This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi
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 09 17.3725 2461300.8725 12.63 20:32:36.71 +45:08:02.4
83.23065 3.14904 galactic Cyg Second-epoch detections are separated by 1.9" and 5.4 pix
The object was found in VSX 2" ASASSN-V J203236.63+450803.8
Type: VAR
# Max. Min./Amp. JD0 Period
14.320 V 14.620 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:32:36.71 +45:08:02.4: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:32:36.71 +45:08:02.4: 13.58 +/- 0.05 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
ASASSN-V J203236.63+450803.8,2461300.8725,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203236.63+450803.8 20260917.3725 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.63 20:51:27.24 +41:34:31.8
82.53115 -1.73855 galactic Cyg Second-epoch detections are separated by 1.4" and 5.9 pix
The object was found in VSX 0" Gaia DR3 2065773273881998464
Type: ROT
# Max. Min./Amp. JD0 Period
13.410 G 13.440 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:27.24 +41:34:31.8: 13.67 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:27.24 +41:34:31.8: 13.81 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065773273881998464,2461300.8725,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065773273881998464 20260917.3725 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:48:47.05 +41:32:05.7
82.18312 -1.37788 galactic Cyg Second-epoch detections are separated by 1.4" 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 | ATO J312.1916+41.5249 | 20:48:47.05 +41:32:05.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.911+/-0.027 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:47.05 +41:32:05.7: 13.65 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:47.05 +41:32:05.7: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.1916+41.5249,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.1916+41.5249 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:48:54.68 +41:52:08.3
82.45737 -1.18557 galactic Cyg Second-epoch detections are separated by 0.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:54.68 +41:52:08.3 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.025 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:54.68 +41:52:08.3: 13.69 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:54.68 +41:52:08.3: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.67 20:14:58.75 +45:49:56.3
82.03730 6.08542 galactic Cyg Second-epoch detections are separated by 0.7" 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 J303.7450+45.8326 | 20:14:58.79 +45:49:57.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.574+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:14:58.75 +45:49:56.3: 13.67 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:14:58.75 +45:49:56.3: 13.54 +/- 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
ATO J303.7450+45.8326,2461300.8725,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.7450+45.8326 20260917.3725 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.70 20:48:11.22 +41:08:48.9
81.81105 -1.53523 galactic Cyg Second-epoch detections are separated by 1.2" 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 | 20:48:11.22 +41:08:48.9 (user input) | T | P | (position from user input) J-Ks=0.517+/-0.034 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:11.22 +41:08:48.9: 13.71 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:11.22 +41:08:48.9: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.69 20:50:51.53 +41:43:36.2
82.57714 -1.55657 galactic Cyg Second-epoch detections are separated by 2.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.7106+41.7274 | 20:50:51.53 +41:43:36.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.588+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:51.53 +41:43:36.2: 13.70 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:51.53 +41:43:36.2: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7106+41.7274,2461300.8725,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.7106+41.7274 20260917.3725 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.75 20:50:04.64 +42:18:47.6
82.93839 -1.07220 galactic Cyg Second-epoch detections are separated by 0.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:04.64 +42:18:47.6 (user input) | T | P | (position from user input) J-Ks=1.443+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:04.64 +42:18:47.6: 13.70 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:04.64 +42:18:47.6: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:47:01.36 +41:37:09.6
82.04165 -1.06862 galactic Cyg Second-epoch detections are separated by 1.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:47:01.36 +41:37:09.6 (user input) | T | P | (position from user input) J-Ks=1.048+/-0.026 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:01.36 +41:37:09.6: 13.75 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:01.36 +41:37:09.6: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.71 20:49:46.94 +42:22:03.4
82.94595 -0.99556 galactic Cyg Second-epoch detections are separated by 0.2" 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 | 20:49:46.94 +42:22:03.4 (user input) | T | P | (position from user input) J-Ks=12.084+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:46.94 +42:22:03.4: 13.75 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:46.94 +42:22:03.4: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:13:29.19 +46:38:35.5
82.57913 6.74439 galactic Cyg Second-epoch detections are separated by 0.8" and 5.7 pix
The object was found in VSX 1" ZTF J201329.15+463834.8
Type: EW
# Max. Min./Amp. JD0 Period
13.412 r Y 0.084 r 2458375.74190 0.409818400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:13:29.19 +46:38:35.5: 13.78 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:13:29.19 +46:38:35.5: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201329.15+463834.8,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J201329.15+463834.8 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.82 20:46:43.86 +42:59:43.9
83.08070 -0.16455 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was found in VSX 4" Gaia DR3 2066882195783848320
Type: YSO
# Max. Min./Amp. JD0 Period
17.780 G 17.890 G
NOTE: the measured mag 12.82 is inconsistent with the record above (maximum 17.78), and the brighter VSX variable Gaia DR3 2066882268799979264 at 15" may be the actual counterpart.
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:43.86 +42:59:43.9: 13.81 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:43.86 +42:59:43.9: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066882195783848320,2461300.8725,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066882195783848320 20260917.3725 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.93 20:41:29.42 +42:25:04.6
82.03062 0.23269 galactic Cyg Second-epoch detections are separated by 0.5" 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 | 20:41:29.42 +42:25:04.6 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:29.42 +42:25:04.6: 13.83 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:29.42 +42:25:04.6: 14.18 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.93,0.05,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
target 20260917.3725 12.93CV 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 09 17.3725 2461300.8725 12.95 20:44:32.41 +44:01:35.5
83.63905 0.78886 galactic Cyg Second-epoch detections are separated by 1.3" 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 J311.1369+44.0248 | 20:44:32.41 +44:01:35.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.697+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:32.41 +44:01:35.5: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:32.41 +44:01:35.5: 13.90 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.1369+44.0248,2461300.8725,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1369+44.0248 20260917.3725 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:38:29.43 +45:07:16.0
83.84229 2.31116 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 | ATO J309.6198+45.1262 | 20:38:29.43 +45:07:16.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.436+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:38:29.43 +45:07:16.0: 13.88 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:38:29.43 +45:07:16.0: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J309.6198+45.1262,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.6198+45.1262 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.80 20:48:18.79 +41:48:05.0
82.33464 -1.14167 galactic Cyg Second-epoch detections are separated by 0.6" and 5.8 pix
The object was found in VSX 1" Gaia DR3 2066214487282823424
Type: ROT
# Max. Min./Amp. JD0 Period
13.650 G 13.670 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:18.79 +41:48:05.0: 13.87 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:18.79 +41:48:05.0: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 2066214487282823424,2461300.8725,12.80,0.05,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
Gaia DR3 2066214487282823424 20260917.3725 12.80CV 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 09 17.3725 2461300.8725 12.88 20:40:38.00 +43:31:06.6
82.80420 1.03110 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 | target | 20:40:38.00 +43:31:06.6 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.479+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:38.00 +43:31:06.6: 13.87 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:38.00 +43:31:06.6: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.98 20:39:25.17 +42:56:24.0
82.21094 0.85308 galactic Cyg Second-epoch detections are separated by 1.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:39:25.17 +42:56:24.0 (user input) | T | P | (position from user input) J-Ks=0.728+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:25.17 +42:56:24.0: 13.93 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:25.17 +42:56:24.0: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:49:14.17 +41:58:17.0
82.57496 -1.16776 galactic Cyg Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:14.17 +41:58:17.0 (user input) | T | P | (position from user input) J-Ks=1.198+/-0.027 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:14.17 +41:58:17.0: 13.94 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:14.17 +41:58:17.0: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.01 20:58:08.83 +41:47:10.6
83.49834 -2.55833 galactic Cyg Second-epoch detections are separated by 2.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:08.83 +41:47:10.6 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:58:08.83 +41:47:10.6: 13.97 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:58:08.83 +41:47:10.6: 14.16 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.08 20:40:09.79 +42:57:36.9
82.31000 0.75759 galactic Cyg Second-epoch detections are separated by 2.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:09.79 +42:57:36.9 (user input) | T | P | (position from user input) SpType: A0III (LAMOST DR5)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:09.79 +42:57:36.9: 13.97 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:09.79 +42:57:36.9: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461300.8725,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:46:30.43 +42:01:03.3
82.29209 -0.74439 galactic Cyg Second-epoch detections are separated by 1.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:30.43 +42:01:03.3 (user input) | T | P | (position from user input) J-Ks=0.570+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:30.43 +42:01:03.3: 13.97 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:30.43 +42:01:03.3: 14.13 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.12 20:42:51.54 +42:09:19.9
81.97962 -0.12833 galactic Cyg Second-epoch detections are separated by 1.8" 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 | ATO J310.7141+42.1548 | 20:42:51.54 +42:09:19.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:51.54 +42:09:19.9: 14.00 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:51.54 +42:09:19.9: 14.34 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.7141+42.1548,2461300.8725,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J310.7141+42.1548 20260917.3725 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.12 20:39:56.24 +42:13:27.5
81.70177 0.34114 galactic Cyg Second-epoch detections are separated by 1.7" 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 | 20:39:56.24 +42:13:27.5 (user input) | T | P | (position from user input) J-Ks=0.506+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:56.24 +42:13:27.5: 14.00 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:56.24 +42:13:27.5: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8725,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:40:26.66 +44:31:56.9
83.58596 1.67800 galactic Cyg Second-epoch detections are separated by 0.8" and 5.7 pix
The object was found in VSX 1" ZTF J204026.66+443156.2
Type: BY
# Max. Min./Amp. JD0 Period
13.777 r Y 0.050 r 2458322.90470 0.256149200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:26.66 +44:31:56.9: 14.05 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:26.66 +44:31:56.9: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204026.66+443156.2,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204026.66+443156.2 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:52:51.60 +41:08:31.3
82.36576 -2.21832 galactic Cyg Second-epoch detections are separated by 1.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:52:51.60 +41:08:31.3 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:51.60 +41:08:31.3: 14.05 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:51.60 +41:08:31.3: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.11 20:48:06.75 +42:21:03.5
82.73831 -0.76680 galactic Cyg Second-epoch detections are separated by 1.2" 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 | target | 20:48:06.75 +42:21:03.5 (user input) | T | P | (position from user input) J-Ks=0.511+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:06.75 +42:21:03.5: 14.06 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:06.75 +42:21:03.5: 14.30 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.11,0.05,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 20260917.3725 13.11CV 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 09 17.3725 2461300.8725 13.13 20:41:06.41 +42:57:17.8
82.41146 0.61779 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 | target | 20:41:06.41 +42:57:17.8 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:06.41 +42:57:17.8: 14.07 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:06.41 +42:57:17.8: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461300.8725,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.95 20:47:19.26 +41:40:34.9
82.12103 -1.07628 galactic Cyg Second-epoch detections are separated by 1.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:47:19.26 +41:40:34.9 (user input) | T | P | (position from user input) J-Ks=0.390+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:19.26 +41:40:34.9: 14.10 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:19.26 +41:40:34.9: 14.18 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.08 20:42:49.40 +44:11:19.2
83.57567 1.13128 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:49.40 +44:11:19.2 (user input) | T | P | (position from user input) J-Ks=0.523+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:49.40 +44:11:19.2: 14.13 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:49.40 +44:11:19.2: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461300.8725,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.13 20:46:19.49 +42:59:59.7
83.03766 -0.10386 galactic Cyg Second-epoch detections are separated by 0.7" 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 | 20:46:19.49 +42:59:59.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.403+/-0.048 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:19.49 +42:59:59.7: 14.16 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:19.49 +42:59:59.7: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.19 +/- 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,2461300.8725,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:44:05.30 +42:26:28.8
82.34480 -0.13017 galactic Cyg Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:05.30 +42:26:28.8 (user input) | T | P | (position from user input) J-Ks=0.545+/-0.039 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:05.30 +42:26:28.8: 14.21 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:05.30 +42:26:28.8: 14.27 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.23 +/- 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,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:41:42.50 +42:28:19.1
82.09796 0.23413 galactic Cyg Second-epoch detections are separated by 0.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:42.50 +42:28:19.1 (user input) | T | P | (position from user input) SpType: F9.5? 2010ApJ...720..679B [BKH2010] J204144.0+422801 J-Ks=0.515+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:42.50 +42:28:19.1: 14.05 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:42.50 +42:28:19.1: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.19 20:51:57.23 +42:20:13.0
83.17732 -1.32478 galactic Cyg Second-epoch detections are separated by 0.5" 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 | 20:51:57.23 +42:20:13.0 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.035 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:57.23 +42:20:13.0: 14.32 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:57.23 +42:20:13.0: 14.42 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.13 20:44:38.24 +41:42:35.0
81.83432 -0.66407 galactic Cyg Second-epoch detections are separated by 2.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.1596+41.7098 | 20:44:38.24 +41:42:35.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.589+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:38.24 +41:42:35.0: 14.32 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:38.24 +41:42:35.0: 14.42 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.1596+41.7098,2461300.8725,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1596+41.7098 20260917.3725 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.15 20:48:54.03 +41:43:31.6
82.34472 -1.27456 galactic Cyg Second-epoch detections are separated by 3.9" 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 | 20:48:54.03 +41:43:31.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:54.03 +41:43:31.6: 14.36 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:54.03 +41:43:31.6: 14.49 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.38 20:41:37.97 +42:32:55.5
82.14999 0.29228 galactic Cyg Second-epoch detections are separated by 0.1" 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 | 20:41:37.97 +42:32:55.5 (user input) | T | P | (position from user input) SpType: K0: 2010ApJ...720..679B [BKH2010] J204138.0+423254 J-Ks=0.809+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:37.97 +42:32:55.5: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:37.97 +42:32:55.5: 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
target,2461300.8725,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 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 09 17.3725 2461300.8725 12.46 20:48:13.02 +42:09:53.6
82.60586 -0.89894 galactic Cyg Second-epoch detections are separated by 1.5" and 5.5 pix
The object was found in VSX 2" ASASSN-V J204813.17+420952.2
Type: SRS
# Max. Min./Amp. JD0 Period
15.570 g Y 0.400 g 2458646.76600 28.012000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:13.02 +42:09:53.6: 13.32 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:13.02 +42:09:53.6: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J204813.17+420952.2,2461300.8725,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J204813.17+420952.2 20260917.3725 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.44 20:49:44.10 +42:13:14.1
82.82657 -1.08186 galactic Cyg Second-epoch detections are separated by 1.0" 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 | 20:49:44.10 +42:13:14.1 (user input) | T | P | (position from user input) J-Ks=0.568+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:44.10 +42:13:14.1: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:44.10 +42:13:14.1: 13.41 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 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 09 17.3725 2461300.8725 13.23 20:42:23.84 +42:34:02.8
82.25133 0.19279 galactic Cyg Second-epoch detections are separated by 1.7" and 5.4 pix
The object was found in VSX 1" Gaia DR3 2066530253276707200
Type: ROT
# Max. Min./Amp. JD0 Period
14.170 G 14.210 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:23.84 +42:34:02.8: 14.39 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:23.84 +42:34:02.8: 14.62 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066530253276707200,2461300.8725,13.23,0.05,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
Gaia DR3 2066530253276707200 20260917.3725 13.23CV 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 09 17.3725 2461300.8725 13.24 20:39:29.97 +42:21:52.0
81.76345 0.49077 galactic Cyg Second-epoch detections are separated by 1.4" 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 | 20:39:29.97 +42:21:52.0 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.646+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:29.97 +42:21:52.0: 14.39 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:29.97 +42:21:52.0: 14.41 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.24,0.05,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 20260917.3725 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.50 20:41:38.95 +42:20:53.0
81.99348 0.16662 galactic Cyg Second-epoch detections are separated by 0.9" and 5.8 pix
The object was found in VSX22" Gaia DR3 2066520735629075840
Type: ROT
# Max. Min./Amp. JD0 Period
15.680 G 15.710 G K
ATTENTION: measured mag 12.50 is 3.2 mag brighter than the VSX record maximum brightness 15.68 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:38.95 +42:20:53.0: 13.36 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:38.95 +42:20:53.0: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 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
