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Considering the candidate 66843_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 66843_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68097_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68097_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 64372_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 64372_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68988_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68988_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 58454_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 58454_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 112145_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 112145_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 87733_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 87733_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 73259_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 73259_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 256430_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 256430_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 71428_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 71428_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 102584_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 102584_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 75458_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 75458_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 70689_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 70689_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 67633_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 67633_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 235871_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 235871_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 51136_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 51136_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 253512_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 253512_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 60415_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 60415_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 191055_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 191055_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (38.3") between the two second-epoch detections
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Considering the candidate 67801_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 67801_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 238277_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 238277_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 72150_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 72150_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 73776_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 73776_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68129_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68129_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 66923_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 66923_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 50477_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 50477_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 66061_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 66061_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 253521_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 253521_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 84025_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 84025_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 56296_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 56296_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 64196_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 64196_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 105304_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 105304_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 80184_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 80184_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 237690_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 237690_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 53058_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 53058_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 195323_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 195323_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:39:39.02 +48:26:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60357_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 60357_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 78158_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 78158_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 165891_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 165891_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (36.4") between the two second-epoch detections
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Considering the candidate 63513_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 63513_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 74296_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 74296_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68214_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68214_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 67850_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 67850_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 257028_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 257028_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (37.4") between the two second-epoch detections
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Considering the candidate 54002_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 54002_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 235507_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 235507_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 216091_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 216091_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:13:05.40 +50:25:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231239_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 231239_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 59140_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 59140_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 71141_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 71141_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 236086_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 236086_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 171066_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 171066_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 73152_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 73152_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68344_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68344_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 263078_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 263078_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (38.0") between the two second-epoch detections
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Considering the candidate 69900_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 69900_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 68033_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 68033_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 230198_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 230198_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 60805_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 60805_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 78699_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 78699_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 66178_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 66178_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 74632_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 74632_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 62302_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 62302_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 62188_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 62188_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 63932_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 63932_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 58025_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 58025_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 70008_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 70008_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 65708_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 65708_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 04390_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 04390_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (40.4") between the two second-epoch detections