Gaia DR3 2066520735629075840,2461300.8725,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066520735629075840 20260917.3725 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.29 20:41:43.44 +42:26:21.8
82.07403 0.21183 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:41:43.44 +42:26:21.8 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.596+/-0.038 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:43.44 +42:26:21.8: 14.50 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:43.44 +42:26:21.8: 14.83 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.29,0.05,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 20260917.3725 13.29CV 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 09 17.3725 2461300.8725 12.64 20:43:48.63 +42:00:25.1
81.97200 -0.35894 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 J310.9557+42.0098 | 20:43:48.63 +42:00:25.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.303+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:48.63 +42:00:25.1: 13.57 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:48.63 +42:00:25.1: 13.67 +/- 0.05 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
ATO J310.9557+42.0098,2461300.8725,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J310.9557+42.0098 20260917.3725 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.71 20:39:14.40 +42:36:13.9
81.92422 0.67453 galactic Cyg Second-epoch detections are separated by 0.8" 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 | 20:39:14.40 +42:36:13.9 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:14.40 +42:36:13.9: 13.59 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:14.40 +42:36:13.9: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461300.8725,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.71 20:54:00.19 +41:34:00.3
82.82957 -2.11063 galactic Cyg Second-epoch detections are separated by 0.7" and 5.8 pix
The object was found in VSX 1" Gaia DR3 2065600135164172416
Type: ROT
# Max. Min./Amp. JD0 Period
13.390 G 13.410 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:00.19 +41:34:00.3: 13.59 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:00.19 +41:34:00.3: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065600135164172416,2461300.8725,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065600135164172416 20260917.3725 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.60 20:53:10.52 +42:10:28.5
83.19704 -1.60238 galactic Cyg Second-epoch detections are separated by 0.5" and 5.7 pix
The object was found in VSX24" ZTF J205312.26+421042.8
Type: EA
# Max. Min./Amp. JD0 Period
17.877 r Y 0.123 r 2458322.88910 1.669709800000
ATTENTION: measured mag 12.60 is 5.2 mag brighter than the VSX record maximum brightness 17.75 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:10.52 +42:10:28.5: 13.58 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:10.52 +42:10:28.5: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205312.26+421042.8,2461300.8725,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205312.26+421042.8 20260917.3725 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.71 20:48:01.31 +41:18:26.8
81.91634 -1.41011 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:01.31 +41:18:26.8 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:01.31 +41:18:26.8: 13.57 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:01.31 +41:18:26.8: 13.83 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.70 20:54:49.61 +41:53:51.9
83.18204 -2.01523 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:49.61 +41:53:51.9 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.050 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:49.61 +41:53:51.9: 13.58 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:49.61 +41:53:51.9: 13.68 +/- 0.06 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
target,2461300.8725,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.62 20:47:25.54 +42:21:01.8
82.65819 -0.66839 galactic Cyg Second-epoch detections are separated by 2.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.8469+42.3548 | 20:47:22.40 +42:20:52.9 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G/K 2013AJ....145..102L PM J20473+4220
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:25.54 +42:21:01.8: 13.55 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:25.54 +42:21:01.8: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.8469+42.3548,2461300.8725,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.8469+42.3548 20260917.3725 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.64 20:40:18.25 +44:40:33.5
83.68437 1.78542 galactic Cyg Second-epoch detections are separated by 0.5" 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 J310.0884+44.6741 | 20:40:18.32 +44:40:32.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.496+/-0.040 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:18.25 +44:40:33.5: 13.55 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:18.25 +44:40:33.5: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.0884+44.6741,2461300.8725,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J310.0884+44.6741 20260917.3725 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.57 20:51:05.07 +41:46:59.9
82.64760 -1.55309 galactic Cyg Second-epoch detections are separated by 1.6" 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 J312.7714+41.7834 | 20:51:05.07 +41:46:59.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.469+/-0.026 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:05.07 +41:46:59.9: 13.55 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:05.07 +41:46:59.9: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7714+41.7834,2461300.8725,12.57,0.05,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
ATO J312.7714+41.7834 20260917.3725 12.57CV 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 09 17.3725 2461300.8725 12.60 20:43:32.97 +41:50:10.8
81.80792 -0.42644 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 | target | 20:43:32.97 +41:50:10.8 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=1.317+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:32.97 +41:50:10.8: 13.56 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:32.97 +41:50:10.8: 13.68 +/- 0.05 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,2461300.8725,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.68 20:42:56.03 +41:57:52.2
81.83789 -0.25716 galactic Cyg Second-epoch detections are separated by 0.8" and 5.7 pix
The object was found in VSX 1" Gaia DR3 2066450538683527168
Type: ROT
# Max. Min./Amp. JD0 Period
13.310 G 13.340 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:56.03 +41:57:52.2: 13.56 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:56.03 +41:57:52.2: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.63 +/- 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 2066450538683527168,2461300.8725,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066450538683527168 20260917.3725 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.61 20:42:10.39 +42:37:32.6
82.27184 0.26118 galactic Cyg Second-epoch detections are separated by 0.4" 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 | 20:42:10.39 +42:37:32.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.479+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:10.39 +42:37:32.6: 13.55 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:10.39 +42:37:32.6: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.60 20:42:16.86 +43:17:16.3
82.80580 0.65327 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2066587045627107968 | 20:42:16.86 +43:17:16.3 (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) SpType: K7 (LAMOST DR5)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:16.86 +43:17:16.3: 13.55 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:16.86 +43:17:16.3: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2066587045627107968,2461300.8725,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2066587045627107968 20260917.3725 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.56 20:51:46.14 +41:34:27.2
82.56772 -1.78477 galactic Cyg Second-epoch detections are separated by 0.5" and 5.7 pix
The object was found in VSX16" Gaia DR3 2065774545192318848
Type: YSO
# Max. Min./Amp. JD0 Period
18.210 G 18.320 G
ATTENTION: measured mag 12.56 is 5.7 mag brighter than the VSX record maximum brightness 18.21 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:46.14 +41:34:27.2: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:46.14 +41:34:27.2: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065774545192318848,2461300.8725,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065774545192318848 20260917.3725 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.54 20:51:19.07 +41:55:31.4
82.78491 -1.49621 galactic Cyg Second-epoch detections are separated by 1.7" 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 | ATO J312.8177+41.9262 | 20:51:19.07 +41:55:31.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.501+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:19.07 +41:55:31.4: 13.53 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:19.07 +41:55:31.4: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.8177+41.9262,2461300.8725,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.8177+41.9262 20260917.3725 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.54 20:50:41.16 +41:48:29.3
82.61956 -1.47996 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 J312.6717+41.8080 | 20:50:41.16 +41:48:29.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.445+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:41.16 +41:48:29.3: 13.53 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:41.16 +41:48:29.3: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.6717+41.8080,2461300.8725,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.6717+41.8080 20260917.3725 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.64 20:49:39.00 +41:39:42.7
82.38384 -1.42319 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.4123+41.6620 | 20:49:39.00 +41:39:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.462+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:39.00 +41:39:42.7: 13.52 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:39.00 +41:39:42.7: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.4123+41.6620,2461300.8725,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.4123+41.6620 20260917.3725 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.57 20:41:07.89 +42:34:21.4
82.11217 0.37981 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:41:07.89 +42:34:21.4 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.385+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:07.89 +42:34:21.4: 13.50 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:07.89 +42:34:21.4: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.57,0.05,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
target 20260917.3725 12.57CV 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 09 17.3725 2461300.8725 12.55 20:47:59.59 +42:39:40.4
82.96565 -0.55452 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 | target | 20:47:59.59 +42:39:40.4 (user input) | T | P | (position from user input) J-Ks=0.509+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:59.59 +42:39:40.4: 13.52 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:59.59 +42:39:40.4: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.45 20:51:56.14 +41:55:20.1
82.85575 -1.58677 galactic Cyg Second-epoch detections are separated by 0.4" 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 | ATO J312.9837+41.9220 | 20:51:56.14 +41:55:20.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.498+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:56.14 +41:55:20.1: 13.51 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:56.14 +41:55:20.1: 13.50 +/- 0.05 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
ATO J312.9837+41.9220,2461300.8725,12.45,0.05,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 J312.9837+41.9220 20260917.3725 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 09 17.3725 2461300.8725 12.62 20:51:03.76 +42:29:30.0
83.19179 -1.09943 galactic Cyg Second-epoch detections are separated by 1.4" 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 J312.7531+42.4985 | 20:51:03.76 +42:29:30.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.355+/-0.034 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:03.76 +42:29:30.0: 13.48 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:03.76 +42:29:30.0: 13.64 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7531+42.4985,2461300.8725,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.7531+42.4985 20260917.3725 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.32 20:40:56.22 +42:27:26.1
81.99905 0.33743 galactic Cyg Second-epoch detections are separated by 3.2" and 5.7 pix
The object was found in VSX23" Gaia DR3 2066525305474304896
Type: E
# Max. Min./Amp. JD0 Period
17.460 G 18.250 G 0.300937000000
ATTENTION: measured mag 13.32 is 4.1 mag brighter than the VSX record maximum brightness 17.46 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:56.22 +42:27:26.1: 14.48 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:56.22 +42:27:26.1: 14.60 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066525305474304896,2461300.8725,13.32,0.05,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 2066525305474304896 20260917.3725 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.64 20:39:59.71 +43:51:28.4
83.00241 1.32980 galactic Cyg Second-epoch detections are separated by 0.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:39:59.71 +43:51:28.4 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:59.71 +43:51:28.4: 13.48 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:59.71 +43:51:28.4: 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,2461300.8725,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.46 20:53:11.56 +42:31:53.6
83.47320 -1.37604 galactic Cyg Second-epoch detections are separated by 1.6" and 5.8 pix
The object was found in VSX 0" Gaia DR3 2065969227472280320
Type: ROT
# Max. Min./Amp. JD0 Period
13.240 G 13.270 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:11.56 +42:31:53.6: 13.48 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:11.56 +42:31:53.6: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065969227472280320,2461300.8725,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065969227472280320 20260917.3725 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.60 20:47:05.03 +41:46:42.6
82.17286 -0.97776 galactic Cyg Second-epoch detections are separated by 1.8" 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 | ATO J311.7739+41.7774 | 20:47:05.03 +41:46:42.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.064+/-0.027 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:05.03 +41:46:42.6: 13.48 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:05.03 +41:46:42.6: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.7739+41.7774,2461300.8725,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.7739+41.7774 20260917.3725 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.58 20:39:41.84 +42:39:33.3
82.01939 0.64157 galactic Cyg Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J309.9286+42.6583 | 20:39:41.84 +42:39:33.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=1.032+/-0.028 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:41.84 +42:39:33.3: 13.49 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:41.84 +42:39:33.3: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J309.9286+42.6583,2461300.8725,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.9286+42.6583 20260917.3725 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.53 20:43:28.61 +42:08:56.5
82.04526 -0.22239 galactic Cyg Second-epoch detections are separated by 1.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:43:28.61 +42:08:56.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.016+/-0.030 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:28.61 +42:08:56.5: 13.50 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:28.61 +42:08:56.5: 13.60 +/- 0.05 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,2461300.8725,12.53,0.05,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 20260917.3725 12.53CV 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 09 17.3725 2461300.8725 12.59 20:50:11.34 +41:48:51.0
82.56544 -1.40455 galactic Cyg Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:11.34 +41:48:51.0 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.026 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:11.34 +41:48:51.0: 13.48 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:11.34 +41:48:51.0: 13.65 +/- 0.05 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,2461300.8725,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.57 20:52:11.10 +40:52:50.6
82.08317 -2.28733 galactic Cyg Second-epoch detections are separated by 0.3" 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 | ATO J313.0366+40.8717 | 20:52:11.10 +40:52:50.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.416+/-0.037 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:11.10 +40:52:50.6: 13.48 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:11.10 +40:52:50.6: 13.58 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.0366+40.8717,2461300.8725,12.57,0.05,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
ATO J313.0366+40.8717 20260917.3725 12.57CV 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 09 17.3725 2461300.8725 12.52 20:41:20.93 +42:27:53.5
82.05163 0.28209 galactic Cyg Second-epoch detections are separated by 1.8" and 5.8 pix
The object was found in VSX 0" Gaia DR3 2066525855230109568
Type: ROT
# Max. Min./Amp. JD0 Period
13.330 G 13.360 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:20.93 +42:27:53.5: 13.45 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:20.93 +42:27:53.5: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066525855230109568,2461300.8725,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066525855230109568 20260917.3725 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.64 20:39:55.86 +44:31:04.8
83.51861 1.74163 galactic Cyg Second-epoch detections are separated by 1.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:39:55.86 +44:31:04.8 (user input) | T | P | (position from user input) J-Ks=0.999+/-0.029 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:55.86 +44:31:04.8: 13.47 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:55.86 +44:31:04.8: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.49 20:39:41.40 +44:46:56.4
83.70212 1.93674 galactic Cyg Second-epoch detections are separated by 0.3" 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 | Gaia DR3 2070277693844328832 | 20:39:41.52 +44:46:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.709+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:41.40 +44:46:56.4: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:41.40 +44:46:56.4: 13.66 +/- 0.05 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 2070277693844328832,2461300.8725,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2070277693844328832 20260917.3725 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.12 20:43:48.81 +42:30:50.9
82.37054 -0.04528 galactic Cyg Second-epoch detections are separated by 2.4" 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 | 20:43:48.81 +42:30:50.9 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.499+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:48.81 +42:30:50.9: 14.45 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:48.81 +42:30:50.9: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.30 +/- 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,2461300.8725,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.61 20:48:32.20 +41:37:34.3
82.22481 -1.28441 galactic Cyg Second-epoch detections are separated by 1.1" 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 J312.1310+41.6261 | 20:48:32.20 +41:37:34.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.542+/-0.026 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:32.20 +41:37:34.3: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:32.20 +41:37:34.3: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.1310+41.6261,2461300.8725,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.1310+41.6261 20260917.3725 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.24 20:52:26.11 +41:16:10.2
82.41272 -2.07538 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:52:26.11 +41:16:10.2 (user input) | T | P | (position from user input) J-Ks=1.156+/-0.025 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:26.11 +41:16:10.2: 14.47 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:26.11 +41:16:10.2: 14.62 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.24,0.05,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 20260917.3725 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.54 20:48:53.30 +41:48:49.1
82.41172 -1.21716 galactic Cyg Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:53.30 +41:48:49.1 (user input) | T | P | (position from user input) J-Ks=0.622+/-0.026 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:53.30 +41:48:49.1: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:53.30 +41:48:49.1: 13.57 +/- 0.06 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,2461300.8725,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.54 20:53:32.74 +42:14:22.0
83.29082 -1.61340 galactic Cyg Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:53:32.74 +42:14:22.0 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:32.74 +42:14:22.0: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:32.74 +42:14:22.0: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.21 20:50:53.04 +40:56:35.2
81.97471 -2.05807 galactic Cyg Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.7219+40.9320 | 20:50:53.04 +40:56:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:53.04 +40:56:35.2: 14.44 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:53.04 +40:56:35.2: 14.38 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7219+40.9320,2461300.8725,13.21,0.05,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
ATO J312.7219+40.9320 20260917.3725 13.21CV 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 09 17.3725 2461300.8725 12.51 20:48:23.46 +41:52:15.1
82.39775 -1.10918 galactic Cyg Second-epoch detections are separated by 0.3" 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 J312.0848+41.8754 | 20:48:23.46 +41:52:15.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.308+/-0.029 (F)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:23.46 +41:52:15.1: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:23.46 +41:52:15.1: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.0848+41.8754,2461300.8725,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.0848+41.8754 20260917.3725 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.23 20:50:25.72 +41:47:32.1
82.57683 -1.45299 galactic Cyg Second-epoch detections are separated by 4.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:25.72 +41:47:32.1 (user input) | T | P | (position from user input) J-Ks=1.707+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:25.72 +41:47:32.1: 14.49 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:25.72 +41:47:32.1: 14.61 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.23,0.05,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 20260917.3725 13.23CV 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 09 17.3725 2461300.8725 12.53 20:38:25.48 +43:01:53.3
82.17296 1.05314 galactic Cyg Second-epoch detections are separated by 1.0" and 5.8 pix
The object was found in VSX 0" ASASSN-V J203825.49+430153.7
Type: EA
# Max. Min./Amp. JD0 Period
13.370 V 13.470 V 2457245.83000 2.386300000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:38:25.48 +43:01:53.3: 13.42 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:38:25.48 +43:01:53.3: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 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
ASASSN-V J203825.49+430153.7,2461300.8725,12.53,0.05,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
ASASSN-V J203825.49+430153.7 20260917.3725 12.53CV 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 09 17.3725 2461300.8725 12.47 20:46:57.01 +42:21:26.2
82.60837 -0.59572 galactic Cyg Second-epoch detections are separated by 1.2" 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 | Gaia DR3 2066664251960960384 | 20:46:53.82 +42:21:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.370+/-0.045 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:57.01 +42:21:26.2: 13.43 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:57.01 +42:21:26.2: 13.52 +/- 0.05 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 2066664251960960384,2461300.8725,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066664251960960384 20260917.3725 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 09 17.3725 2461300.8725 12.50 20:34:39.22 +44:00:04.4
82.53563 2.18289 galactic Cyg Second-epoch detections are separated by 0.8" 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 | 20:34:39.22 +44:00:04.4 (user input) | T | P | (position from user input) J-Ks=1.130+/-0.028 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:34:39.22 +44:00:04.4: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:34:39.22 +44:00:04.4: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 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,2461300.8725,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.53 20:48:39.23 +41:57:07.3
82.49161 -1.09601 galactic Cyg Second-epoch detections are separated by 1.1" 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 J312.1685+41.9448 | 20:48:39.23 +41:57:07.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.521+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:39.23 +41:57:07.3: 13.39 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:39.23 +41:57:07.3: 13.54 +/- 0.05 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 J312.1685+41.9448,2461300.8725,12.53,0.05,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
ATO J312.1685+41.9448 20260917.3725 12.53CV 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 09 17.3725 2461300.8725 12.48 20:51:49.86 +41:28:19.7
82.49643 -1.85879 galactic Cyg Second-epoch detections are separated by 0.2" 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 | 20:51:49.86 +41:28:19.7 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.025 (F)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:49.86 +41:28:19.7: 13.41 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:49.86 +41:28:19.7: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.48,0.05,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 20260917.3725 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 09 17.3725 2461300.8725 12.48 20:47:03.33 +42:47:09.3
82.95455 -0.34219 galactic Cyg Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:47:03.33 +42:47:09.3 (user input) | T | P | (position from user input) SpType: A0 (LAMOST DR5) J-Ks=0.559+/-0.034 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:03.33 +42:47:09.3: 13.41 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:03.33 +42:47:09.3: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.48,0.05,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 20260917.3725 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 09 17.3725 2461300.8725 12.52 20:49:24.04 +41:41:59.4
82.38382 -1.36311 galactic Cyg Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:24.04 +41:41:59.4 (user input) | T | P | (position from user input) J-Ks=0.315+/-0.034 (F)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:24.04 +41:41:59.4: 13.41 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:24.04 +41:41:59.4: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.49 20:40:39.24 +42:33:46.5
82.05065 0.44337 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 | target | 20:40:39.24 +42:33:46.5 (user input) | T | P | (position from user input) SpType: K0? 2010ApJ...720..679B [BKH2010] J204039.2+423347 J-Ks=1.024+/-0.031 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:39.24 +42:33:46.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:39.24 +42:33:46.5: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.50 20:52:06.36 +42:31:31.5
83.34037 -1.22609 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 | target | 20:52:06.36 +42:31:31.5 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:06.36 +42:31:31.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:06.36 +42:31:31.5: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.48 20:51:09.25 +41:37:26.0
82.53281 -1.66451 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 J312.7884+41.6239 | 20:51:09.25 +41:37:26.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.363+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:09.25 +41:37:26.0: 13.39 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:09.25 +41:37:26.0: 13.54 +/- 0.05 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 J312.7884+41.6239,2461300.8725,12.48,0.05,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
ATO J312.7884+41.6239 20260917.3725 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 09 17.3725 2461300.8725 12.47 20:40:48.41 +44:40:10.2
83.73391 1.71074 galactic Cyg Second-epoch detections are separated by 0.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:48.41 +44:40:10.2 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:48.41 +44:40:10.2: 13.39 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:48.41 +44:40:10.2: 13.39 +/- 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,2461300.8725,12.47,0.05,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 20260917.3725 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 09 17.3725 2461300.8725 13.29 20:50:20.72 +41:43:22.4
82.51333 -1.48497 galactic Cyg Second-epoch detections are separated by 2.6" 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 J312.5827+41.7227 | 20:50:20.72 +41:43:22.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.594+/-0.026 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:20.72 +41:43:22.4: 14.46 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:20.72 +41:43:22.4: 14.38 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.5827+41.7227,2461300.8725,13.29,0.05,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 J312.5827+41.7227 20260917.3725 13.29CV 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 09 17.3725 2461300.8725 12.44 20:46:48.48 +41:08:06.5
81.63888 -1.34049 galactic Cyg Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:48.48 +41:08:06.5 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:48.48 +41:08:06.5: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:48.48 +41:08:06.5: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 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 09 17.3725 2461300.8725 12.39 20:41:05.93 +42:24:42.0
81.98133 0.28590 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 | target | 20:41:05.93 +42:24:42.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.379+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:05.93 +42:24:42.0: 13.35 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:05.93 +42:24:42.0: 13.30 +/- 0.04 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
target,2461300.8725,12.39,0.05,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 20260917.3725 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 09 17.3725 2461300.8725 13.29 20:45:32.53 +42:12:28.1
82.32892 -0.48582 galactic Cyg Second-epoch detections are separated by 1.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:45:32.53 +42:12:28.1 (user input) | T | P | (position from user input) J-Ks=0.678+/-0.035 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:32.53 +42:12:28.1: 14.38 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:32.53 +42:12:28.1: 14.48 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.29,0.05,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 20260917.3725 13.29CV 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 09 17.3725 2461300.8725 12.40 20:51:17.31 +41:50:44.9
82.72003 -1.54265 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.8219+41.8458 | 20:51:17.31 +41:50:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.408+/-0.037 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:17.31 +41:50:44.9: 13.39 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:17.31 +41:50:44.9: 13.40 +/- 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 J312.8219+41.8458,2461300.8725,12.40,0.05,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
ATO J312.8219+41.8458 20260917.3725 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 09 17.3725 2461300.8725 12.44 20:49:38.36 +41:42:49.3
82.42273 -1.38885 galactic Cyg Second-epoch detections are separated by 1.2" 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 | 20:49:38.36 +41:42:49.3 (user input) | T | P | (position from user input) J-Ks=1.008+/-0.029 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:38.36 +41:42:49.3: 13.37 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:38.36 +41:42:49.3: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 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 09 17.3725 2461300.8725 12.47 20:41:52.91 +42:11:50.4
81.90103 0.04003 galactic Cyg Second-epoch detections are separated by 0.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:52.91 +42:11:50.4 (user input) | T | P | (position from user input) SpType: G4: 2010ApJ...720..679B [BKH2010] J204152.9+421150 J-Ks=1.202+/-0.030 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:52.91 +42:11:50.4: 13.35 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:52.91 +42:11:50.4: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 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
target,2461300.8725,12.47,0.05,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 20260917.3725 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 09 17.3725 2461300.8725 12.44 20:50:43.74 +42:05:55.4
82.84915 -1.30157 galactic Cyg Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:43.74 +42:05:55.4 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:43.74 +42:05:55.4: 13.35 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:43.74 +42:05:55.4: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 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 09 17.3725 2461300.8725 12.38 20:43:43.35 +42:21:50.5
82.24227 -0.12505 galactic Cyg Second-epoch detections are separated by 0.8" 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 | ATO J310.9288+42.3669 | 20:43:43.34 +42:21:51.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.458+/-9.995 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:43.35 +42:21:50.5: 13.36 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:43.35 +42:21:50.5: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.9288+42.3669,2461300.8725,12.38,0.05,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
ATO J310.9288+42.3669 20260917.3725 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 09 17.3725 2461300.8725 12.37 20:43:56.67 +42:25:37.2
82.31710 -0.11822 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 | target | 20:43:56.67 +42:25:37.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.379+/-0.034 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:56.67 +42:25:37.2: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:56.67 +42:25:37.2: 13.64 +/- 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
target,2461300.8725,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 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 09 17.3725 2461300.8725 12.42 20:46:56.69 +43:01:26.9
83.12749 -0.17710 galactic Cyg Second-epoch detections are separated by 1.2" 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 J311.7345+43.0220 | 20:46:56.69 +43:01:26.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.349+/-0.038 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:56.69 +43:01:26.9: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:56.69 +43:01:26.9: 13.40 +/- 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
ATO J311.7345+43.0220,2461300.8725,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.7345+43.0220 20260917.3725 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.29 20:43:06.16 +42:25:20.9
82.21743 0.00103 galactic Cyg Second-epoch detections are separated by 0.1" 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 | 20:43:06.16 +42:25:20.9 (user input) | T | P | (position from user input) J-Ks=0.544+/-0.035 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:06.16 +42:25:20.9: 14.39 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:06.16 +42:25:20.9: 14.50 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.43 +/- 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,2461300.8725,13.29,0.05,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 20260917.3725 13.29CV 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 09 17.3725 2461300.8725 12.29 20:51:02.18 +41:32:18.8
82.45290 -1.70177 galactic Cyg Second-epoch detections are separated by 0.2" 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 | ATO J312.7587+41.5384 | 20:51:02.18 +41:32:18.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.526+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:02.18 +41:32:18.8: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:02.18 +41:32:18.8: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7587+41.5384,2461300.8725,12.29,0.05,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 J312.7587+41.5384 20260917.3725 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 09 17.3725 2461300.8725 13.19 20:51:27.41 +41:53:07.5
82.77055 -1.54160 galactic Cyg Second-epoch detections are separated by 0.8" 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 | ATO J312.8639+41.8850 | 20:51:27.41 +41:53:07.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.408+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:27.41 +41:53:07.5: 14.38 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:27.41 +41:53:07.5: 14.51 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.8639+41.8850,2461300.8725,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.8639+41.8850 20260917.3725 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.37 20:40:11.51 +42:24:38.9
81.87819 0.41777 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J310.0480+42.4107 | 20:40:11.51 +42:24:38.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.327+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:11.51 +42:24:38.9: 13.32 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:11.51 +42:24:38.9: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 J310.0480+42.4107,2461300.8725,12.37,0.05,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 J310.0480+42.4107 20260917.3725 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 09 17.3725 2461300.8725 12.36 20:47:51.49 +41:57:28.1
82.40296 -0.97743 galactic Cyg Second-epoch detections are separated by 0.2" 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 | ATO J311.9646+41.9575 | 20:47:51.49 +41:57:28.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.305+/-0.030 (F)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:51.49 +41:57:28.1: 13.31 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:51.49 +41:57:28.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 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 J311.9646+41.9575,2461300.8725,12.36,0.05,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 J311.9646+41.9575 20260917.3725 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 09 17.3725 2461300.8725 12.30 20:53:21.23 +42:19:15.9
83.33070 -1.53381 galactic Cyg Second-epoch detections are separated by 1.6" and 5.6 pix
The object was found in VSX13" Gaia DR3 2065911262593617536
Type: ROT
# Max. Min./Amp. JD0 Period
14.370 G 14.400 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:21.23 +42:19:15.9: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:21.23 +42:19:15.9: 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
Gaia DR3 2065911262593617536,2461300.8725,12.30,0.05,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 2065911262593617536 20260917.3725 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 09 17.3725 2461300.8725 12.35 20:40:58.64 +43:27:45.7
82.79827 0.94760 galactic Cyg Second-epoch detections are separated by 0.4" and 5.7 pix
The object was found in VSX 6" ASASSN-V J204058.09+432744.7
Type: CWB
# Max. Min./Amp. JD0 Period
13.700 V 13.860 V 2457693.78000 10.910000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:58.64 +43:27:45.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:58.64 +43:27:45.7: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 J204058.09+432744.7,2461300.8725,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J204058.09+432744.7 20260917.3725 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.12 20:46:54.96 +42:39:27.0
82.83842 -0.40270 galactic Cyg Second-epoch detections are separated by 2.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:54.96 +42:39:27.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:54.96 +42:39:27.0: 14.36 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:54.96 +42:39:27.0: 14.56 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.18 20:46:00.19 +42:18:21.6
82.45889 -0.49123 galactic Cyg Second-epoch detections are separated by 3.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:00.19 +42:18:21.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.517+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:00.19 +42:18:21.6: 14.36 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:00.19 +42:18:21.6: 14.40 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.38 +/- 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,2461300.8725,13.18,0.05,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 20260917.3725 13.18CV 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 09 17.3725 2461300.8725 13.23 20:37:34.46 +43:31:51.0
82.47664 1.47874 galactic Cyg Second-epoch detections are separated by 2.1" and 5.9 pix
The object was found in VSX 1" Gaia DR3 2069640359355250048
Type: ROT
# Max. Min./Amp. JD0 Period
14.030 G 14.060 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:37:34.46 +43:31:51.0: 14.35 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:37:34.46 +43:31:51.0: 14.51 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2069640359355250048,2461300.8725,13.23,0.05,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
Gaia DR3 2069640359355250048 20260917.3725 13.23CV 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 09 17.3725 2461300.8725 13.21 20:43:30.49 +42:12:43.6
82.09841 -0.18793 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 | target | 20:43:30.49 +42:12:43.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.536+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:30.49 +42:12:43.6: 14.33 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:30.49 +42:12:43.6: 14.46 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.37 +/- 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,2461300.8725,13.21,0.05,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 20260917.3725 13.21CV 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 09 17.3725 2461300.8725 13.10 20:45:20.32 +42:15:12.9
82.34126 -0.42784 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 | ATO J311.3349+42.2534 | 20:45:20.32 +42:15:12.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.853+/-0.028 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:20.32 +42:15:12.9: 14.36 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:20.32 +42:15:12.9: 14.45 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.3349+42.2534,2461300.8725,13.10,0.05,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
ATO J311.3349+42.2534 20260917.3725 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.32 20:44:28.34 +42:14:08.7
82.22759 -0.31336 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 J311.1180+42.2357 | 20:44:28.34 +42:14:08.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.354+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:28.34 +42:14:08.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:28.34 +42:14:08.7: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 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 J311.1180+42.2357,2461300.8725,12.32,0.05,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