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Considering the candidate 255226_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 255226_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 232371_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 232371_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:29:39.63 +49:49:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64482_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 64482_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:41:01.21 +43:56:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64165_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 64165_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 78010_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 78010_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 202157_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 202157_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 233133_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 233133_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 237959_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 237959_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 69370_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 69370_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 71504_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 71504_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 49275_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 49275_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:39:40.79 +43:18:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256483_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 256483_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 238252_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 238252_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 242988_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 242988_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 59875_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 59875_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 57110_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 57110_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 238258_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 238258_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 136542_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 136542_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 21:41:11.64 +46:31:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57310_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 57310_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 64233_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 64233_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 243199_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 243199_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 36854_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 36854_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (39.5") between the two second-epoch detections
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Considering the candidate 237950_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 237950_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 223163_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 223163_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 242395_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 242395_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 233517_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 233517_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
**** FOUND 20:50:26.13 +49:13:25.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 254035_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 254035_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 111099_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 111099_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 56047_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 56047_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 65602_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 65602_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 69891_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 69891_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 138451_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 138451_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (40.0") between the two second-epoch detections
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Considering the candidate 69297_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 69297_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
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Considering the candidate 55273_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 55273_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 98762_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 98762_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (39.7") between the two second-epoch detections
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Considering the candidate 254220_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
Preparing report for the candidate 254220_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
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Considering the candidate 14772_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035
The candidate 14772_fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035 did not pass the final checks
Rejecting candidate due to large distance (40.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 14s
make_report_in_HTML.sh TOTAL: 237s
Prepared the HTML report for the field Cyg-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:51:04.60 +50:25:11.0
20:50:26.16 +49:13:24.7
20:49:37.51 +50:24:52.9
20:49:46.41 +50:22:36.4
20:51:43.72 +50:27:45.2
20:51:05.79 +50:26:41.7
20:49:45.71 +50:21:50.8
20:52:42.25 +50:27:26.3
20:51:12.21 +50:12:01.2
21:45:11.48 +45:25:21.5
21:44:43.54 +45:30:10.4
21:44:14.84 +45:35:57.6
21:45:40.60 +45:38:54.6
21:43:48.59 +45:37:49.7
21:45:09.78 +45:43:57.9
21:28:36.73 +48:15:41.1
21:28:31.62 +48:19:14.0
21:28:06.13 +48:20:54.6
21:39:13.07 +48:41:33.9
21:21:43.45 +48:41:45.6
21:27:55.72 +48:53:28.8
21:26:55.09 +48:57:44.0
21:23:05.05 +48:55:25.7
21:15:02.83 +50:17:58.7
21:24:01.99 +50:11:05.8
20:50:08.10 +49:21:40.0
20:50:19.79 +49:19:18.5
21:30:36.63 +49:51:16.9
20:50:05.56 +49:13:57.8
20:50:08.66 +49:09:12.8
20:50:57.80 +49:10:08.2
20:50:35.73 +49:08:24.0
20:50:36.51 +49:07:48.8
20:51:13.15 +49:07:13.9
20:51:11.94 +49:04:19.5
20:50:49.44 +49:04:34.0
20:52:20.39 +49:05:57.2
20:50:38.65 +49:03:16.4
20:50:56.12 +49:04:13.6
20:50:23.96 +49:04:34.7
20:51:27.17 +49:04:07.0
20:51:28.89 +49:03:48.5
20:50:26.01 +49:01:53.9
20:50:39.04 +49:01:04.8
20:50:40.80 +48:59:01.0
20:51:56.16 +48:53:47.5
20:50:47.20 +48:51:48.7
20:50:55.70 +48:52:58.0
20:52:07.65 +48:52:24.5
21:25:54.68 +49:22:23.7
20:50:19.67 +50:31:03.9
20:51:48.04 +50:32:15.1
20:50:45.92 +50:29:43.7
20:49:30.79 +50:27:22.5
20:49:55.60 +50:26:15.0
20:50:21.21 +50:26:08.3
20:51:00.98 +50:27:14.4
20:49:50.79 +50:26:08.0
20:50:14.79 +50:28:25.5
20:51:01.44 +50:24:15.3
20:50:58.13 +50:24:12.4
20:52:01.94 +50:26:37.7
20:50:19.46 +50:24:28.8
21:12:01.13 +50:30:46.6
21:39:07.89 +43:21:35.7
21:40:55.30 +43:23:10.2