ATO J311.1180+42.2357 20260917.3725 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 09 17.3725 2461300.8725 12.35 20:15:17.99 +46:27:35.3
82.59580 6.38307 galactic Cyg Second-epoch detections are separated by 1.4" and 5.5 pix
The object was found in VSX 2" ASASSN-V J201517.88+462737.3
Type: SR
# Max. Min./Amp. JD0 Period
13.680 V 13.780 V 2458431.72000 49.440000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:15:17.99 +46:27:35.3: 13.31 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:15:17.99 +46:27:35.3: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201517.88+462737.3,2461300.8725,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201517.88+462737.3 20260917.3725 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.06 20:50:43.06 +41:53:42.4
82.69051 -1.42928 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 | ATO J312.6762+41.8852 | 20:50:43.06 +41:53:42.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.641+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:43.06 +41:53:42.4: 14.35 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:43.06 +41:53:42.4: 14.34 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.6762+41.8852,2461300.8725,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.6762+41.8852 20260917.3725 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.26 20:51:01.65 +41:37:20.3
82.51652 -1.64725 galactic Cyg Second-epoch detections are separated by 0.8" 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 J312.7570+41.6224 | 20:51:01.69 +41:37:20.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.613+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:01.65 +41:37:20.3: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:01.65 +41:37:20.3: 13.47 +/- 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
ATO J312.7570+41.6224,2461300.8725,12.26,0.05,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 J312.7570+41.6224 20260917.3725 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 09 17.3725 2461300.8725 13.24 20:43:22.33 +42:52:06.8
82.59876 0.23775 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 | 20:43:22.33 +42:52:06.8 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.539+/-0.042 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:22.33 +42:52:06.8: 14.31 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:22.33 +42:52:06.8: 14.56 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.38 +/- 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,2461300.8725,13.24,0.05,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 20260917.3725 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.28 20:42:32.70 +44:14:46.6
83.59028 1.20606 galactic Cyg Second-epoch detections are separated by 1.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:32.70 +44:14:46.6 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.511+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:32.70 +44:14:46.6: 14.29 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:32.70 +44:14:46.6: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.31 +/- 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,2461300.8725,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.39 20:41:43.82 +43:06:18.7
82.60003 0.62004 galactic Cyg Second-epoch detections are separated by 0.9" and 5.8 pix
The object was found in VSX 0" ZTF J204143.81+430618.7
Type: EW
# Max. Min./Amp. JD0 Period
12.870 r Y 0.411 r 2458274.96820 0.631824000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:43.82 +43:06:18.7: 13.20 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:43.82 +43:06:18.7: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204143.81+430618.7,2461300.8725,12.39,0.05,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
ZTF J204143.81+430618.7 20260917.3725 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 09 17.3725 2461300.8725 13.20 20:45:07.57 +41:35:23.8
81.79728 -0.81007 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 | target | 20:45:07.57 +41:35:23.8 (user input) | T | P | (position from user input) J-Ks=1.599+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:07.57 +41:35:23.8: 14.31 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:07.57 +41:35:23.8: 14.60 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.38 +/- 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,2461300.8725,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.20CV 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 09 17.3725 2461300.8725 12.23 20:43:13.54 +42:22:47.0
82.19785 -0.04324 galactic Cyg Second-epoch detections are separated by 1.1" 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 2066477511078179840 | 20:43:13.83 +42:22:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.464+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:13.54 +42:22:47.0: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:13.54 +42:22:47.0: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066477511078179840,2461300.8725,12.23,0.05,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
Gaia DR3 2066477511078179840 20260917.3725 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 09 17.3725 2461300.8725 13.17 20:48:47.96 +42:14:18.9
82.73106 -0.93624 galactic Cyg Second-epoch detections are separated by 1.0" 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 | ATO J312.2089+42.2336 | 20:48:47.96 +42:14:18.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.547+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:47.96 +42:14:18.9: 14.24 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:47.96 +42:14:18.9: 13.98 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.2089+42.2336,2461300.8725,13.17,0.05,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
ATO J312.2089+42.2336 20260917.3725 13.17CV 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 09 17.3725 2461300.8725 12.24 20:42:18.04 +42:34:26.4
82.24553 0.21085 galactic Cyg Second-epoch detections are separated by 1.2" 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 | Gaia DR3 2066531004894011520 | 20:42:18.03 +42:34:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.538+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:18.04 +42:34:26.4: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:18.04 +42:34:26.4: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066531004894011520,2461300.8725,12.24,0.05,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 2066531004894011520 20260917.3725 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 09 17.3725 2461300.8725 13.26 20:38:30.98 +42:40:59.5
81.90631 0.82843 galactic Cyg Second-epoch detections are separated by 4.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:38:30.98 +42:40:59.5 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.530+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:38:30.98 +42:40:59.5: 14.26 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:38:30.98 +42:40:59.5: 14.34 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.29 +/- 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,2461300.8725,13.26,0.05,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 20260917.3725 13.26CV 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 09 17.3725 2461300.8725 13.16 20:46:01.52 +42:17:52.8
82.45520 -0.49943 galactic Cyg Second-epoch detections are separated by 2.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:01.52 +42:17:52.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.446+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:01.52 +42:17:52.8: 14.27 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:01.52 +42:17:52.8: 14.54 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.35 +/- 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,2461300.8725,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.28 20:49:49.81 +42:25:12.6
82.99223 -0.96912 galactic Cyg Second-epoch detections are separated by 0.2" and 5.7 pix
The object was found in VSX23" Gaia DR3 2066629724724309504
Type: L
# Max. Min./Amp. JD0 Period
15.770 G 16.340 G M
ATTENTION: measured mag 12.28 is 3.5 mag brighter than the VSX record maximum brightness 15.77 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:49.81 +42:25:12.6: 13.14 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:49.81 +42:25:12.6: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066629724724309504,2461300.8725,12.28,0.05,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 2066629724724309504 20260917.3725 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 09 17.3725 2461300.8725 12.25 20:41:36.24 +42:29:14.6
82.09830 0.25878 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:41:36.24 +42:29:14.6 (user input) | T | P | (position from user input) SpType: A0.5: 2010ApJ...720..679B [BKH2010] J204136.2+422915 J-Ks=0.385+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:36.24 +42:29:14.6: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:36.24 +42:29:14.6: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.25,0.05,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 20260917.3725 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 09 17.3725 2461300.8725 13.04 20:51:18.70 +41:45:29.5
82.65518 -1.60174 galactic Cyg Second-epoch detections are separated by 2.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:51:18.70 +41:45:29.5 (user input) | T | P | (position from user input) J-Ks=0.905+/- (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:18.70 +41:45:29.5: 14.29 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:18.70 +41:45:29.5: 14.44 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.34 +/- 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,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.20 20:40:29.54 +44:41:45.8
83.72072 1.77121 galactic Cyg Second-epoch detections are separated by 1.1" 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 | 20:40:29.54 +44:41:45.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.372+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:29.54 +44:41:45.8: 14.25 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:29.54 +44:41:45.8: 14.30 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.20CV 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 09 17.3725 2461300.8725 13.20 20:41:08.20 +44:26:50.2
83.59414 1.52821 galactic Cyg Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:08.20 +44:26:50.2 (user input) | T | P | (position from user input) J-Ks=1.135+/-0.030 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:08.20 +44:26:50.2: 14.31 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:08.20 +44:26:50.2: 14.28 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.30 +/- 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,2461300.8725,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.20CV 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 09 17.3725 2461300.8725 12.21 20:40:33.71 +42:33:42.3
82.03935 0.45608 galactic Cyg Second-epoch detections are separated by 0.1" 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 | Gaia DR3 2066538495316786688 | 20:40:33.68 +42:33:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0.5? 2010ApJ...720..679B [BKH2010] J204033.6+423342 J-Ks=1.102+/-0.030 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:33.71 +42:33:42.3: 13.14 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:33.71 +42:33:42.3: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066538495316786688,2461300.8725,12.21,0.05,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 2066538495316786688 20260917.3725 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 09 17.3725 2461300.8725 12.20 20:51:30.68 +41:32:16.3
82.50895 -1.77078 galactic Cyg Second-epoch detections are separated by 0.1" 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 | ATO J312.8778+41.5379 | 20:51:30.68 +41:32:16.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.412+/-0.026 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:30.68 +41:32:16.3: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:30.68 +41:32:16.3: 13.17 +/- 0.04 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
ATO J312.8778+41.5379,2461300.8725,12.20,0.05,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 J312.8778+41.5379 20260917.3725 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 09 17.3725 2461300.8725 13.20 20:43:39.89 +43:49:55.4
83.38873 0.79197 galactic Cyg Second-epoch detections are separated by 1.0" 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 | 20:43:39.89 +43:49:55.4 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:39.89 +43:49:55.4: 14.25 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:39.89 +43:49:55.4: 14.60 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.34 +/- 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,2461300.8725,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.20CV 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 09 17.3725 2461300.8725 13.16 20:48:29.57 +41:29:14.6
82.11183 -1.36550 galactic Cyg Second-epoch detections are separated by 1.4" 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 | ATO J312.1235+41.4873 | 20:48:29.57 +41:29:14.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.541+/-0.039 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:29.57 +41:29:14.6: 14.30 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:29.57 +41:29:14.6: 14.27 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.1235+41.4873,2461300.8725,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.1235+41.4873 20260917.3725 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.20 20:43:37.19 +42:26:25.2
82.29047 -0.06293 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:43:37.19 +42:26:25.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.307+/-0.028 (F)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:37.19 +42:26:25.2: 13.07 +/- 0.02 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:37.19 +42:26:25.2: 13.25 +/- 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,2461300.8725,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 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 09 17.3725 2461300.8725 13.05 20:48:41.07 +41:49:47.2
82.40029 -1.17751 galactic Cyg Second-epoch detections are separated by 2.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.1699+41.8322 | 20:48:41.07 +41:49:47.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.532+/-0.026 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:41.07 +41:49:47.2: 14.22 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:41.07 +41:49:47.2: 14.11 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.1699+41.8322,2461300.8725,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.1699+41.8322 20260917.3725 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.22 20:50:03.95 +43:00:11.4
83.47077 -0.63326 galactic Cyg Second-epoch detections are separated by 1.6" 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 | Gaia DR3 2066753415480268800 | 20:50:03.96 +43:00:11.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0: 2018A&A...612A..50B 2MASS J20500395+4300117 J-Ks=1.135+/-0.042 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:03.95 +43:00:11.4: 13.06 +/- 0.02 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:03.95 +43:00:11.4: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 2066753415480268800,2461300.8725,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066753415480268800 20260917.3725 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.11 20:50:58.16 +42:36:05.0
83.26554 -1.01638 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 | target | 20:50:58.16 +42:36:05.0 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.040 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:58.16 +42:36:05.0: 14.22 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:58.16 +42:36:05.0: 14.35 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.26 +/- 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,2461300.8725,13.11,0.05,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 20260917.3725 13.11CV 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 09 17.3725 2461300.8725 13.03 20:50:03.84 +41:50:52.3
82.57675 -1.36519 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 | ATO J312.5162+41.8477 | 20:50:03.84 +41:50:52.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.540+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:03.84 +41:50:52.3: 14.20 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:03.84 +41:50:52.3: 14.31 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.5162+41.8477,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.5162+41.8477 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.19 20:47:51.50 +41:24:19.2
81.97320 -1.32471 galactic Cyg Second-epoch detections are separated by 2.3" 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 | 20:47:51.50 +41:24:19.2 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:51.50 +41:24:19.2: 14.19 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:51.50 +41:24:19.2: 14.26 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.09 20:50:00.64 +42:58:09.8
83.43825 -0.64686 galactic Cyg Second-epoch detections are separated by 1.8" and 5.6 pix
The object was found in VSX 0" Gaia DR3 2066659342819010432
Type: ROT
# Max. Min./Amp. JD0 Period
13.880 G 13.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:00.64 +42:58:09.8: 14.22 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:00.64 +42:58:09.8: 14.23 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066659342819010432,2461300.8725,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066659342819010432 20260917.3725 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:47:09.04 +41:59:16.3
82.34379 -0.85621 galactic Cyg Second-epoch detections are separated by 2.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.7826+42.0000 | 20:47:09.04 +41:59:16.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.469+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:09.04 +41:59:16.3: 14.23 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:09.04 +41:59:16.3: 14.20 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.7826+42.0000,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.7826+42.0000 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.04 20:46:13.93 +43:12:46.4
83.19333 0.04246 galactic Cyg Second-epoch detections are separated by 1.0" and 5.7 pix
The object was found in VSX 0" V3065 Cyg
Type: DCEP
# Max. Min./Amp. JD0 Period
12.950 V 13.690 V 2458001.26200 5.968500000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:13.93 +43:12:46.4: 13.00 +/- 0.03 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:13.93 +43:12:46.4: 13.27 +/- 0.04 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
V3065 Cyg,2461300.8725,12.04,0.05,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
V3065 Cyg 20260917.3725 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 09 17.3725 2461300.8725 12.99 20:46:39.35 +41:43:16.8
82.07828 -0.95133 galactic Cyg Second-epoch detections are separated by 3.1" and 5.9 pix
The object was found in VSX18" ZTF J204639.18+414334.9
Type: SR
# Max. Min./Amp. JD0 Period
17.228 r Y 0.095 r 2458288.92010 83.338282800000
ATTENTION: measured mag 12.99 is 4.1 mag brighter than the VSX record maximum brightness 17.13 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:39.35 +41:43:16.8: 14.01 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:39.35 +41:43:16.8: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204639.18+414334.9,2461300.8725,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204639.18+414334.9 20260917.3725 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.98 20:41:41.09 +42:37:35.5
82.21724 0.33251 galactic Cyg Second-epoch detections are separated by 1.1" 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 | 20:41:41.09 +42:37:35.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.419+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:41.09 +42:37:35.5: 14.21 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:41.09 +42:37:35.5: 14.39 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.20 20:41:21.14 +44:32:39.7
83.69446 1.55734 galactic Cyg Second-epoch detections are separated by 2.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:21.14 +44:32:39.7 (user input) | T | P | (position from user input) J-Ks=0.611+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:21.14 +44:32:39.7: 14.17 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:21.14 +44:32:39.7: 14.27 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.20CV 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 09 17.3725 2461300.8725 13.10 20:41:28.21 +42:27:29.9
82.06019 0.26040 galactic Cyg Second-epoch detections are separated by 1.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:28.21 +42:27:29.9 (user input) | T | P | (position from user input) J-Ks=0.505+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:28.21 +42:27:29.9: 14.18 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:28.21 +42:27:29.9: 14.18 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461300.8725,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.19 20:41:32.33 +44:30:23.9
83.68506 1.50795 galactic Cyg Second-epoch detections are separated by 0.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:32.33 +44:30:23.9 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.056 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:32.33 +44:30:23.9: 14.19 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:32.33 +44:30:23.9: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:52:14.80 +41:10:34.8
82.31833 -2.10760 galactic Cyg Second-epoch detections are separated by 1.1" 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 | 20:52:14.80 +41:10:34.8 (user input) | T | P | (position from user input) J-Ks=1.109+/-0.026 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:14.80 +41:10:34.8: 14.18 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:14.80 +41:10:34.8: 14.26 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.21 +/- 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,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.10 20:53:16.86 +42:09:03.0