21:42:05.20 +43:28:02.8
21:42:02.75 +43:29:48.7
21:41:21.18 +43:31:18.1
21:40:45.67 +43:31:46.6
21:42:37.29 +43:32:25.6
21:40:11.53 +43:33:30.8
21:37:27.43 +43:34:41.6
21:41:40.87 +43:34:42.4
21:43:14.68 +43:36:25.5
21:40:42.04 +43:38:53.2
21:42:02.02 +43:38:59.8
21:41:36.89 +43:39:11.3
21:40:43.45 +43:39:25.9
21:40:16.53 +43:41:28.6
21:41:57.27 +43:40:45.4
21:42:21.99 +43:41:44.1
21:42:01.92 +43:42:27.6
21:41:04.59 +43:42:38.9
21:37:43.61 +43:44:13.7
21:40:24.93 +43:44:24.5
21:40:38.14 +43:44:28.7
21:41:21.14 +43:46:10.9
21:41:45.97 +43:47:14.2
21:41:09.73 +43:47:22.3
21:41:11.45 +43:47:54.2
21:41:41.43 +43:48:23.6
21:40:37.16 +43:48:47.5
21:41:18.70 +43:48:56.3
21:39:07.45 +43:49:17.0
21:41:44.21 +43:49:09.6
21:40:43.31 +43:49:30.5
21:39:52.23 +43:50:53.7
21:38:41.33 +43:51:44.8
21:42:25.60 +43:51:20.1
21:41:49.27 +43:52:18.3
21:40:12.92 +43:52:03.8
21:41:20.31 +43:52:27.2
21:41:43.92 +43:52:22.8
21:40:26.91 +43:54:44.3
21:42:57.32 +43:54:22.5
21:41:25.95 +43:55:28.2
21:40:54.20 +43:55:55.0
21:42:52.08 +43:55:03.2
21:42:36.82 +43:55:55.5
21:42:05.79 +43:56:24.1
21:41:02.22 +43:56:55.5
21:40:42.41 +43:57:37.8
21:42:53.85 +43:55:35.8
21:42:30.77 +43:57:27.3
21:40:54.90 +43:57:59.3
21:42:38.88 +43:59:12.5
21:40:23.49 +44:00:23.2
21:40:59.63 +44:00:04.8
21:42:39.84 +44:00:47.6
21:39:19.20 +44:00:46.3
21:41:36.67 +44:02:03.5
21:39:48.96 +44:02:03.4
21:41:08.78 +44:01:21.4
21:40:44.51 +44:04:07.0
21:41:46.94 +44:03:58.9
21:41:19.21 +44:04:16.1
21:40:38.90 +44:05:14.7
21:42:16.86 +44:05:41.1
21:41:44.75 +44:06:22.5
21:42:29.68 +44:06:23.5
21:41:16.73 +44:07:02.1
21:39:04.37 +44:07:38.6
21:42:39.01 +44:06:48.7
21:40:36.79 +44:07:30.9
21:40:29.65 +44:08:05.1
21:43:26.88 +44:08:01.8
21:42:48.44 +44:08:08.0
21:41:35.44 +44:08:45.4
21:39:59.14 +44:09:50.6
21:42:07.35 +44:09:55.1
21:41:48.82 +44:10:05.6
21:40:09.03 +44:10:03.6
21:40:04.32 +44:10:32.7
21:40:48.22 +44:11:21.3
21:41:11.98 +44:11:42.8
21:41:20.62 +44:12:11.3
21:41:58.48 +44:11:35.6
21:42:01.66 +44:11:54.1
21:45:28.02 +44:12:35.8
21:41:25.84 +44:13:55.0
21:41:19.20 +44:14:36.5
21:41:49.52 +44:14:22.6
21:39:15.45 +44:15:53.0
21:41:49.42 +44:15:10.4
21:42:10.34 +44:16:04.1
21:37:41.38 +44:16:34.7
21:39:44.02 +44:17:42.2
21:41:08.31 +44:17:24.1
21:41:12.10 +44:19:42.7
21:40:10.81 +44:19:47.1
21:42:38.05 +44:19:35.4
21:41:22.43 +44:21:27.6
21:39:57.12 +44:20:58.4
21:40:06.08 +44:22:23.2
21:41:02.78 +44:23:06.9
21:38:35.60 +44:25:10.0
21:41:27.90 +44:25:30.0
21:41:46.25 +44:26:44.8
21:38:55.14 +44:28:22.9
21:40:54.19 +44:30:41.3
21:41:32.66 +44:31:33.9
21:40:26.78 +44:33:27.1
21:39:16.47 +44:34:15.5
21:40:51.19 +44:36:41.5
21:39:56.69 +44:39:34.3
21:42:09.79 +44:45:56.8
21:43:07.46 +44:54:07.6
Source monitoring: NOT measuring the monitored positions on the field Cyg-04-Q1b1x1 - the transient search raised a processing error: ERROR: large change in astrometric-star counts between the two new images (q2: 1700 -> 2301, 26.119% > 20%; fd_Cyg-04-Q1b1x1_2026-10-03_22-47-23_20.00sec_-0.00C_LIGHTs_0034.fits vs fd_Cyg-04-Q1b1x1_2026-10-03_22-48-24_20.00sec_-0.00C_LIGHTs_0035.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
Source monitoring: the monitored positions on the field Cyg-04-Q1b1x1 are recorded as run_error (rejected by this run, never measured later)
########### Completed Cyg-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
20:52:42.25 +50:27:26.3
21:42:43.06 +43:35:11.1
20:51:12.21 +50:12:01.2
20:51:05.79 +50:26:41.7
20:49:46.41 +50:22:36.4
20:49:37.51 +50:24:52.9
20:51:43.72 +50:27:45.2
20:50:26.16 +49:13:24.7
20:49:45.71 +50:21:50.8
20:51:04.60 +50:25:11.0
21:41:45.97 +43:47:14.2
21:41:11.98 +44:11:42.8
21:41:18.70 +43:48:56.3
20:51:00.98 +50:27:14.4
21:39:57.12 +44:20:58.4
20:49:50.79 +50:26:08.0
21:40:38.14 +43:44:28.7
20:51:11.94 +49:04:19.5
20:50:14.79 +50:28:25.5
21:40:43.31 +43:49:30.5
21:41:43.92 +43:52:22.8
20:51:13.15 +49:07:13.9
20:50:39.04 +49:01:04.8
20:50:19.46 +50:24:28.8
21:40:10.81 +44:19:47.1
21:37:41.38 +44:16:34.7
20:50:21.21 +50:26:08.3
21:40:11.53 +43:33:30.8
20:50:08.66 +49:09:12.8
20:50:23.96 +49:04:34.7
21:39:16.47 +44:34:15.5
21:41:04.59 +43:42:38.9
21:43:26.88 +44:08:01.8
21:42:57.32 +43:54:22.5
21:15:02.83 +50:17:58.7
20:50:05.56 +49:13:57.8
21:39:48.96 +44:02:03.4
21:27:55.72 +48:53:28.8
21:41:44.21 +43:49:09.6
21:23:05.05 +48:55:25.7
21:42:38.88 +43:59:12.5
21:41:46.94 +44:03:58.9
21:45:40.60 +45:38:54.6
21:41:21.18 +43:31:18.1
21:28:06.13 +48:20:54.6
21:42:48.44 +44:08:08.0
21:42:02.02 +43:38:59.8
21:28:31.62 +48:19:14.0
20:52:07.65 +48:52:24.5
20:52:01.94 +50:26:37.7
21:28:36.73 +48:15:41.1
21:40:45.67 +43:31:46.6
21:39:52.23 +43:50:53.7
21:38:55.14 +44:28:22.9
21:41:08.31 +44:17:24.1
21:40:26.91 +43:54:44.3
21:38:35.60 +44:25:10.0
20:49:30.79 +50:27:22.5
21:40:16.53 +43:41:28.6
21:41:40.87 +43:34:42.4
21:40:59.63 +44:00:04.8
21:39:07.45 +43:49:17.0
21:42:37.29 +43:32:25.6
20:50:40.80 +48:59:01.0
21:42:21.99 +43:41:44.1
21:41:25.95 +43:55:28.2
21:41:41.43 +43:48:23.6
21:40:38.90 +44:05:14.7
21:42:25.60 +43:51:20.1
21:41:48.82 +44:10:05.6
21:39:56.69 +44:39:34.3
21:40:43.45 +43:39:25.9
21:41:25.84 +44:13:55.0
21:12:01.13 +50:30:46.6
21:40:12.92 +43:52:03.8
21:40:04.32 +44:10:32.7
21:42:07.35 +44:09:55.1
21:40:23.49 +44:00:23.2
21:41:46.25 +44:26:44.8
21:40:48.22 +44:11:21.3
21:26:55.09 +48:57:44.0
21:42:36.82 +43:55:55.5
20:52:20.39 +49:05:57.2
21:25:54.68 +49:22:23.7
21:42:30.77 +43:57:27.3
21:37:43.61 +43:44:13.7
21:41:19.20 +44:14:36.5
21:41:35.44 +44:08:45.4
21:44:14.84 +45:35:57.6
21:38:41.33 +43:51:44.8
21:42:10.34 +44:16:04.1
21:40:54.20 +43:55:55.0
21:21:43.45 +48:41:45.6
21:40:44.51 +44:04:07.0
21:39:04.37 +44:07:38.6
21:40:54.90 +43:57:59.3
21:39:59.14 +44:09:50.6
21:42:01.92 +43:42:27.6
21:45:09.78 +45:43:57.9
21:43:07.46 +44:54:07.6
21:42:38.05 +44:19:35.4
20:51:01.44 +50:24:15.3
21:39:15.45 +44:15:53.0
21:45:11.48 +45:25:21.5
21:41:27.90 +44:25:30.0
21:45:28.02 +44:12:35.8
21:42:16.86 +44:05:41.1
20:50:35.73 +49:08:24.0
21:40:55.30 +43:23:10.2
20:50:19.67 +50:31:03.9
21:41:11.45 +43:47:54.2
21:41:44.75 +44:06:22.5
20:50:26.01 +49:01:53.9
21:39:44.02 +44:17:42.2
21:41:22.43 +44:21:27.6
21:42:39.01 +44:06:48.7
21:41:19.21 +44:04:16.1
21:39:07.89 +43:21:35.7
21:41:36.67 +44:02:03.5
21:42:09.79 +44:45:56.8
21:43:14.68 +43:36:25.5
21:40:42.41 +43:57:37.8
21:44:43.54 +45:30:10.4
21:40:51.19 +44:36:41.5
20:50:49.44 +49:04:34.0
21:42:05.20 +43:28:02.8
21:41:09.73 +43:47:22.3
21:41:32.66 +44:31:33.9
21:42:52.08 +43:55:03.2
21:40:06.08 +44:22:23.2
21:40:36.79 +44:07:30.9
21:42:29.68 +44:06:23.5
21:42:02.75 +43:29:48.7
20:50:57.80 +49:10:08.2
20:50:19.79 +49:19:18.5
21:40:24.93 +43:44:24.5
21:41:49.52 +44:14:22.6
20:50:36.51 +49:07:48.8
21:41:12.10 +44:19:42.7
21:40:29.65 +44:08:05.1
21:41:58.48 +44:11:35.6
21:41:16.73 +44:07:02.1
20:50:08.10 +49:21:40.0
21:40:37.16 +43:48:47.5
21:40:26.78 +44:33:27.1
21:41:08.78 +44:01:21.4
21:41:02.78 +44:23:06.9
21:41:20.31 +43:52:27.2
21:41:49.27 +43:52:18.3
21:42:05.79 +43:56:24.1
21:41:57.27 +43:40:45.4
21:42:01.66 +44:11:54.1
21:39:19.20 +44:00:46.3
20:49:55.60 +50:26:15.0
21:41:02.22 +43:56:55.5
21:40:54.19 +44:30:41.3
21:39:13.07 +48:41:33.9
21:30:36.63 +49:51:16.9
20:50:56.12 +49:04:13.6
21:40:09.03 +44:10:03.6
21:41:49.42 +44:15:10.4
20:50:58.13 +50:24:12.4
20:51:27.17 +49:04:07.0
20:50:47.20 +48:51:48.7
21:41:21.14 +43:46:10.9
21:40:42.04 +43:38:53.2
20:51:28.89 +49:03:48.5
21:41:36.89 +43:39:11.3
21:42:53.85 +43:55:35.8
20:50:55.70 +48:52:58.0
20:50:38.65 +49:03:16.4
21:24:01.99 +50:11:05.8
20:51:56.16 +48:53:47.5
20:51:48.04 +50:32:15.1
21:43:48.59 +45:37:49.7
21:42:43.07 +43:35:11.2
21:42:39.84 +44:00:47.6
21:41:20.62 +44:12:11.3
21:37:27.43 +43:34:41.6
20:50:45.92 +50:29:43.7
###################################################################################
20:52:42.25 +50:27:26.3 -- not an asteroid (will add it to exclusion list)
21:42:43.06 +43:35:11.1 -- listed in neverexclude_list.txt (will NOT add it to exclusion list)
20:51:12.21 +50:12:01.2 -- not an asteroid (will add it to exclusion list)
20:51:05.79 +50:26:41.7 -- not an asteroid (will add it to exclusion list)
20:49:46.41 +50:22:36.4 -- not an asteroid (will add it to exclusion list)
20:49:37.51 +50:24:52.9 -- not an asteroid (will add it to exclusion list)
20:51:43.72 +50:27:45.2 -- not an asteroid (will add it to exclusion list)
20:50:26.16 +49:13:24.7 -- not an asteroid (will add it to exclusion list)
20:49:45.71 +50:21:50.8 -- not an asteroid (will add it to exclusion list)
20:51:04.60 +50:25:11.0 -- not an asteroid (will add it to exclusion list)
21:41:45.97 +43:47:14.2 -- not an asteroid (will add it to exclusion list)
21:41:11.98 +44:11:42.8 -- not an asteroid (will add it to exclusion list)
21:41:18.70 +43:48:56.3 -- not an asteroid (will add it to exclusion list)
20:51:00.98 +50:27:14.4 -- not an asteroid (will add it to exclusion list)
21:39:57.12 +44:20:58.4 -- not an asteroid (will add it to exclusion list)
20:49:50.79 +50:26:08.0 -- not an asteroid (will add it to exclusion list)
21:40:38.14 +43:44:28.7 -- not an asteroid (will add it to exclusion list)
20:51:11.94 +49:04:19.5 -- not an asteroid (will add it to exclusion list)
20:50:14.79 +50:28:25.5 -- not an asteroid (will add it to exclusion list)
21:40:43.31 +43:49:30.5 -- not an asteroid (will add it to exclusion list)
21:41:43.92 +43:52:22.8 -- not an asteroid (will add it to exclusion list)
20:51:13.15 +49:07:13.9 -- not an asteroid (will add it to exclusion list)
20:50:39.04 +49:01:04.8 -- not an asteroid (will add it to exclusion list)
20:50:19.46 +50:24:28.8 -- not an asteroid (will add it to exclusion list)
21:40:10.81 +44:19:47.1 -- not an asteroid (will add it to exclusion list)
21:37:41.38 +44:16:34.7 -- not an asteroid (will add it to exclusion list)
20:50:21.21 +50:26:08.3 -- not an asteroid (will add it to exclusion list)
21:40:11.53 +43:33:30.8 -- not an asteroid (will add it to exclusion list)
20:50:08.66 +49:09:12.8 -- not an asteroid (will add it to exclusion list)
20:50:23.96 +49:04:34.7 -- not an asteroid (will add it to exclusion list)
21:39:16.47 +44:34:15.5 -- not an asteroid (will add it to exclusion list)
21:41:04.59 +43:42:38.9 -- not an asteroid (will add it to exclusion list)
21:43:26.88 +44:08:01.8 -- not an asteroid (will add it to exclusion list)
21:42:57.32 +43:54:22.5 -- not an asteroid (will add it to exclusion list)
21:15:02.83 +50:17:58.7 -- not an asteroid (will add it to exclusion list)
20:50:05.56 +49:13:57.8 -- not an asteroid (will add it to exclusion list)
21:39:48.96 +44:02:03.4 -- not an asteroid (will add it to exclusion list)
21:27:55.72 +48:53:28.8 -- not an asteroid (will add it to exclusion list)
21:41:44.21 +43:49:09.6 -- not an asteroid (will add it to exclusion list)
21:23:05.05 +48:55:25.7 -- not an asteroid (will add it to exclusion list)
21:42:38.88 +43:59:12.5 -- not an asteroid (will add it to exclusion list)
21:41:46.94 +44:03:58.9 -- not an asteroid (will add it to exclusion list)
21:45:40.60 +45:38:54.6 -- not an asteroid (will add it to exclusion list)
21:41:21.18 +43:31:18.1 -- not an asteroid (will add it to exclusion list)
21:28:06.13 +48:20:54.6 -- not an asteroid (will add it to exclusion list)
21:42:48.44 +44:08:08.0 -- not an asteroid (will add it to exclusion list)
21:42:02.02 +43:38:59.8 -- not an asteroid (will add it to exclusion list)
21:28:31.62 +48:19:14.0 -- not an asteroid (will add it to exclusion list)
20:52:07.65 +48:52:24.5 -- not an asteroid (will add it to exclusion list)
20:52:01.94 +50:26:37.7 -- not an asteroid (will add it to exclusion list)
21:28:36.73 +48:15:41.1 -- not an asteroid (will add it to exclusion list)
21:40:45.67 +43:31:46.6 -- not an asteroid (will add it to exclusion list)
21:39:52.23 +43:50:53.7 -- not an asteroid (will add it to exclusion list)
21:38:55.14 +44:28:22.9 -- not an asteroid (will add it to exclusion list)
21:41:08.31 +44:17:24.1 -- not an asteroid (will add it to exclusion list)
21:40:26.91 +43:54:44.3 -- not an asteroid (will add it to exclusion list)
21:38:35.60 +44:25:10.0 -- not an asteroid (will add it to exclusion list)
20:49:30.79 +50:27:22.5 -- not an asteroid (will add it to exclusion list)
21:40:16.53 +43:41:28.6 -- not an asteroid (will add it to exclusion list)
21:41:40.87 +43:34:42.4 -- not an asteroid (will add it to exclusion list)
21:40:59.63 +44:00:04.8 -- not an asteroid (will add it to exclusion list)
21:39:07.45 +43:49:17.0 -- not an asteroid (will add it to exclusion list)
21:42:37.29 +43:32:25.6 -- not an asteroid (will add it to exclusion list)
20:50:40.80 +48:59:01.0 -- not an asteroid (will add it to exclusion list)
21:42:21.99 +43:41:44.1 -- not an asteroid (will add it to exclusion list)
21:41:25.95 +43:55:28.2 -- not an asteroid (will add it to exclusion list)
21:41:41.43 +43:48:23.6 -- not an asteroid (will add it to exclusion list)
21:40:38.90 +44:05:14.7 -- not an asteroid (will add it to exclusion list)
21:42:25.60 +43:51:20.1 -- not an asteroid (will add it to exclusion list)
21:41:48.82 +44:10:05.6 -- not an asteroid (will add it to exclusion list)
21:39:56.69 +44:39:34.3 -- not an asteroid (will add it to exclusion list)
21:40:43.45 +43:39:25.9 -- not an asteroid (will add it to exclusion list)
21:41:25.84 +44:13:55.0 -- not an asteroid (will add it to exclusion list)
21:12:01.13 +50:30:46.6 -- not an asteroid (will add it to exclusion list)
21:40:12.92 +43:52:03.8 -- not an asteroid (will add it to exclusion list)
21:40:04.32 +44:10:32.7 -- not an asteroid (will add it to exclusion list)
21:42:07.35 +44:09:55.1 -- not an asteroid (will add it to exclusion list)
21:40:23.49 +44:00:23.2 -- not an asteroid (will add it to exclusion list)
21:41:46.25 +44:26:44.8 -- not an asteroid (will add it to exclusion list)
21:40:48.22 +44:11:21.3 -- not an asteroid (will add it to exclusion list)
21:26:55.09 +48:57:44.0 -- not an asteroid (will add it to exclusion list)
21:42:36.82 +43:55:55.5 -- not an asteroid (will add it to exclusion list)
20:52:20.39 +49:05:57.2 -- not an asteroid (will add it to exclusion list)
21:25:54.68 +49:22:23.7 -- not an asteroid (will add it to exclusion list)
21:42:30.77 +43:57:27.3 -- not an asteroid (will add it to exclusion list)
21:37:43.61 +43:44:13.7 -- not an asteroid (will add it to exclusion list)
21:41:19.20 +44:14:36.5 -- not an asteroid (will add it to exclusion list)
21:41:35.44 +44:08:45.4 -- not an asteroid (will add it to exclusion list)
21:44:14.84 +45:35:57.6 -- not an asteroid (will add it to exclusion list)
21:38:41.33 +43:51:44.8 -- not an asteroid (will add it to exclusion list)
21:42:10.34 +44:16:04.1 -- not an asteroid (will add it to exclusion list)
21:40:54.20 +43:55:55.0 -- not an asteroid (will add it to exclusion list)
21:21:43.45 +48:41:45.6 -- not an asteroid (will add it to exclusion list)
21:40:44.51 +44:04:07.0 -- not an asteroid (will add it to exclusion list)
21:39:04.37 +44:07:38.6 -- not an asteroid (will add it to exclusion list)
21:40:54.90 +43:57:59.3 -- not an asteroid (will add it to exclusion list)
21:39:59.14 +44:09:50.6 -- not an asteroid (will add it to exclusion list)
21:42:01.92 +43:42:27.6 -- not an asteroid (will add it to exclusion list)
21:45:09.78 +45:43:57.9 -- not an asteroid (will add it to exclusion list)
21:43:07.46 +44:54:07.6 -- not an asteroid (will add it to exclusion list)
21:42:38.05 +44:19:35.4 -- not an asteroid (will add it to exclusion list)
20:51:01.44 +50:24:15.3 -- not an asteroid (will add it to exclusion list)
21:39:15.45 +44:15:53.0 -- not an asteroid (will add it to exclusion list)
21:45:11.48 +45:25:21.5 -- not an asteroid (will add it to exclusion list)
21:41:27.90 +44:25:30.0 -- not an asteroid (will add it to exclusion list)
21:45:28.02 +44:12:35.8 -- not an asteroid (will add it to exclusion list)
21:42:16.86 +44:05:41.1 -- not an asteroid (will add it to exclusion list)
20:50:35.73 +49:08:24.0 -- not an asteroid (will add it to exclusion list)
21:40:55.30 +43:23:10.2 -- not an asteroid (will add it to exclusion list)
20:50:19.67 +50:31:03.9 -- not an asteroid (will add it to exclusion list)
21:41:11.45 +43:47:54.2 -- not an asteroid (will add it to exclusion list)
21:41:44.75 +44:06:22.5 -- not an asteroid (will add it to exclusion list)
20:50:26.01 +49:01:53.9 -- not an asteroid (will add it to exclusion list)
21:39:44.02 +44:17:42.2 -- not an asteroid (will add it to exclusion list)
21:41:22.43 +44:21:27.6 -- not an asteroid (will add it to exclusion list)
21:42:39.01 +44:06:48.7 -- not an asteroid (will add it to exclusion list)