83.19136 -1.63263 galactic Cyg Second-epoch detections are separated by 1.4" 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 | 20:53:16.86 +42:09:03.0 (user input) | T | P | (position from user input) J-Ks=0.409+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:16.86 +42:09:03.0: 14.13 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:16.86 +42:09:03.0: 14.01 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.15 20:45:12.41 +42:41:22.6
82.66730 -0.13730 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:45:12.41 +42:41:22.6 (user input) | T | P | (position from user input) J-Ks=1.186+/-0.028 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:12.41 +42:41:22.6: 14.18 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:12.41 +42:41:22.6: 14.36 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.23 +/- 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,2461300.8725,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.14 20:41:20.73 +44:26:46.9
83.61628 1.49820 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 | target | 20:41:20.73 +44:26:46.9 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:20.73 +44:26:46.9: 14.14 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:20.73 +44:26:46.9: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.11 +/- 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,2461300.8725,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.01 20:51:55.06 +41:15:59.2
82.34826 -2.00247 galactic Cyg Second-epoch detections are separated by 0.4" 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 | 20:51:55.06 +41:15:59.2 (user input) | T | P | (position from user input) J-Ks=1.528+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:55.06 +41:15:59.2: 14.17 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:55.06 +41:15:59.2: 14.27 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 11.93 20:50:01.41 +41:46:18.5
82.51311 -1.40754 galactic Cyg Second-epoch detections are separated by 0.1" and 5.7 pix
The object was found in VSX20" ZTF J204959.64+414622.4
Type: EW:
# Max. Min./Amp. JD0 Period
19.196 r Y 0.655 r 2458319.85900 0.724655400000
ATTENTION: measured mag 11.93 is 6.6 mag brighter than the VSX record maximum brightness 18.54 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:01.41 +41:46:18.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:01.41 +41:46:18.5: 13.04 +/- 0.03 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
ZTF J204959.64+414622.4,2461300.8725,11.93,0.05,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
ZTF J204959.64+414622.4 20260917.3725 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 09 17.3725 2461300.8725 13.21 20:42:53.48 +41:50:22.5
81.73473 -0.32805 galactic Cyg Second-epoch detections are separated by 2.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:53.48 +41:50:22.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.201+/-0.033 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:53.48 +41:50:22.5: 14.14 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:53.48 +41:50:22.5: 14.48 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.21,0.05,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 20260917.3725 13.21CV 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 09 17.3725 2461300.8725 12.97 20:44:43.68 +42:20:56.9
82.34582 -0.27999 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 | ATO J311.1803+42.3472 | 20:44:43.68 +42:20:56.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.531+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:43.68 +42:20:56.9: 14.15 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:43.68 +42:20:56.9: 14.18 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.1803+42.3472,2461300.8725,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1803+42.3472 20260917.3725 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.12 20:48:08.95 +41:10:32.1
81.82886 -1.51166 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 | ATO J312.0378+41.1755 | 20:48:08.95 +41:10:32.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.446+/-0.040 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:08.95 +41:10:32.1: 14.13 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:08.95 +41:10:32.1: 14.12 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.0378+41.1755,2461300.8725,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.0378+41.1755 20260917.3725 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.05 20:43:03.84 +42:25:15.8
82.21191 0.00577 galactic Cyg Second-epoch detections are separated by 1.3" and 5.9 pix
The object was found in VSX 2" Gaia DR3 2066478644949553280
Type: ROT
# Max. Min./Amp. JD0 Period
13.930 G 13.950 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:03.84 +42:25:15.8: 14.09 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:03.84 +42:25:15.8: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066478644949553280,2461300.8725,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066478644949553280 20260917.3725 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:48:59.55 +41:55:26.5
82.50961 -1.16254 galactic Cyg Second-epoch detections are separated by 1.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.2481+41.9242 | 20:48:59.55 +41:55:26.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.466+/-0.036 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:59.55 +41:55:26.5: 14.13 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:59.55 +41:55:26.5: 14.20 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.2481+41.9242,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.2481+41.9242 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.16 20:40:04.49 +42:45:08.1
82.13540 0.64338 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 | 20:40:04.49 +42:45:08.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.383+/-0.036 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:04.49 +42:45:08.1: 14.12 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:04.49 +42:45:08.1: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 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,2461300.8725,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.19 20:45:17.66 +43:13:15.4
83.09302 0.18102 galactic Cyg Second-epoch detections are separated by 1.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:45:17.66 +43:13:15.4 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:17.66 +43:13:15.4: 14.15 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:17.66 +43:13:15.4: 14.13 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.14 20:38:49.39 +42:29:54.2
81.79380 0.67131 galactic Cyg Second-epoch detections are separated by 0.2" 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 | 20:38:49.39 +42:29:54.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.503+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:38:49.39 +42:29:54.2: 14.10 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:38:49.39 +42:29:54.2: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.16 20:42:33.74 +42:03:31.4
81.86948 -0.14473 galactic Cyg Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:33.74 +42:03:31.4 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:33.74 +42:03:31.4: 14.09 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:33.74 +42:03:31.4: 14.23 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.18 20:40:42.64 +42:10:43.2
81.75319 0.19990 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 | Large-amplitude variable Gaia DR2 2066427101045440000 | 20:40:42.64 +42:10:43.2 (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=0.460+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:42.64 +42:10:43.2: 14.10 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:42.64 +42:10:43.2: 14.26 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.15 +/- 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
Large-amplitude variable Gaia DR2 2066427101045440000,2461300.8725,13.18,0.05,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
Large-amplitude variable Gaia DR2 2066427101045440000 20260917.3725 13.18CV 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 09 17.3725 2461300.8725 13.00 20:53:06.23 +42:24:01.2
83.36193 -1.44756 galactic Cyg Second-epoch detections are separated by 0.8" 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 | ATO J313.2759+42.4002 | 20:53:06.23 +42:24:01.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.043+/-0.033 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:06.23 +42:24:01.2: 14.10 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:06.23 +42:24:01.2: 14.20 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.2759+42.4002,2461300.8725,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.2759+42.4002 20260917.3725 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.99 20:52:53.29 +40:41:38.1
82.02445 -2.50907 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 | target | 20:52:53.29 +40:41:38.1 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.025 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:53.29 +40:41:38.1: 14.13 +/- 0.08 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:53.29 +40:41:38.1: 14.03 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.08 +/- 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,2461300.8725,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.13 20:48:03.25 +41:34:59.4
82.13458 -1.24142 galactic Cyg Second-epoch detections are separated by 2.1" and 5.6 pix
The object was found in VSX 1" Gaia DR3 2065454449873002496
Type: ROT
# Max. Min./Amp. JD0 Period
13.870 G 13.900 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:03.25 +41:34:59.4: 14.09 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:03.25 +41:34:59.4: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065454449873002496,2461300.8725,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065454449873002496 20260917.3725 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:41:50.65 +42:22:13.8
82.03332 0.15199 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:50.65 +42:22:13.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.462+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:50.65 +42:22:13.8: 14.10 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:50.65 +42:22:13.8: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:50:20.20 +41:52:25.6
82.62900 -1.38802 galactic Cyg Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.5836+41.8739 | 20:50:20.20 +41:52:25.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.645+/-0.026 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:20.20 +41:52:25.6: 14.08 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:20.20 +41:52:25.6: 14.32 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.5836+41.8739,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.5836+41.8739 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.19 20:44:05.94 +41:49:10.2
81.85811 -0.51723 galactic Cyg Second-epoch detections are separated by 1.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:05.94 +41:49:10.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.453+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:05.94 +41:49:10.2: 14.10 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:05.94 +41:49:10.2: 14.39 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461300.8725,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.01 20:46:22.01 +41:40:26.4
82.00760 -0.93885 galactic Cyg Second-epoch detections are separated by 1.0" 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 | 20:46:22.01 +41:40:26.4 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:22.01 +41:40:26.4: 14.09 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:22.01 +41:40:26.4: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461300.8725,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.05 20:50:51.21 +42:25:34.6
83.11678 -1.11123 galactic Cyg Second-epoch detections are separated by 1.9" 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 | 20:50:51.21 +42:25:34.6 (user input) | T | P | (position from user input) J-Ks=0.459+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:51.21 +42:25:34.6: 14.11 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:51.21 +42:25:34.6: 14.30 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:41:04.28 +42:41:02.7
82.19346 0.45689 galactic Cyg Second-epoch detections are separated by 1.6" and 5.4 pix
The object was found in VSX 3" Gaia DR3 2066540801716328832
Type: ROT
# Max. Min./Amp. JD0 Period
14.500 G 14.540 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:04.28 +42:41:02.7: 14.09 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:04.28 +42:41:02.7: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066540801716328832,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066540801716328832 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:51:39.83 +40:52:41.3
82.01832 -2.21309 galactic Cyg Second-epoch detections are separated by 2.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:51:39.83 +40:52:41.3 (user input) | T | P | (position from user input) J-Ks=1.738+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:39.83 +40:52:41.3: 14.08 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:39.83 +40:52:41.3: 14.20 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.05 20:18:26.77 +45:24:20.3
82.01688 5.34438 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:26.77 +45:24:20.3 (user input) | T | P | (position from user input) J-Ks=1.213+/-0.030 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:18:26.77 +45:24:20.3: 14.05 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:18:26.77 +45:24:20.3: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461300.8725,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.11 20:43:55.84 +42:11:44.3
82.13392 -0.25957 galactic Cyg Second-epoch detections are separated by 2.5" 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 | 20:43:55.84 +42:11:44.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.366+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:55.84 +42:11:44.3: 14.06 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:55.84 +42:11:44.3: 14.15 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461300.8725,13.11,0.05,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 20260917.3725 13.11CV 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 09 17.3725 2461300.8725 13.04 20:44:24.85 +42:29:04.4
82.41598 -0.15048 galactic Cyg Second-epoch detections are separated by 1.8" 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 | ATO J311.1032+42.4846 | 20:44:24.85 +42:29:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.368+/-0.034 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:24.85 +42:29:04.4: 14.08 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:24.85 +42:29:04.4: 14.13 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.1032+42.4846,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1032+42.4846 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.14 20:47:40.50 +41:05:32.6
81.70799 -1.49451 galactic Cyg Second-epoch detections are separated by 0.7" and 5.8 pix
The object was found in VSX 1" Gaia DR3 2065408339103558528
Type: ROT
# Max. Min./Amp. JD0 Period
13.840 G 13.860 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:40.50 +41:05:32.6: 14.10 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:40.50 +41:05:32.6: 14.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065408339103558528,2461300.8725,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065408339103558528 20260917.3725 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.06 20:15:48.73 +46:33:24.4
82.72605 6.36262 galactic Cyg Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9531+46.5569 | 20:15:48.73 +46:33:24.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.555+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:15:48.73 +46:33:24.4: 14.07 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:15:48.73 +46:33:24.4: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 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 J303.9531+46.5569,2461300.8725,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.9531+46.5569 20260917.3725 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.02 20:51:09.00 +42:28:31.3
83.18945 -1.12222 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 J312.7901+42.4747 | 20:51:09.00 +42:28:31.3 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.530+/-0.042 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:09.00 +42:28:31.3: 14.08 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:09.00 +42:28:31.3: 14.23 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7901+42.4747,2461300.8725,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.7901+42.4747 20260917.3725 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.92 20:55:43.79 +41:47:35.7
83.21081 -2.21112 galactic Cyg Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:43.79 +41:47:35.7 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.056 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:55:43.79 +41:47:35.7: 14.07 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:55:43.79 +41:47:35.7: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.92,0.05,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 20260917.3725 12.92CV 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 09 17.3725 2461300.8725 12.96 20:45:36.47 +42:13:42.1
82.35258 -0.48252 galactic Cyg Second-epoch detections are separated by 1.9" 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 J311.3951+42.2364 | 20:45:36.47 +42:13:42.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.437+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:36.47 +42:13:42.1: 14.04 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:36.47 +42:13:42.1: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.3951+42.2364,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.3951+42.2364 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.99 20:47:24.57 +42:53:04.9
83.07219 -0.33077 galactic Cyg Second-epoch detections are separated by 0.4" 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 J311.8509+42.8872 | 20:47:24.57 +42:53:04.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.617+/-0.034 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:24.57 +42:53:04.9: 14.03 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:24.57 +42:53:04.9: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.8509+42.8872,2461300.8725,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.8509+42.8872 20260917.3725 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.07 20:50:40.96 +41:38:00.9
82.48428 -1.59033 galactic Cyg Second-epoch detections are separated by 1.5" 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 | 20:50:40.96 +41:38:00.9 (user input) | T | P | (position from user input) J-Ks=1.079+/-0.026 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:40.96 +41:38:00.9: 14.06 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:40.96 +41:38:00.9: 14.34 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461300.8725,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.05 20:49:06.85 +41:49:21.7
82.44531 -1.24408 galactic Cyg Second-epoch detections are separated by 2.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.2806+41.8254 | 20:49:06.85 +41:49:21.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.512+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:06.85 +41:49:21.7: 14.06 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:06.85 +41:49:21.7: 14.22 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.2806+41.8254,2461300.8725,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.2806+41.8254 20260917.3725 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.01 20:48:57.73 +41:55:54.9
82.51217 -1.15318 galactic Cyg Second-epoch detections are separated by 2.1" 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 J312.2406+41.9319 | 20:48:57.73 +41:55:54.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.591+/-9.995 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:57.73 +41:55:54.9: 14.14 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:57.73 +41:55:54.9: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.2406+41.9319,2461300.8725,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.2406+41.9319 20260917.3725 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.97 20:48:16.50 +42:38:47.2
82.98678 -0.60409 galactic Cyg Second-epoch detections are separated by 0.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:16.50 +42:38:47.2 (user input) | T | P | (position from user input) J-Ks=1.198+/-0.032 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:16.50 +42:38:47.2: 14.04 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:16.50 +42:38:47.2: 14.20 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461300.8725,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:41:24.25 +42:18:49.5
81.93859 0.18129 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 | target | 20:41:24.25 +42:18:49.5 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.545+/-0.034 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:24.25 +42:18:49.5: 14.03 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:24.25 +42:18:49.5: 14.15 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.08 20:46:23.97 +42:06:23.3
82.34896 -0.67321 galactic Cyg Second-epoch detections are separated by 2.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.5992+42.1096 | 20:46:23.97 +42:06:23.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.459+/-0.037 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:23.97 +42:06:23.3: 14.06 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:23.97 +42:06:23.3: 14.20 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.5992+42.1096,2461300.8725,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.5992+42.1096 20260917.3725 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:48:25.24 +40:51:06.1
81.60930 -1.75530 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:48:25.24 +40:51:06.1 (user input) | T | P | (position from user input) J-Ks=0.518+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:25.24 +40:51:06.1: 14.05 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:25.24 +40:51:06.1: 14.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:48:40.13 +41:50:15.6