21:41:19.21 +44:04:16.1 -- not an asteroid (will add it to exclusion list)
21:39:07.89 +43:21:35.7 -- not an asteroid (will add it to exclusion list)
21:41:36.67 +44:02:03.5 -- not an asteroid (will add it to exclusion list)
21:42:09.79 +44:45:56.8 -- not an asteroid (will add it to exclusion list)
21:43:14.68 +43:36:25.5 -- not an asteroid (will add it to exclusion list)
21:40:42.41 +43:57:37.8 -- not an asteroid (will add it to exclusion list)
21:44:43.54 +45:30:10.4 -- not an asteroid (will add it to exclusion list)
21:40:51.19 +44:36:41.5 -- not an asteroid (will add it to exclusion list)
20:50:49.44 +49:04:34.0 -- not an asteroid (will add it to exclusion list)
21:42:05.20 +43:28:02.8 -- not an asteroid (will add it to exclusion list)
21:41:09.73 +43:47:22.3 -- not an asteroid (will add it to exclusion list)
21:41:32.66 +44:31:33.9 -- not an asteroid (will add it to exclusion list)
21:42:52.08 +43:55:03.2 -- not an asteroid (will add it to exclusion list)
21:40:06.08 +44:22:23.2 -- not an asteroid (will add it to exclusion list)
21:40:36.79 +44:07:30.9 -- not an asteroid (will add it to exclusion list)
21:42:29.68 +44:06:23.5 -- not an asteroid (will add it to exclusion list)
21:42:02.75 +43:29:48.7 -- not an asteroid (will add it to exclusion list)
20:50:57.80 +49:10:08.2 -- not an asteroid (will add it to exclusion list)
20:50:19.79 +49:19:18.5 -- not an asteroid (will add it to exclusion list)
21:40:24.93 +43:44:24.5 -- not an asteroid (will add it to exclusion list)
21:41:49.52 +44:14:22.6 -- not an asteroid (will add it to exclusion list)
20:50:36.51 +49:07:48.8 -- not an asteroid (will add it to exclusion list)
21:41:12.10 +44:19:42.7 -- not an asteroid (will add it to exclusion list)
21:40:29.65 +44:08:05.1 -- not an asteroid (will add it to exclusion list)
21:41:58.48 +44:11:35.6 -- not an asteroid (will add it to exclusion list)
21:41:16.73 +44:07:02.1 -- not an asteroid (will add it to exclusion list)
20:50:08.10 +49:21:40.0 -- not an asteroid (will add it to exclusion list)
21:40:37.16 +43:48:47.5 -- not an asteroid (will add it to exclusion list)
21:40:26.78 +44:33:27.1 -- not an asteroid (will add it to exclusion list)
21:41:08.78 +44:01:21.4 -- not an asteroid (will add it to exclusion list)
21:41:02.78 +44:23:06.9 -- not an asteroid (will add it to exclusion list)
21:41:20.31 +43:52:27.2 -- not an asteroid (will add it to exclusion list)
21:41:49.27 +43:52:18.3 -- not an asteroid (will add it to exclusion list)
21:42:05.79 +43:56:24.1 -- not an asteroid (will add it to exclusion list)
21:41:57.27 +43:40:45.4 -- not an asteroid (will add it to exclusion list)
21:42:01.66 +44:11:54.1 -- not an asteroid (will add it to exclusion list)
21:39:19.20 +44:00:46.3 -- not an asteroid (will add it to exclusion list)
20:49:55.60 +50:26:15.0 -- not an asteroid (will add it to exclusion list)
21:41:02.22 +43:56:55.5 -- not an asteroid (will add it to exclusion list)
21:40:54.19 +44:30:41.3 -- not an asteroid (will add it to exclusion list)
21:39:13.07 +48:41:33.9 -- not an asteroid (will add it to exclusion list)
21:30:36.63 +49:51:16.9 -- not an asteroid (will add it to exclusion list)
20:50:56.12 +49:04:13.6 -- not an asteroid (will add it to exclusion list)
21:40:09.03 +44:10:03.6 -- not an asteroid (will add it to exclusion list)
21:41:49.42 +44:15:10.4 -- not an asteroid (will add it to exclusion list)
20:50:58.13 +50:24:12.4 -- not an asteroid (will add it to exclusion list)
20:51:27.17 +49:04:07.0 -- not an asteroid (will add it to exclusion list)
20:50:47.20 +48:51:48.7 -- not an asteroid (will add it to exclusion list)
21:41:21.14 +43:46:10.9 -- not an asteroid (will add it to exclusion list)
21:40:42.04 +43:38:53.2 -- not an asteroid (will add it to exclusion list)
20:51:28.89 +49:03:48.5 -- not an asteroid (will add it to exclusion list)
21:41:36.89 +43:39:11.3 -- not an asteroid (will add it to exclusion list)
21:42:53.85 +43:55:35.8 -- not an asteroid (will add it to exclusion list)
20:50:55.70 +48:52:58.0 -- not an asteroid (will add it to exclusion list)
20:50:38.65 +49:03:16.4 -- not an asteroid (will add it to exclusion list)
21:24:01.99 +50:11:05.8 -- not an asteroid (will add it to exclusion list)
20:51:56.16 +48:53:47.5 -- not an asteroid (will add it to exclusion list)
20:51:48.04 +50:32:15.1 -- not an asteroid (will add it to exclusion list)
21:43:48.59 +45:37:49.7 -- not an asteroid (will add it to exclusion list)
21:42:43.07 +43:35:11.2 -- listed in neverexclude_list.txt (will NOT add it to exclusion list)
21:42:39.84 +44:00:47.6 -- not an asteroid (will add it to exclusion list)
21:41:20.62 +44:12:11.3 -- not an asteroid (will add it to exclusion list)
21:37:27.43 +43:34:41.6 -- not an asteroid (will add it to exclusion list)
20:50:45.92 +50:29:43.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:49:30.79 +50:27:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:37.51 +50:24:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:45.71 +50:21:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:46.41 +50:22:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:50.79 +50:26:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:55.60 +50:26:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:05.56 +49:13:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:08.10 +49:21:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:08.66 +49:09:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:14.79 +50:28:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:19.46 +50:24:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:19.67 +50:31:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:19.79 +49:19:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:21.21 +50:26:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:23.96 +49:04:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:26.01 +49:01:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:26.16 +49:13:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:35.73 +49:08:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:36.51 +49:07:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:38.65 +49:03:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:39.04 +49:01:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:40.80 +48:59:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:45.92 +50:29:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:47.20 +48:51:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:49.44 +49:04:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:55.70 +48:52:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:56.12 +49:04:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:57.80 +49:10:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:58.13 +50:24:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:00.98 +50:27:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:01.44 +50:24:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:04.60 +50:25:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:05.79 +50:26:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:11.94 +49:04:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:12.21 +50:12:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:13.15 +49:07:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:27.17 +49:04:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:28.89 +49:03:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:43.72 +50:27:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:48.04 +50:32:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:56.16 +48:53:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:01.94 +50:26:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:07.65 +48:52:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:20.39 +49:05:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:42.25 +50:27:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:01.13 +50:30:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:15:02.83 +50:17:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:21:43.45 +48:41:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:23:05.05 +48:55:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:24:01.99 +50:11:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:54.68 +49:22:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:26:55.09 +48:57:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:27:55.72 +48:53:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:06.13 +48:20:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:31.62 +48:19:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:28:36.73 +48:15:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:30:36.63 +49:51:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:27.43 +43:34:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:41.38 +44:16:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:43.61 +43:44:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:35.60 +44:25:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:41.33 +43:51:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:38:55.14 +44:28:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:04.37 +44:07:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:07.45 +43:49:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:07.89 +43:21:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:13.07 +48:41:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:15.45 +44:15:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:16.47 +44:34:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:19.20 +44:00:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:44.02 +44:17:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:48.96 +44:02:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:52.23 +43:50:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:56.69 +44:39:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:57.12 +44:20:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:59.14 +44:09:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:04.32 +44:10:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:06.08 +44:22:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:09.03 +44:10:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:10.81 +44:19:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:11.53 +43:33:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:12.92 +43:52:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:16.53 +43:41:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:23.49 +44:00:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:24.93 +43:44:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:26.78 +44:33:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:26.91 +43:54:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:29.65 +44:08:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:36.79 +44:07:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:37.16 +43:48:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:38.14 +43:44:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:38.90 +44:05:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:42.04 +43:38:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:42.41 +43:57:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.31 +43:49:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:43.45 +43:39:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:44.51 +44:04:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:45.67 +43:31:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:48.22 +44:11:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:51.19 +44:36:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:54.19 +44:30:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:54.20 +43:55:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:54.90 +43:57:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:55.30 +43:23:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:40:59.63 +44:00:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:02.22 +43:56:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:02.78 +44:23:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:04.59 +43:42:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:08.31 +44:17:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:08.78 +44:01:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:09.73 +43:47:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:11.45 +43:47:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:11.98 +44:11:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:12.10 +44:19:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:16.73 +44:07:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:18.70 +43:48:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:19.20 +44:14:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:19.21 +44:04:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:20.31 +43:52:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:20.62 +44:12:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:21.14 +43:46:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:21.18 +43:31:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:22.43 +44:21:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:25.84 +44:13:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:25.95 +43:55:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:27.90 +44:25:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:32.66 +44:31:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:35.44 +44:08:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:36.67 +44:02:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:36.89 +43:39:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:40.87 +43:34:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:41.43 +43:48:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:43.92 +43:52:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:44.21 +43:49:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:44.75 +44:06:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:45.97 +43:47:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:46.25 +44:26:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:46.94 +44:03:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:48.82 +44:10:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:49.27 +43:52:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:49.42 +44:15:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:49.52 +44:14:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:57.27 +43:40:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:58.48 +44:11:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:01.66 +44:11:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:01.92 +43:42:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:02.02 +43:38:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:02.75 +43:29:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:05.20 +43:28:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:05.79 +43:56:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:07.35 +44:09:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:09.79 +44:45:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:10.34 +44:16:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:16.86 +44:05:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:21.99 +43:41:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:25.60 +43:51:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:29.68 +44:06:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:30.77 +43:57:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:36.82 +43:55:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:37.29 +43:32:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:38.05 +44:19:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:38.88 +43:59:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:39.01 +44:06:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:39.84 +44:00:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:48.44 +44:08:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:52.08 +43:55:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:53.85 +43:55:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:42:57.32 +43:54:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:07.46 +44:54:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:14.68 +43:36:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:26.88 +44:08:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:43:48.59 +45:37:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:14.84 +45:35:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:44:43.54 +45:30:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:09.78 +45:43:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:11.48 +45:25:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:28.02 +44:12:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:40.60 +45:38:54.6 -- 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)