82.40458 -1.17027 galactic Cyg Second-epoch detections are separated by 1.1" 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 J312.1667+41.8376 | 20:48:40.13 +41:50:15.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.410+/-0.045 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:40.13 +41:50:15.6: 14.07 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:40.13 +41:50:15.6: 14.11 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.1667+41.8376,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.1667+41.8376 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.05 20:43:46.66 +42:54:51.7
82.68070 0.20774 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 | 20:43:46.66 +42:54:51.7 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:46.66 +42:54:51.7: 14.07 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:46.66 +42:54:51.7: 14.29 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.09 20:48:58.68 +42:34:19.3
83.01057 -0.75141 galactic Cyg Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.2444+42.5722 | 20:48:58.68 +42:34:19.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.156+/-0.033 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:58.68 +42:34:19.3: 14.03 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:58.68 +42:34:19.3: 14.38 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.2444+42.5722,2461300.8725,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.2444+42.5722 20260917.3725 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:50:59.21 +42:44:17.0
83.37308 -0.93195 galactic Cyg Second-epoch detections are separated by 4.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.7464+42.7383 | 20:50:59.14 +42:44:17.9 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.852+/-0.028 (Very red!)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:59.21 +42:44:17.0: 14.10 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:59.21 +42:44:17.0: 14.38 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7464+42.7383,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.7464+42.7383 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:42:04.38 +42:27:06.1
82.12332 0.16863 galactic Cyg Second-epoch detections are separated by 1.4" and 5.8 pix
The object was found in VSX 1" Gaia DR3 2066528054253449600
Type: ROT
# Max. Min./Amp. JD0 Period
13.850 G 13.890 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:04.38 +42:27:06.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:04.38 +42:27:06.1: 14.20 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066528054253449600,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066528054253449600 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:45:44.41 +42:18:37.9
82.43208 -0.45041 galactic Cyg Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:45:44.41 +42:18:37.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.585+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:44.41 +42:18:37.9: 14.05 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:44.41 +42:18:37.9: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.13 20:41:41.21 +42:49:09.8
82.36964 0.45071 galactic Cyg Second-epoch detections are separated by 2.2" and 6.1 pix
The object was found in VSX21" Gaia DR3 2066548837599450240
Type: L
# Max. Min./Amp. JD0 Period
18.860 G 19.140 G
ATTENTION: measured mag 13.13 is 5.7 mag brighter than the VSX record maximum brightness 18.86 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:41.21 +42:49:09.8: 14.05 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:41.21 +42:49:09.8: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 2066548837599450240,2461300.8725,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066548837599450240 20260917.3725 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.10 20:45:37.47 +41:41:31.9
81.93527 -0.81922 galactic Cyg Second-epoch detections are separated by 3.1" 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 | Large-amplitude variable Gaia DR2 2066199948815646464 | 20:45:37.47 +41:41:31.9 (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=0.555+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:37.47 +41:41:31.9: 14.05 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:37.47 +41:41:31.9: 14.30 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2066199948815646464,2461300.8725,13.10,0.05,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
Large-amplitude variable Gaia DR2 2066199948815646464 20260917.3725 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.16 20:42:44.26 +41:52:40.5
81.74724 -0.28188 galactic Cyg Second-epoch detections are separated by 0.7" and 5.7 pix
The object was found in VSX 0" Gaia DR3 2066356049403303680
Type: ROT
# Max. Min./Amp. JD0 Period
13.830 G 13.890 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:44.26 +41:52:40.5: 14.04 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:44.26 +41:52:40.5: 14.20 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066356049403303680,2461300.8725,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066356049403303680 20260917.3725 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.98 20:53:10.61 +42:23:32.5
83.36445 -1.46302 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 J313.3068+42.3883 | 20:53:10.61 +42:23:32.5 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.402+/-0.043 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:10.61 +42:23:32.5: 14.00 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:10.61 +42:23:32.5: 14.06 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.3068+42.3883,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.3068+42.3883 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.10 20:42:40.42 +42:27:08.9
82.19218 0.08182 galactic Cyg Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:40.42 +42:27:08.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:40.42 +42:27:08.9: 14.07 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:40.42 +42:27:08.9: 14.24 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.07 20:41:31.87 +42:30:25.9
82.10569 0.28154 galactic Cyg Second-epoch detections are separated by 0.4" and 5.8 pix
The object was found in VSX 1" Gaia DR3 2066526404985922816
Type: ROT
# Max. Min./Amp. JD0 Period
13.880 G 13.900 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:31.87 +42:30:25.9: 14.00 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:31.87 +42:30:25.9: 14.25 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066526404985922816,2461300.8725,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066526404985922816 20260917.3725 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.93 20:36:47.07 +43:29:11.2
82.35476 1.56611 galactic Cyg Second-epoch detections are separated by 1.4" and 5.8 pix
The object was found in VSX 1" ZTF J203647.02+432910.8
Type: EA
# Max. Min./Amp. JD0 Period
13.521 r Y 0.354 r 2458632.97250 2.293334400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:36:47.07 +43:29:11.2: 14.02 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:36:47.07 +43:29:11.2: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203647.02+432910.8,2461300.8725,12.93,0.05,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
ZTF J203647.02+432910.8 20260917.3725 12.93CV 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 09 17.3725 2461300.8725 13.09 20:49:37.78 +41:08:54.5
81.98365 -1.74498 galactic Cyg Second-epoch detections are separated by 2.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:37.78 +41:08:54.5 (user input) | T | P | (position from user input) J-Ks=0.518+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:37.78 +41:08:54.5: 14.04 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:37.78 +41:08:54.5: 14.41 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.02 20:41:43.19 +43:03:05.0
82.55640 0.58849 galactic Cyg Second-epoch detections are separated by 0.5" 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 | target | 20:41:43.19 +43:03:05.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.456+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:43.19 +43:03:05.0: 14.02 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:43.19 +43:03:05.0: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 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,2461300.8725,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:47:06.59 +42:38:55.8
82.85401 -0.43591 galactic Cyg Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:47:06.59 +42:38:55.8 (user input) | T | P | (position from user input) J-Ks=1.583+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:06.59 +42:38:55.8: 14.04 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:06.59 +42:38:55.8: 14.39 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.99 20:45:00.48 +41:37:55.1
81.81644 -0.76663 galactic Cyg Second-epoch detections are separated by 2.0" and 5.3 pix
The object was found in VSX 1" ZTF J204500.52+413753.7
Type: BY
# Max. Min./Amp. JD0 Period
13.912 r Y 0.056 r 2458277.95920 1.976052400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:00.48 +41:37:55.1: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:00.48 +41:37:55.1: 13.92 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204500.52+413753.7,2461300.8725,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204500.52+413753.7 20260917.3725 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.91 20:50:35.07 +40:46:12.4
81.80498 -2.12415 galactic Cyg Second-epoch detections are separated by 1.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:35.07 +40:46:12.4 (user input) | T | P | (position from user input) J-Ks=1.374+/-0.025 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:35.07 +40:46:12.4: 14.06 +/- 0.07 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:35.07 +40:46:12.4: 13.99 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461300.8725,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.10 20:40:18.24 +43:16:36.7
82.57638 0.93068 galactic Cyg Second-epoch detections are separated by 1.7" 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 | 20:40:18.24 +43:16:36.7 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.539+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:18.24 +43:16:36.7: 14.01 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:18.24 +43:16:36.7: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461300.8725,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:49:51.50 +41:48:17.7
82.51924 -1.36274 galactic Cyg Second-epoch detections are separated by 1.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.4644+41.8050 | 20:49:51.50 +41:48:17.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.461+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:51.50 +41:48:17.7: 14.00 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:51.50 +41:48:17.7: 14.04 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.4644+41.8050,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.4644+41.8050 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:46:10.36 +43:04:35.2
83.08002 -0.03433 galactic Cyg Second-epoch detections are separated by 2.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.5505+43.0758 | 20:46:10.36 +43:04:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.545+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:10.36 +43:04:35.2: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:10.36 +43:04:35.2: 14.41 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.5505+43.0758,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.5505+43.0758 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:47:42.36 +42:15:51.3
82.62361 -0.76289 galactic Cyg Second-epoch detections are separated by 1.5" 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 J311.9244+42.2709 | 20:47:42.36 +42:15:51.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.469+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:42.36 +42:15:51.3: 13.99 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:42.36 +42:15:51.3: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 J311.9244+42.2709,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.9244+42.2709 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:51:43.40 +41:15:39.2
82.32068 -1.97788 galactic Cyg Second-epoch detections are separated by 3.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:51:43.40 +41:15:39.2 (user input) | T | P | (position from user input) J-Ks=0.486+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:43.40 +41:15:39.2: 14.01 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:43.40 +41:15:39.2: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.07 20:42:12.27 +41:52:14.3
81.68035 -0.20819 galactic Cyg Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:12.27 +41:52:14.3 (user input) | T | P | (position from user input) J-Ks=1.149+/-0.031 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:12.27 +41:52:14.3: 14.00 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:12.27 +41:52:14.3: 14.12 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.98 20:50:28.78 +41:56:06.7
82.69337 -1.36962 galactic Cyg Second-epoch detections are separated by 1.4" and 5.6 pix
The object was found in VSX19" ZTF J205030.49+415603.7
Type: SR
# Max. Min./Amp. JD0 Period
15.422 r Y 0.395 r 2458350.95670 226.875349000000 C
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:28.78 +41:56:06.7: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:28.78 +41:56:06.7: 14.02 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205030.49+415603.7,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205030.49+415603.7 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:49:35.86 +42:22:16.8
82.92724 -0.96680 galactic Cyg Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:35.86 +42:22:16.8 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:35.86 +42:22:16.8: 14.00 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:35.86 +42:22:16.8: 14.05 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:48:36.18 +41:52:31.9
82.42625 -1.13689 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 | ATO J312.1506+41.8753 | 20:48:36.18 +41:52:31.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.407+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:36.18 +41:52:31.9: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:36.18 +41:52:31.9: 14.05 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.1506+41.8753,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.1506+41.8753 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.93 20:41:13.45 +44:38:12.3
83.75348 1.63201 galactic Cyg Second-epoch detections are separated by 1.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:13.45 +44:38:12.3 (user input) | T | P | (position from user input) J-Ks=0.543+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:13.45 +44:38:12.3: 13.99 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:13.45 +44:38:12.3: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461300.8725,12.93,0.05,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
target 20260917.3725 12.93CV 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 09 17.3725 2461300.8725 13.06 20:45:42.96 +42:00:25.1
82.19200 -0.63625 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:45:42.96 +42:00:25.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.497+/-0.056 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:42.96 +42:00:25.1: 14.00 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:42.96 +42:00:25.1: 14.15 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.93 20:50:48.69 +41:48:13.7
82.63107 -1.50077 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 J312.7030+41.8037 | 20:50:48.69 +41:48:13.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.415+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:48.69 +41:48:13.7: 13.97 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:48.69 +41:48:13.7: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7030+41.8037,2461300.8725,12.93,0.05,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 J312.7030+41.8037 20260917.3725 12.93CV 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 09 17.3725 2461300.8725 12.98 20:51:14.23 +42:16:58.7
83.05126 -1.25707 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 | target | 20:51:14.23 +42:16:58.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:14.23 +42:16:58.7: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:14.23 +42:16:58.7: 14.05 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:41:29.08 +42:32:38.2
82.12944 0.31087 galactic Cyg Second-epoch detections are separated by 1.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:29.08 +42:32:38.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.987+/-0.029 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:29.08 +42:32:38.2: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:29.08 +42:32:38.2: 14.40 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.93 20:41:18.00 +42:10:57.5
81.82324 0.11606 galactic Cyg Second-epoch detections are separated by 1.8" and 6.0 pix
The object was found in VSX14" Gaia DR3 2066424592785196416
Type: L
# Max. Min./Amp. JD0 Period
17.980 G 18.220 G
ATTENTION: measured mag 12.93 is 5.1 mag brighter than the VSX record maximum brightness 17.98 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:18.00 +42:10:57.5: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:18.00 +42:10:57.5: 14.10 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066424592785196416,2461300.8725,12.93,0.05,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
Gaia DR3 2066424592785196416 20260917.3725 12.93CV 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 09 17.3725 2461300.8725 12.88 20:40:57.66 +42:37:51.9
82.13914 0.44044 galactic Cyg Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J310.2342+42.6164 | 20:40:59.37 +42:37:15.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7.5: 2010ApJ...720..679B [BKH2010] J204059.4+423715 J-Ks=0.390+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:57.66 +42:37:51.9: 13.96 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:57.66 +42:37:51.9: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.2342+42.6164,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J310.2342+42.6164 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.06 20:42:57.95 +43:34:25.0
83.10746 0.73154 galactic Cyg Second-epoch detections are separated by 1.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:57.95 +43:34:25.0 (user input) | T | P | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.428+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:57.95 +43:34:25.0: 13.97 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:57.95 +43:34:25.0: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461300.8725,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:52:50.35 +40:47:52.5
82.09853 -2.43542 galactic Cyg Second-epoch detections are separated by 0.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:52:50.35 +40:47:52.5 (user input) | T | P | (position from user input) J-Ks=1.011+/-0.026 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:50.35 +40:47:52.5: 13.95 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:50.35 +40:47:52.5: 14.27 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:42:13.97 +43:07:33.8
82.67288 0.56056 galactic Cyg Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:13.97 +43:07:33.8 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.573+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:13.97 +43:07:33.8: 13.95 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:13.97 +43:07:33.8: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 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,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.01 20:45:30.80 +42:09:03.0
82.28104 -0.51716 galactic Cyg Second-epoch detections are separated by 1.2" 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 | 20:45:30.80 +42:09:03.0 (user input) | T | P | (position from user input) J-Ks=0.538+/-0.035 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:30.80 +42:09:03.0: 13.97 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:30.80 +42:09:03.0: 14.11 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8725,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.87 20:53:37.73 +41:50:07.6
82.99077 -1.88452 galactic Cyg Second-epoch detections are separated by 2.1" 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 | ATO J313.4070+41.8354 | 20:53:37.73 +41:50:07.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.528+/-0.040 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:37.73 +41:50:07.6: 13.95 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:37.73 +41:50:07.6: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 J313.4070+41.8354,2461300.8725,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.4070+41.8354 20260917.3725 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.03 20:51:51.20 +41:31:29.8
82.53980 -1.82834 galactic Cyg Second-epoch detections are separated by 2.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:51:51.20 +41:31:29.8 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:51.20 +41:31:29.8: 13.95 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:51.20 +41:31:29.8: 14.20 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.06 20:47:00.83 +41:57:50.4
82.30925 -0.85135 galactic Cyg Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:47:00.83 +41:57:50.4 (user input) | T | P | (position from user input) J-Ks=0.610+/-0.034 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:00.83 +41:57:50.4: 13.96 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:00.83 +41:57:50.4: 14.20 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461300.8725,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:41:04.52 +42:38:07.3
82.15541 0.42645 galactic Cyg Second-epoch detections are separated by 1.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J310.2687+42.6354 | 20:41:04.52 +42:38:07.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.399+/-0.040 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:04.52 +42:38:07.3: 13.95 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:04.52 +42:38:07.3: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.2687+42.6354,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J310.2687+42.6354 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.02 20:44:14.98 +42:07:12.8
82.11139 -0.35271 galactic Cyg Second-epoch detections are separated by 0.3" and 5.7 pix
The object was found in VSX 1" Gaia DR3 2066271936765350912