20:49:30.79 +50:27:22.5 -- not a known variable star
20:49:37.51 +50:24:52.9 -- not a known variable star
20:49:45.71 +50:21:50.8 -- not a known variable star
20:49:46.41 +50:22:36.4 -- not a known variable star
20:49:50.79 +50:26:08.0 -- not a known variable star
20:49:55.60 +50:26:15.0 -- not a known variable star
20:50:05.56 +49:13:57.8 -- not a known variable star
20:50:08.10 +49:21:40.0 -- not a known variable star
20:50:08.66 +49:09:12.8 -- not a known variable star
20:50:14.79 +50:28:25.5 -- not a known variable star
20:50:19.46 +50:24:28.8 -- not a known variable star
20:50:19.67 +50:31:03.9 -- not a known variable star
20:50:19.79 +49:19:18.5 -- not a known variable star
20:50:21.21 +50:26:08.3 -- a known variable star
20:50:23.96 +49:04:34.7 -- not a known variable star
20:50:26.01 +49:01:53.9 -- not a known variable star
20:50:26.16 +49:13:24.7 -- not a known variable star
20:50:35.73 +49:08:24.0 -- not a known variable star
20:50:36.51 +49:07:48.8 -- not a known variable star
20:50:38.65 +49:03:16.4 -- not a known variable star
20:50:39.04 +49:01:04.8 -- not a known variable star
20:50:40.80 +48:59:01.0 -- not a known variable star
20:50:45.92 +50:29:43.7 -- a known variable star
20:50:47.20 +48:51:48.7 -- not a known variable star
20:50:49.44 +49:04:34.0 -- not a known variable star
20:50:55.70 +48:52:58.0 -- a known variable star
20:50:56.12 +49:04:13.6 -- not a known variable star
20:50:57.80 +49:10:08.2 -- not a known variable star
20:50:58.13 +50:24:12.4 -- a known variable star
20:51:00.98 +50:27:14.4 -- not a known variable star
20:51:01.44 +50:24:15.3 -- not a known variable star
20:51:04.60 +50:25:11.0 -- not a known variable star
20:51:05.79 +50:26:41.7 -- a known variable star
20:51:11.94 +49:04:19.5 -- not a known variable star
20:51:12.21 +50:12:01.2 -- not a known variable star
20:51:13.15 +49:07:13.9 -- not a known variable star
20:51:27.17 +49:04:07.0 -- not a known variable star
20:51:28.89 +49:03:48.5 -- not a known variable star
20:51:43.72 +50:27:45.2 -- not a known variable star
20:51:48.04 +50:32:15.1 -- not a known variable star
20:51:56.16 +48:53:47.5 -- a known variable star
20:52:01.94 +50:26:37.7 -- not a known variable star
20:52:07.65 +48:52:24.5 -- not a known variable star
20:52:20.39 +49:05:57.2 -- not a known variable star
20:52:42.25 +50:27:26.3 -- not a known variable star
21:12:01.13 +50:30:46.6 -- a known variable star
21:15:02.83 +50:17:58.7 -- a known variable star
21:21:43.45 +48:41:45.6 -- a known variable star
21:23:05.05 +48:55:25.7 -- a known variable star
21:24:01.99 +50:11:05.8 -- not a known variable star
21:25:54.68 +49:22:23.7 -- not a known variable star
21:26:55.09 +48:57:44.0 -- not a known variable star
21:27:55.72 +48:53:28.8 -- a known variable star
21:28:06.13 +48:20:54.6 -- not a known variable star
21:28:31.62 +48:19:14.0 -- a known variable star
21:28:36.73 +48:15:41.1 -- not a known variable star
21:30:36.63 +49:51:16.9 -- a known variable star
21:37:27.43 +43:34:41.6 -- not a known variable star
21:37:41.38 +44:16:34.7 -- a known variable star
21:37:43.61 +43:44:13.7 -- not a known variable star
21:38:35.60 +44:25:10.0 -- not a known variable star
21:38:41.33 +43:51:44.8 -- a known variable star
21:38:55.14 +44:28:22.9 -- not a known variable star
21:39:04.37 +44:07:38.6 -- not a known variable star
21:39:07.45 +43:49:17.0 -- not a known variable star
21:39:07.89 +43:21:35.7 -- not a known variable star
21:39:13.07 +48:41:33.9 -- a known variable star
21:39:15.45 +44:15:53.0 -- not a known variable star
21:39:16.47 +44:34:15.5 -- not a known variable star
21:39:19.20 +44:00:46.3 -- a known variable star
21:39:44.02 +44:17:42.2 -- not a known variable star
21:39:48.96 +44:02:03.4 -- not a known variable star
21:39:52.23 +43:50:53.7 -- not a known variable star
21:39:56.69 +44:39:34.3 -- not a known variable star
21:39:57.12 +44:20:58.4 -- a known variable star
21:39:59.14 +44:09:50.6 -- not a known variable star
21:40:04.32 +44:10:32.7 -- not a known variable star
21:40:06.08 +44:22:23.2 -- not a known variable star
21:40:09.03 +44:10:03.6 -- a known variable star
21:40:10.81 +44:19:47.1 -- not a known variable star
21:40:11.53 +43:33:30.8 -- not a known variable star
21:40:12.92 +43:52:03.8 -- not a known variable star
21:40:16.53 +43:41:28.6 -- not a known variable star
21:40:23.49 +44:00:23.2 -- not a known variable star
21:40:24.93 +43:44:24.5 -- not a known variable star
21:40:26.78 +44:33:27.1 -- not a known variable star
21:40:26.91 +43:54:44.3 -- a known variable star
21:40:29.65 +44:08:05.1 -- not a known variable star
21:40:36.79 +44:07:30.9 -- not a known variable star
21:40:37.16 +43:48:47.5 -- not a known variable star
21:40:38.14 +43:44:28.7 -- not a known variable star
21:40:38.90 +44:05:14.7 -- not a known variable star
21:40:42.04 +43:38:53.2 -- not a known variable star
21:40:42.41 +43:57:37.8 -- not a known variable star
21:40:43.31 +43:49:30.5 -- not a known variable star
21:40:43.45 +43:39:25.9 -- not a known variable star
21:40:44.51 +44:04:07.0 -- a known variable star
21:40:45.67 +43:31:46.6 -- not a known variable star
21:40:48.22 +44:11:21.3 -- not a known variable star
21:40:51.19 +44:36:41.5 -- a known variable star
21:40:54.19 +44:30:41.3 -- not a known variable star
21:40:54.20 +43:55:55.0 -- not a known variable star
21:40:54.90 +43:57:59.3 -- not a known variable star
21:40:55.30 +43:23:10.2 -- not a known variable star
21:40:59.63 +44:00:04.8 -- not a known variable star
21:41:02.22 +43:56:55.5 -- a known variable star
21:41:02.78 +44:23:06.9 -- not a known variable star
21:41:04.59 +43:42:38.9 -- not a known variable star
21:41:08.31 +44:17:24.1 -- not a known variable star
21:41:08.78 +44:01:21.4 -- not a known variable star
21:41:09.73 +43:47:22.3 -- not a known variable star
21:41:11.45 +43:47:54.2 -- not a known variable star
21:41:11.98 +44:11:42.8 -- not a known variable star
21:41:12.10 +44:19:42.7 -- not a known variable star
21:41:16.73 +44:07:02.1 -- not a known variable star
21:41:18.70 +43:48:56.3 -- not a known variable star
21:41:19.20 +44:14:36.5 -- not a known variable star
21:41:19.21 +44:04:16.1 -- not a known variable star
21:41:20.31 +43:52:27.2 -- not a known variable star
21:41:20.62 +44:12:11.3 -- a known variable star
21:41:21.14 +43:46:10.9 -- not a known variable star
21:41:21.18 +43:31:18.1 -- not a known variable star
21:41:22.43 +44:21:27.6 -- a known variable star
21:41:25.84 +44:13:55.0 -- not a known variable star
21:41:25.95 +43:55:28.2 -- not a known variable star
21:41:27.90 +44:25:30.0 -- not a known variable star
21:41:32.66 +44:31:33.9 -- not a known variable star
21:41:35.44 +44:08:45.4 -- not a known variable star
21:41:36.67 +44:02:03.5 -- not a known variable star
21:41:36.89 +43:39:11.3 -- a known variable star
21:41:40.87 +43:34:42.4 -- not a known variable star
21:41:41.43 +43:48:23.6 -- not a known variable star
21:41:43.92 +43:52:22.8 -- not a known variable star
21:41:44.21 +43:49:09.6 -- not a known variable star
21:41:44.75 +44:06:22.5 -- not a known variable star
21:41:45.97 +43:47:14.2 -- not a known variable star
21:41:46.25 +44:26:44.8 -- not a known variable star
21:41:46.94 +44:03:58.9 -- not a known variable star
21:41:48.82 +44:10:05.6 -- not a known variable star
21:41:49.27 +43:52:18.3 -- not a known variable star
21:41:49.42 +44:15:10.4 -- not a known variable star
21:41:49.52 +44:14:22.6 -- not a known variable star
21:41:57.27 +43:40:45.4 -- not a known variable star
21:41:58.48 +44:11:35.6 -- not a known variable star
21:42:01.66 +44:11:54.1 -- a known variable star
21:42:01.92 +43:42:27.6 -- not a known variable star
21:42:02.02 +43:38:59.8 -- a known variable star
21:42:02.75 +43:29:48.7 -- not a known variable star
21:42:05.20 +43:28:02.8 -- not a known variable star
21:42:05.79 +43:56:24.1 -- not a known variable star
21:42:07.35 +44:09:55.1 -- not a known variable star
21:42:09.79 +44:45:56.8 -- not a known variable star
21:42:10.34 +44:16:04.1 -- not a known variable star
21:42:16.86 +44:05:41.1 -- not a known variable star
21:42:21.99 +43:41:44.1 -- a known variable star
21:42:25.60 +43:51:20.1 -- not a known variable star
21:42:29.68 +44:06:23.5 -- a known variable star
21:42:30.77 +43:57:27.3 -- not a known variable star
21:42:36.82 +43:55:55.5 -- not a known variable star
21:42:37.29 +43:32:25.6 -- not a known variable star
21:42:38.05 +44:19:35.4 -- not a known variable star
21:42:38.88 +43:59:12.5 -- not a known variable star
21:42:39.01 +44:06:48.7 -- a known variable star
21:42:39.84 +44:00:47.6 -- a known variable star
21:42:48.44 +44:08:08.0 -- not a known variable star
21:42:52.08 +43:55:03.2 -- not a known variable star
21:42:53.85 +43:55:35.8 -- a known variable star
21:42:57.32 +43:54:22.5 -- not a known variable star
21:43:07.46 +44:54:07.6 -- a known variable star
21:43:14.68 +43:36:25.5 -- a known variable star
21:43:26.88 +44:08:01.8 -- not a known variable star
21:43:48.59 +45:37:49.7 -- a known variable star
21:44:14.84 +45:35:57.6 -- not a known variable star
21:44:43.54 +45:30:10.4 -- not a known variable star
21:45:09.78 +45:43:57.9 -- a known variable star
21:45:11.48 +45:25:21.5 -- not a known variable star
21:45:28.02 +44:12:35.8 -- a known variable star
21:45:40.60 +45:38:54.6 -- not a known variable star
Found 140 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
178 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 178 (excluding asteroids and hot pixels, 140 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461317.65802685 -observatory V36
14:05:30.81 -14:58:01.2 Mercury (-0.0mag)
14:12:48.70 -21:06:43.3 Venus (-4.7mag)
08:22:48.48 +20:29:31.0 Mars (1.1mag)
09:29:31.98 +15:27:28.8 Jupiter (-1.9mag)
00:44:31.96 +01:50:11.5 Saturn (0.3mag)
04:12:44.83 +20:59:38.8 Uranus (5.6mag)
00:11:03.83 -00:20:58.7 Neptune (7.7mag)
20:24:18.45 -23:43:21.7 Pluto (14.5mag)
07:23:57.70 +24:42:52.2 Moon (-10.2mag)
-rw-r--r-- 1 apache apache 363 Oct 4 00:35 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461317.65802685:
09:29:28.77 +15:27:46.8 Io (9.6mag)
09:29:40.53 +15:26:42.8 Europa (6.2mag)
09:29:46.21 +15:26:12.8 Ganymede (8.0mag)
09:29:49.45 +15:25:56.6 Callisto (6.9mag)
09:28:45.11 +15:49:16.4 Himalia (15.7mag)
09:29:33.89 +15:27:19.8 Thebe (16.5mag)
09:27:47.95 +15:47:17.0 Elara (17.5mag)
09:32:23.44 +14:50:15.4 Pasiphae (17.8mag)
09:28:39.48 +15:52:40.7 Carme (18.9mag)
00:44:44.08 +01:49:52.0 Titan (8.2mag)
00:44:24.96 +01:50:08.4 Rhea (9.6mag)
00:43:52.88 +01:47:55.1 Iapetus (11.0mag)
00:44:39.10 +01:50:23.4 Hyperion (14.1mag)
00:42:55.60 +01:38:05.8 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Oct 4 00:35 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461317.65802685:
01:58:03.66 +20:36:56.7 JWST
18:19:37.05 +23:12:58.1 Chandra
04:40:25.34 +50:33:05.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Oct 4 00:35 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461317.65802685 -observatory V36
03:47:30.42 +20:08:24.0 17.2mag P/1996 R2 (Lagerkvist)
18:18:37.14 -33:39:51.2 14.7mag P/2010 H2 (Vales)
07:36:33.25 -71:55:47.1 17.2mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:29.17 +34:26:26.8 17.7mag C/2017 K2 (PANSTARRS)
05:04:17.23 +48:11:27.7 16.8mag P/2021 N1 (ZTF)
07:27:02.11 +25:32:27.3 16.9mag C/2022 N2 (PANSTARRS)
15:27:33.75 -17:58:37.6 15.2mag C/2023 R1 (PANSTARRS)
08:58:08.21 +34:56:48.9 16.1mag C/2024 E1 (Wierzchos)
18:25:50.49 +41:52:06.2 17.4mag C/2024 J3 (ATLAS)
05:45:21.78 -13:29:02.3 16.7mag C/2024 T5 (ATLAS)
07:15:42.12 +12:45:38.6 17.7mag C/2025 J1 (Borisov)
12:03:48.85 +16:35:30.7 16.3mag C/2025 V2 (Rankin)
13:43:49.05 -02:06:49.8 16.6mag C/2025 Y1 (ATLAS)
18:13:12.69 +67:49:38.0 16.0mag C/2026 A2 (Bok)
02:44:04.01 +44:13:40.7 17.7mag C/2026 B2 (Sun-Gao)
12:38:42.36 +13:33:50.3 17.7mag A/2026 E1
00:43:55.71 +19:50:43.0 17.8mag 2P/Encke
22:50:34.34 -33:08:57.9 14.2mag 10P/Tempel
02:00:31.48 +39:31:47.7 16.9mag 11P/Tempel-Swift-LINEAR
12:06:21.64 -07:34:30.3 16.3mag 29P/Schwassmann-Wachmann
13:02:39.05 -13:17:14.7 18.0mag 63P/Wild
00:27:12.60 -08:36:24.7 15.5mag 65P/Gunn
07:25:36.21 +16:46:30.8 13.8mag 78P/Gehrels
03:06:39.90 +14:39:02.5 17.5mag 88P/Howell
07:12:31.63 +38:05:08.8 17.1mag 112P/Urata-Niijima
08:45:13.03 +16:40:44.3 17.8mag 114P/Wiseman-Skiff
11:26:01.08 +14:54:51.1 14.8mag 123P/West-Hartley
13:48:47.91 -30:06:02.3 17.7mag 124P/Mrkos
06:45:15.47 +19:37:15.9 15.7mag 128P/Shoemaker-Holt
23:37:02.52 +00:36:39.4 17.2mag 139P/Vaisala-Oterma
22:51:04.59 -03:19:47.9 9.5mag 161P/Hartley-IRAS
10:02:59.85 +35:52:19.2 16.8mag 162P/Siding Spring
10:00:48.02 +03:26:55.5 13.7mag 169P/NEAT
03:32:15.61 +05:31:17.9 14.7mag 220P/McNaught
05:51:09.41 +43:34:48.9 15.4mag 260P/McNaught
15:45:36.76 -03:09:13.3 18.0mag 391P/Kowalski
09:48:42.88 +32:05:29.6 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 1.8K Oct 4 00:35 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
08:07:27.96 -65:51:03.90 ASASSN-26fi 2026-10-1.36 15.82
21:02:34.66 +23:57:26.20 ASASSN-26fh 2026-10-1.27 15.94
20:00:16.62 +03:26:29.90 AT2026adfv 2026-10-1.3 16.42
00:08:42.74 -32:33:16.50 SN2026abhc 2026-09-29.15 15.57
21:02:30.26 -19:27:41.80 SN2026acxa 2026-09-29.13 14.65
04:39:17.45 -28:06:12.40 ASASSN-26fg 2026-09-23.25 15.73
05:25:07.80 +04:38:32.40 SN2026aajs 2026-09-21.32 17.04
19:56:12.67 +08:25:27.70 AT2026acgs 2026-09-18.14 15.84
00:02:34.07 +52:55:19.10 ASASSN-26ff 2026-09-16.43 15.37
23:44:33.18 +17:46:12.20 SN2026yjv 2026-09-15.38 18.32
16:21:12.24 +57:37:51.30 SN 2026aafh 2026-09-14.11 15.02
23:36:00.27 -19:28:18.00 SN 2026aaks 2026-09-14.44 16.89
16:35:24.86 -05:32:38.20 SN2026aasi 2026-09-12.99 16.58
16:46:08.71 +37:25:21.80 SN2026aafk 2026-09-13.25 17.4
23:48:37.86 +50:25:24.60 SN2026aafs 2026-09-13.47 17
21:20:27.02 +02:10:42.50 SN2026aagh -------
08:02:26.85 -24:37:44.10 ASASSN-26fe 2026-09-13.34 13.67
02:29:34.91 +23:06:56.30 SN2026aars 2026-09-12.27 16.93
02:47:25.52 -32:58:34.50 SN 2026znh 2026-09-9.92 16.26
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.64 +34:24:35.00 SN2026aaiv 2026-09-7.25 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.79 -22:25:29.10 V8055 2026-08-30 10.76
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
-rw-r--r-- 1 apache apache 5.7K Oct 4 00:35 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
00:42:40.94 +41:15:37.1 PNV J00424094+4115371 2026-09-17.8925 18.3mag
08:49:20.13 -09:19:15.8 TCP J08492013-0919158 2026-09-18.4698 13.3mag
00:42:13.93 +41:16:35.6 PNV J00421393+4116356 2026-09-22.6597 19.66Cmag
18:14:01.58 +15:13:55.5 TCP J18140158+1513555 2026-09-24.4645 14.1mag
00:42:36.61 +41:13:50.5 TCP J00423661+4113505 2026-09-29.7462 17.4mag
22:03:46.29 -11:07:57.8 TCP J22034629-1107578 2026-09-29.7438 14.51Cmag
22:05:02.06 +20:49:01.2 TCP J22050206+2049012 2026-10-03.5715 17.13Cmag
-rw-r--r-- 1 apache apache 191K Oct 4 00:35 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
23:07:40.547 +16:49:47.27 AT 2026acai 2026-09-13.94 19.57
00:48:05.016 -23:46:35.80 AT 2026acah 2026-09-16.57 20.17
21:11:13.518 -41:27:55.00 AT 2026acag 2026-09-11.48 20.26
03:14:10.165 +01:00:34.77 AT 2026acaf 2026-09-18.13 19.836
03:10:38.472 -02:59:14.60 AT 2026acae 2026-09-18.14 20.248
23:19:10.207 -42:10:18.70 AT 2026acad 2026-09-17.49 20.14
22:45:42.369 -32:03:13.11 AT 2026acac 2026-09-17.57 20.42
21:06:10.283 -26:29:48.88 AT 2026acab 2026-09-17.42 20.14
02:59:42.870 -32:10:51.62 AT 2026acaa 2026-09-17.71 19.79
03:12:48.598 -25:41:36.30 AT 2026abzz 2026-08-07.77 20.11
03:27:04.244 -02:48:44.64 AT 2026abzy 2026-09-16.21 19.9
01:33:35.787 -29:12:14.34 AT 2026abzx 2026-09-14.75 20.32
05:25:39.066 -07:33:55.88 AT 2026abzw 2026-09-12.24 19.63
01:48:46.374 +07:27:55.45 AT 2026abzv 2026-09-11.68 19.9
04:01:35.497 -03:50:58.41 AT 2026abzu 2026-09-17.17 20.26
02:10:03.461 +06:00:29.47 AT 2026abzt 2026-09-18.06 20.09
23:56:05.061 +07:13:14.64 AT 2026abzs 2026-09-18.02 19.953
03:09:38.698 -79:15:01.74 AT 2026abzr 2026-09-17.29 19.444
03:13:00.122 -45:33:01.75 AT 2026abzq 2026-09-15.27 19.756
06:56:27.724 -50:51:56.56 AT 2026abzp 2026-09-14.38 19.123
-rw-r--r-- 1 apache apache 89K Oct 4 00:35 tns_transients_list.txt