Type: ROT
# Max. Min./Amp. JD0 Period
13.980 G 14.000 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:14.98 +42:07:12.8: 13.91 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:14.98 +42:07:12.8: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 2066271936765350912,2461300.8725,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066271936765350912 20260917.3725 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.81 20:52:12.43 +42:00:58.9
82.96044 -1.56555 galactic Cyg Second-epoch detections are separated by 0.4" 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 | 20:52:12.43 +42:00:58.9 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:12.43 +42:00:58.9: 13.96 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:12.43 +42:00:58.9: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.81CV 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 09 17.3725 2461300.8725 13.02 20:54:35.22 +42:34:50.3
83.67588 -1.54124 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 J313.6466+42.5807 | 20:54:35.22 +42:34:50.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.564+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:35.22 +42:34:50.3: 13.96 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:35.22 +42:34:50.3: 14.24 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.6466+42.5807,2461300.8725,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.6466+42.5807 20260917.3725 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:44:19.10 +41:55:48.8
81.97029 -0.48059 galactic Cyg Second-epoch detections are separated by 0.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:19.10 +41:55:48.8 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.485+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:19.10 +41:55:48.8: 13.96 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:19.10 +41:55:48.8: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.98 20:47:26.96 +42:43:10.6
82.94827 -0.44009 galactic Cyg Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:47:26.96 +42:43:10.6 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.517+/-0.038 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:26.96 +42:43:10.6: 13.97 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:26.96 +42:43:10.6: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.02 20:44:31.32 +41:39:26.4
81.77988 -0.67973 galactic Cyg Second-epoch detections are separated by 0.9" 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 | ATO J311.1323+41.6603 | 20:44:31.32 +41:39:26.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.463+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:31.32 +41:39:26.4: 13.92 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:31.32 +41:39:26.4: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 J311.1323+41.6603,2461300.8725,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1323+41.6603 20260917.3725 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.91 20:53:00.18 +42:36:15.5
83.50668 -1.30261 galactic Cyg Second-epoch detections are separated by 0.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:53:00.18 +42:36:15.5 (user input) | T | P | (position from user input) J-Ks=0.680+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:00.18 +42:36:15.5: 13.92 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:00.18 +42:36:15.5: 14.05 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.86 20:48:09.51 +41:43:30.3
82.25718 -1.16729 galactic Cyg Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:09.51 +41:43:30.3 (user input) | T | P | (position from user input) J-Ks=0.471+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:09.51 +41:43:30.3: 13.96 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:09.51 +41:43:30.3: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.97 +/- 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,2461300.8725,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.04 20:40:30.87 +42:46:56.2
82.20848 0.59786 galactic Cyg Second-epoch detections are separated by 1.9" and 5.5 pix
The object was found in VSX 1" Gaia DR3 2069547553701483136
Type: ROT
# Max. Min./Amp. JD0 Period
13.710 G 13.750 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:30.87 +42:46:56.2: 13.94 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:30.87 +42:46:56.2: 14.22 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.02 +/- 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 2069547553701483136,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2069547553701483136 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.00 20:45:22.25 +42:29:22.1
82.52950 -0.28555 galactic Cyg Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.3543+42.4913 | 20:45:22.25 +42:29:22.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.564+/-0.034 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:22.25 +42:29:22.1: 13.95 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:22.25 +42:29:22.1: 13.88 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.3543+42.4913,2461300.8725,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.3543+42.4913 20260917.3725 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:39:24.63 +44:43:29.3
83.62623 1.94107 galactic Cyg Second-epoch detections are separated by 5.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:39:24.63 +44:43:29.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:24.63 +44:43:29.3: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:24.63 +44:43:29.3: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:51:33.96 +41:04:35.6
82.15963 -2.07248 galactic Cyg Second-epoch detections are separated by 0.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:51:33.96 +41:04:35.6 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:33.96 +41:04:35.6: 13.93 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:33.96 +41:04:35.6: 14.07 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:51:11.95 +42:42:18.7
83.37254 -0.98295 galactic Cyg Second-epoch detections are separated by 1.9" 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 | 20:51:11.95 +42:42:18.7 (user input) | T | P | (position from user input) J-Ks=0.290+/-0.038 (F)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:11.95 +42:42:18.7: 13.89 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:11.95 +42:42:18.7: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.01 20:41:10.32 +44:09:31.8
83.37002 1.34644 galactic Cyg Second-epoch detections are separated by 1.7" 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 | ATO J310.2864+44.1597 | 20:41:10.32 +44:09:31.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.391+/-0.037 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:10.32 +44:09:31.8: 13.89 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:10.32 +44:09:31.8: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.2864+44.1597,2461300.8725,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J310.2864+44.1597 20260917.3725 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:49:46.03 +42:08:00.9
82.76298 -1.14155 galactic Cyg Second-epoch detections are separated by 2.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.4445+42.1390 | 20:49:46.03 +42:08:00.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.429+/-0.034 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:46.03 +42:08:00.9: 13.93 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:46.03 +42:08:00.9: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 J312.4445+42.1390,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.4445+42.1390 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.89 20:53:29.11 +42:10:19.8
83.23201 -1.64798 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 J313.3766+42.1633 | 20:53:29.11 +42:10:19.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.409+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:29.11 +42:10:19.8: 13.92 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:29.11 +42:10:19.8: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.3766+42.1633,2461300.8725,12.89,0.05,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 J313.3766+42.1633 20260917.3725 12.89CV 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 09 17.3725 2461300.8725 13.04 20:46:54.24 +41:21:48.9
81.82834 -1.21152 galactic Cyg Second-epoch detections are separated by 0.9" and 5.7 pix
The object was found in VSX23" ZTF J204656.06+412139.2
Type: EA
# Max. Min./Amp. JD0 Period
16.929 r Y 0.240 r 2458219.00880 2.085322800000
ATTENTION: measured mag 13.04 is 3.6 mag brighter than the VSX record maximum brightness 16.69 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:54.24 +41:21:48.9: 13.91 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:54.24 +41:21:48.9: 14.15 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J204656.06+412139.2,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204656.06+412139.2 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.85 20:44:38.55 +42:21:56.0
82.34887 -0.25741 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 | Large-amplitude variable Gaia DR2 2066486307171295872 | 20:44:38.55 +42:21:56.0 (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) SpType: F0 (LAMOST DR5) J-Ks=0.637+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:38.55 +42:21:56.0: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:38.55 +42:21:56.0: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2066486307171295872,2461300.8725,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2066486307171295872 20260917.3725 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.99 20:46:14.81 +40:46:43.6
81.29444 -1.48066 galactic Cyg Second-epoch detections are separated by 1.0" and 5.5 pix
The object was found in VSX 9" ZTF J204614.02+404644.7
Type: SR
# Max. Min./Amp. JD0 Period
17.974 r Y 0.883 r 2458450.08590 264.063865000000
ATTENTION: measured mag 12.99 is 4.1 mag brighter than the VSX record maximum brightness 17.09 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:14.81 +40:46:43.6: 13.94 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:14.81 +40:46:43.6: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204614.02+404644.7,2461300.8725,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204614.02+404644.7 20260917.3725 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.06 20:47:08.92 +42:14:20.3
82.53919 -0.69847 galactic Cyg Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.7712+42.2443 | 20:47:08.92 +42:14:20.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.519+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:08.92 +42:14:20.3: 13.93 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:08.92 +42:14:20.3: 14.07 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.7712+42.2443,2461300.8725,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.7712+42.2443 20260917.3725 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.89 20:44:39.24 +42:00:53.6
82.07540 -0.47693 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:44:39.24 +42:00:53.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.482+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:39.24 +42:00:53.6: 13.93 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:39.24 +42:00:53.6: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.89CV 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 09 17.3725 2461300.8725 13.04 20:46:35.79 +42:30:17.7
82.68262 -0.45239 galactic Cyg Second-epoch detections are separated by 2.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2066677892777086592 | 20:46:39.00 +42:30:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.515+/-0.039 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:35.79 +42:30:17.7: 13.93 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:35.79 +42:30:17.7: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 2066677892777086592,2461300.8725,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066677892777086592 20260917.3725 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.98 20:54:30.76 +41:50:56.2
83.10699 -2.00193 galactic Cyg Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:30.76 +41:50:56.2 (user input) | T | P | (position from user input) J-Ks=0.514+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:30.76 +41:50:56.2: 13.93 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:30.76 +41:50:56.2: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.96 +/- 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,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.90 20:52:47.87 +41:59:28.7
83.01135 -1.66595 galactic Cyg Second-epoch detections are separated by 2.2" and 6.0 pix
The object was found in VSX21" ZTF J205246.17+415919.3
Type: SR
# Max. Min./Amp. JD0 Period
20.809 r Y 0.540 r 2458341.42770 123.096409400000
ATTENTION: measured mag 12.90 is 7.4 mag brighter than the VSX record maximum brightness 20.27 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:47.87 +41:59:28.7: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:47.87 +41:59:28.7: 14.09 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205246.17+415919.3,2461300.8725,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205246.17+415919.3 20260917.3725 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:49:31.65 +41:57:07.4
82.59422 -1.22195 galactic Cyg Second-epoch detections are separated by 2.4" and 6.0 pix
The object was found in VSX 0" ZTF J204931.68+415707.2
Type: SR
# Max. Min./Amp. JD0 Period
13.197 r Y 0.084 r 2458318.68600 114.015698300000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:31.65 +41:57:07.4: 13.92 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:31.65 +41:57:07.4: 14.01 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204931.68+415707.2,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204931.68+415707.2 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:38:29.33 +42:32:11.1
81.78659 0.74335 galactic Cyg Second-epoch detections are separated by 1.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:38:29.33 +42:32:11.1 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.387+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:38:29.33 +42:32:11.1: 13.88 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:38:29.33 +42:32:11.1: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.06 20:46:34.17 +42:50:10.4
82.93795 -0.24120 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:34.17 +42:50:10.4 (user input) | T | P | (position from user input) J-Ks=1.789+/-0.029 (Very red!)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:34.17 +42:50:10.4: 13.93 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:34.17 +42:50:10.4: 14.28 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461300.8725,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.98 20:52:59.23 +40:57:24.1
82.23858 -2.35533 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 | target | 20:52:59.23 +40:57:24.1 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:59.23 +40:57:24.1: 13.94 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:59.23 +40:57:24.1: 13.99 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.82 20:50:57.06 +41:54:30.1
82.72834 -1.45438 galactic Cyg Second-epoch detections are separated by 0.7" 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 J312.7376+41.9083 | 20:50:57.06 +41:54:30.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.583+/-0.034 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:57.06 +41:54:30.1: 13.91 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:57.06 +41:54:30.1: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7376+41.9083,2461300.8725,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.7376+41.9083 20260917.3725 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.92 20:48:57.94 +41:03:20.8
81.83270 -1.70656 galactic Cyg Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:57.94 +41:03:20.8 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:57.94 +41:03:20.8: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:57.94 +41:03:20.8: 14.04 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.92,0.05,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 20260917.3725 12.92CV 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 09 17.3725 2461300.8725 12.95 20:52:05.62 +42:28:27.9
83.29966 -1.25691 galactic Cyg Second-epoch detections are separated by 2.8" 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 | Large-amplitude variable Gaia DR2 2065973934750283904 | 20:52:05.62 +42:28:27.9 (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=0.384+/-0.038 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:05.62 +42:28:27.9: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:05.62 +42:28:27.9: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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
Large-amplitude variable Gaia DR2 2065973934750283904,2461300.8725,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2065973934750283904 20260917.3725 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.87 20:43:52.11 +42:24:05.9
82.28850 -0.12292 galactic Cyg Second-epoch detections are separated by 0.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:43:52.11 +42:24:05.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.425+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:52.11 +42:24:05.9: 13.88 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:52.11 +42:24:05.9: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461300.8725,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:46:57.10 +40:59:06.4
81.53883 -1.45555 galactic Cyg Second-epoch detections are separated by 1.4" and 5.5 pix
The object was found in VSX 0" Gaia DR3 2065413286906031488
Type: RS
# Max. Min./Amp. JD0 Period
13.630 G 13.680 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:57.10 +40:59:06.4: 13.89 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:57.10 +40:59:06.4: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065413286906031488,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065413286906031488 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.97 20:51:38.47 +42:34:34.4
83.32487 -1.12776 galactic Cyg Second-epoch detections are separated by 0.5" 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 | 20:51:38.47 +42:34:34.4 (user input) | T | P | (position from user input) J-Ks=1.315+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:38.47 +42:34:34.4: 13.93 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:38.47 +42:34:34.4: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:39:21.47 +42:59:33.2
82.24576 0.89403 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was found in VSX16" ZTF J203921.65+425917.5
Type: EA
# Max. Min./Amp. JD0 Period
17.139 r Y 0.164 r 2458372.80360 1.362462000000
ATTENTION: measured mag 12.94 is 4.0 mag brighter than the VSX record maximum brightness 16.97 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:21.47 +42:59:33.2: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:21.47 +42:59:33.2: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203921.65+425917.5,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J203921.65+425917.5 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.93 20:42:18.15 +42:50:32.1
82.45709 0.37578 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 | target | 20:42:18.15 +42:50:32.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.364+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:18.15 +42:50:32.1: 13.89 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:18.15 +42:50:32.1: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461300.8725,12.93,0.05,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
target 20260917.3725 12.93CV 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 09 17.3725 2461300.8725 12.90 20:41:33.41 +42:27:22.5
82.06839 0.24652 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 20:41:33.41 +42:27:22.5 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:33.41 +42:27:22.5: 13.87 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:33.41 +42:27:22.5: 14.16 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.83 20:51:51.65 +41:52:04.8
82.80506 -1.61065 galactic Cyg Second-epoch detections are separated by 1.8" 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 | 20:51:51.65 +41:52:04.8 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:51.65 +41:52:04.8: 13.88 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:51.65 +41:52:04.8: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461300.8725,12.83,0.05,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
target 20260917.3725 12.83CV 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 09 17.3725 2461300.8725 12.98 20:42:46.37 +41:56:29.2
81.80128 -0.24784 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 | target | 20:42:46.37 +41:56:29.2 (user input) | T | P | (position from user input) J-Ks=0.531+/-0.035 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:46.37 +41:56:29.2: 13.88 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:46.37 +41:56:29.2: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.95 20:47:27.94 +42:57:38.2
83.13774 -0.29112 galactic Cyg Second-epoch detections are separated by 1.4" 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 | 20:47:27.94 +42:57:38.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:27.94 +42:57:38.2: 13.91 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:27.94 +42:57:38.2: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.92 +/- 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,2461300.8725,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:49:44.05 +41:51:30.8
82.54613 -1.31088 galactic Cyg Second-epoch detections are separated by 1.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:44.05 +41:51:30.8 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:44.05 +41:51:30.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:44.05 +41:51:30.8: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:40:15.41 +43:47:43.5
82.98174 1.25428 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:40:15.41 +43:47:43.5 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.400+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:15.41 +43:47:43.5: 13.87 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:15.41 +43:47:43.5: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.81 20:43:45.89 +42:26:49.2
82.31227 -0.07981 galactic Cyg Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J310.9407+42.4453 | 20:43:45.89 +42:26:49.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.779+/-0.044 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:45.89 +42:26:49.2: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:45.89 +42:26:49.2: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 J310.9407+42.4453,2461300.8725,12.81,0.05,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 J310.9407+42.4453 20260917.3725 12.81CV 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 09 17.3725 2461300.8725 12.95 20:54:02.41 +42:06:27.6
83.24865 -1.76826 galactic Cyg Second-epoch detections are separated by 2.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:02.41 +42:06:27.6 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:02.41 +42:06:27.6: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:02.41 +42:06:27.6: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461300.8725,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.93 20:45:12.88 +43:03:09.7
82.95232 0.08763 galactic Cyg Second-epoch detections are separated by 1.8" 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 | ATO J311.3039+43.0525 | 20:45:12.88 +43:03:09.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.631+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:12.88 +43:03:09.7: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:12.88 +43:03:09.7: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 J311.3039+43.0525,2461300.8725,12.93,0.05,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 J311.3039+43.0525 20260917.3725 12.93CV 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 09 17.3725 2461300.8725 12.96 20:38:52.74 +42:28:01.6
81.77521 0.64413 galactic Cyg Second-epoch detections are separated by 0.5" 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 J309.7197+42.4670 | 20:38:52.74 +42:28:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.720+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:38:52.74 +42:28:01.6: 13.89 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:38:52.74 +42:28:01.6: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J309.7197+42.4670,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.7197+42.4670 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.85 20:41:21.08 +43:27:15.4
82.83323 0.88882 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 20:41:21.08 +43:27:15.4 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:21.08 +43:27:15.4: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:21.08 +43:27:15.4: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461300.8725,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.99 20:42:22.22 +44:28:53.4
83.75640 1.37554 galactic Cyg Second-epoch detections are separated by 0.4" and 5.6 pix
The object was found in VSX 1" Gaia DR3 2070079786050755072
Type: ROT
# Max. Min./Amp. JD0 Period
13.730 G 13.770 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:22.22 +44:28:53.4: 13.83 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:22.22 +44:28:53.4: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2070079786050755072,2461300.8725,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2070079786050755072 20260917.3725 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:44:46.86 +41:53:09.3
81.98902 -0.57557 galactic Cyg Second-epoch detections are separated by 0.5" 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 | ATO J311.1829+41.8823 | 20:44:46.86 +41:53:09.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.405+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:46.86 +41:53:09.3: 13.83 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:46.86 +41:53:09.3: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.1829+41.8823,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1829+41.8823 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.86 20:49:30.68 +41:11:17.7
82.00039 -1.70258 galactic Cyg Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:30.68 +41:11:17.7 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:30.68 +41:11:17.7: 13.86 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:30.68 +41:11:17.7: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461300.8725,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.90 20:53:43.21 +41:52:38.1
83.03376 -1.87072 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 | 20:53:43.21 +41:52:38.1 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.045 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:43.21 +41:52:38.1: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:43.21 +41:52:38.1: 13.99 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461300.8725,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.89 20:48:33.09 +41:42:36.7
82.29180 -1.23363 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 20:48:33.09 +41:42:36.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:33.09 +41:42:36.7: 13.84 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:33.09 +41:42:36.7: 14.01 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.89CV 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 09 17.3725 2461300.8725 12.72 20:52:31.41 +41:34:07.8
82.65369 -1.89683 galactic Cyg Second-epoch detections are separated by 1.4" and 5.9 pix
The object was found in VSX 1" ZTF J205231.41+413407.1
Type: BY
# Max. Min./Amp. JD0 Period
13.351 r Y 0.098 r 2458229.96630 4.174051100000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:31.41 +41:34:07.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:31.41 +41:34:07.8: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205231.41+413407.1,2461300.8725,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205231.41+413407.1 20260917.3725 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:35:49.43 +43:55:31.6
82.60111 1.96889 galactic Cyg Second-epoch detections are separated by 0.3" and 5.7 pix
The object was found in VSX25" ZTF J203549.12+435507.2
Type: RS
# Max. Min./Amp. JD0 Period
13.592 r Y 0.064 r 2458640.97150 2.431416600000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:35:49.43 +43:55:31.6: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:35:49.43 +43:55:31.6: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203549.12+435507.2,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J203549.12+435507.2 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:54:29.35 +42:05:12.8
83.28634 -1.84540 galactic Cyg Second-epoch detections are separated by 2.2" 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 | target | 20:54:29.35 +42:05:12.8 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:29.35 +42:05:12.8: 13.86 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:29.35 +42:05:12.8: 14.08 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.92 20:40:03.89 +42:25:12.7
81.87131 0.44207 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 | Large-amplitude variable Gaia DR2 2066446346793739392 | 20:40:03.89 +42:25:12.7 (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=0.422+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:03.89 +42:25:12.7: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:03.89 +42:25:12.7: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2066446346793739392,2461300.8725,12.92,0.05,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
Large-amplitude variable Gaia DR2 2066446346793739392 20260917.3725 12.92CV 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 09 17.3725 2461300.8725 12.98 20:46:07.80 +43:06:31.8
83.10044 -0.00801 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was found in VSX 1" Gaia DR3 2066887457120494592
Type: ROT
# Max. Min./Amp. JD0 Period
13.720 G 13.740 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:07.80 +43:06:31.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:07.80 +43:06:31.8: 14.18 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066887457120494592,2461300.8725,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066887457120494592 20260917.3725 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.86 20:51:22.15 +41:47:39.9
82.68995 -1.58695 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 20:51:22.15 +41:47:39.9 (user input) | T | P | (position from user input) J-Ks=0.772+/-0.028 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:22.15 +41:47:39.9: 13.86 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:22.15 +41:47:39.9: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.85 20:51:15.82 +41:26:13.7
82.40170 -1.79913 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:51:15.82 +41:26:13.7 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:15.82 +41:26:13.7: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:15.82 +41:26:13.7: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.96 20:48:26.11 +42:07:56.8
82.60612 -0.95079 galactic Cyg Second-epoch detections are separated by 1.2" 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 | 20:48:26.11 +42:07:56.8 (user input) | T | P | (position from user input) J-Ks=0.827+/-0.036 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:26.11 +42:07:56.8: 13.83 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:26.11 +42:07:56.8: 14.01 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:54:12.96 +41:57:07.9
83.15052 -1.89324 galactic Cyg Second-epoch detections are separated by 0.7" 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 J313.5606+41.9511 | 20:54:12.96 +41:57:07.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.633+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:12.96 +41:57:07.9: 13.86 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:12.96 +41:57:07.9: 14.04 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.5606+41.9511,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.5606+41.9511 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.87 20:51:12.93 +40:44:12.7
81.85524 -2.23756 galactic Cyg Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:51:12.93 +40:44:12.7 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:12.93 +40:44:12.7: 13.83 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:12.93 +40:44:12.7: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:40:53.22 +43:18:20.9
82.66419 0.86447 galactic Cyg Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:53.22 +43:18:20.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.449+/-0.027 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:53.22 +43:18:20.9: 13.83 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:53.22 +43:18:20.9: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.86 20:44:27.01 +41:46:44.9
81.86705 -0.59360 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 | target | 20:44:27.01 +41:46:44.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:27.01 +41:46:44.9: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:27.01 +41:46:44.9: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461300.8725,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.81 20:53:24.99 +42:30:38.5
83.48364 -1.42106 galactic Cyg Second-epoch detections are separated by 0.3" 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 | 20:53:24.99 +42:30:38.5 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.038 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:24.99 +42:30:38.5: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:24.99 +42:30:38.5: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461300.8725,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.81CV 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 09 17.3725 2461300.8725 12.90 20:50:43.19 +42:15:26.8
82.97069 -1.19943 galactic Cyg Second-epoch detections are separated by 1.2" 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 | ATO J312.6800+42.2576 | 20:50:43.19 +42:15:26.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=12.095+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:43.19 +42:15:26.8: 13.86 +/- 0.06 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:43.19 +42:15:26.8: 14.03 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J312.6800+42.2576,2461300.8725,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.6800+42.2576 20260917.3725 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.90 20:53:10.15 +40:52:40.3
82.19999 -2.43222 galactic Cyg Second-epoch detections are separated by 1.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:53:10.15 +40:52:40.3 (user input) | T | P | (position from user input) J-Ks=0.475+/-0.027 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:10.15 +40:52:40.3: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:10.15 +40:52:40.3: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.94 20:47:43.59 +41:31:42.6
82.05351 -1.22811 galactic Cyg Second-epoch detections are separated by 2.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:47:43.59 +41:31:42.6 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:43.59 +41:31:42.6: 13.78 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:43.59 +41:31:42.6: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.83 20:43:56.21 +43:55:58.2
83.49822 0.81589 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 | target | 20:43:56.21 +43:55:58.2 (user input) | T | P | (position from user input) J-Ks=0.503+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:56.21 +43:55:58.2: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:56.21 +43:55:58.2: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.83,0.05,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
target 20260917.3725 12.83CV 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 09 17.3725 2461300.8725 12.88 20:46:59.57 +42:40:45.8
82.86433 -0.39999 galactic Cyg Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:59.57 +42:40:45.8 (user input) | T | P | (position from user input) SpType: A0III (LAMOST DR5) J-Ks=0.668+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:59.57 +42:40:45.8: 13.79 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:59.57 +42:40:45.8: 13.98 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.80 20:47:44.97 +41:43:20.9
82.20715 -1.10959 galactic Cyg Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.9373+41.7223 | 20:47:44.97 +41:43:20.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.966+/-0.026 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:44.97 +41:43:20.9: 13.81 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:44.97 +41:43:20.9: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.9373+41.7223,2461300.8725,12.80,0.05,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 J311.9373+41.7223 20260917.3725 12.80CV 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 09 17.3725 2461300.8725 12.87 20:46:12.54 +42:59:23.5
83.01657 -0.09362 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.5443+42.9827 | 20:46:12.54 +42:59:23.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.428+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:12.54 +42:59:23.5: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:12.54 +42:59:23.5: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.5443+42.9827,2461300.8725,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.5443+42.9827 20260917.3725 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:45:49.52 +42:03:56.3
82.25052 -0.61552 galactic Cyg Second-epoch detections are separated by 1.7" 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 | 20:45:49.52 +42:03:56.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.389+/-0.034 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:49.52 +42:03:56.3: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:49.52 +42:03:56.3: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:41:19.77 +42:24:44.6
82.00801 0.25271 galactic Cyg Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:19.77 +42:24:44.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.363+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:19.77 +42:24:44.6: 13.80 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:19.77 +42:24:44.6: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.87 20:42:00.63 +43:18:43.4
82.79458 0.70695 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 | target | 20:42:00.63 +43:18:43.4 (user input) | T | P | (position from user input) J-Ks=0.819+/-0.030 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:00.63 +43:18:43.4: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:00.63 +43:18:43.4: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461300.8725,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.85 20:39:49.84 +44:27:58.5
83.46666 1.72426 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 2070258383671441920 | 20:39:49.86 +44:27:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.738+/-0.043 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:49.84 +44:27:58.5: 13.82 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:49.84 +44:27:58.5: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 2070258383671441920,2461300.8725,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2070258383671441920 20260917.3725 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 13.29 20:40:41.72 +42:13:22.5
81.78645 0.22923 galactic Cyg Second-epoch detections are separated by 1.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:41.72 +42:13:22.5 (user input) | T | P | (position from user input) J-Ks=0.497+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:41.72 +42:13:22.5: 14.64 +/- 0.09 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:41.72 +42:13:22.5: 14.68 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,13.29,0.05,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 20260917.3725 13.29CV 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 09 17.3725 2461300.8725 12.81 20:50:44.32 +41:29:51.2
82.38581 -1.68480 galactic Cyg Second-epoch detections are separated by 1.6" 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 | target | 20:50:44.32 +41:29:51.2 (user input) | T | P | (position from user input) J-Ks=12.617+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:44.32 +41:29:51.2: 13.80 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:44.32 +41:29:51.2: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.81CV 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 09 17.3725 2461300.8725 12.89 20:50:55.68 +41:40:20.2
82.54330 -1.60114 galactic Cyg Second-epoch detections are separated by 1.1" and 5.6 pix
The object was found in VSX15" Gaia DR3 2065824259436448128
Type: ROT
# Max. Min./Amp. JD0 Period
16.030 G 16.070 G K
ATTENTION: measured mag 12.89 is 3.1 mag brighter than the VSX record maximum brightness 16.03 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:55.68 +41:40:20.2: 13.80 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:55.68 +41:40:20.2: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065824259436448128,2461300.8725,12.89,0.05,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 2065824259436448128 20260917.3725 12.89CV 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 09 17.3725 2461300.8725 12.89 20:46:47.72 +41:26:14.2
81.87305 -1.14948 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 | target | 20:46:47.72 +41:26:14.2 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.271+/-0.030 (F)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:47.72 +41:26:14.2: 13.80 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:47.72 +41:26:14.2: 14.05 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.89CV 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 09 17.3725 2461300.8725 12.80 20:41:21.37 +44:41:30.9
83.81147 1.64729 galactic Cyg Second-epoch detections are separated by 1.3" 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 J310.3548+44.6951 | 20:41:21.37 +44:41:30.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.306+/-0.035 (F)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:21.37 +44:41:30.9: 13.75 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:21.37 +44:41:30.9: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.3548+44.6951,2461300.8725,12.80,0.05,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 J310.3548+44.6951 20260917.3725 12.80CV 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 09 17.3725 2461300.8725 12.88 20:43:41.55 +41:54:54.4
81.88628 -0.39859 galactic Cyg Second-epoch detections are separated by 1.6" 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 | 20:43:41.55 +41:54:54.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.657+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:41.55 +41:54:54.4: 13.81 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:41.55 +41:54:54.4: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.85 20:51:46.20 +42:27:04.2
83.24365 -1.22578 galactic Cyg Second-epoch detections are separated by 0.4" and 5.7 pix
The object was found in VSX 6" Gaia DR3 2065880957299120896
Type: L
# Max. Min./Amp. JD0 Period
18.540 G 18.740 G
ATTENTION: measured mag 12.85 is 5.7 mag brighter than the VSX record maximum brightness 18.54 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:46.20 +42:27:04.2: 13.79 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:46.20 +42:27:04.2: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065880957299120896,2461300.8725,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065880957299120896 20260917.3725 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.91 20:55:11.39 +41:51:15.9
83.19251 -2.09482 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:11.39 +41:51:15.9 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:55:11.39 +41:51:15.9: 13.78 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:55:11.39 +41:51:15.9: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.84 20:39:42.16 +44:42:30.0
83.64478 1.88987 galactic Cyg Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:39:42.16 +44:42:30.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=11.699+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:42.16 +44:42:30.0: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:42.16 +44:42:30.0: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461300.8725,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.76 20:46:49.32 +41:46:10.9
82.13540 -0.94523 galactic Cyg Second-epoch detections are separated by 1.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:49.32 +41:46:10.9 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:49.32 +41:46:10.9: 13.78 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:49.32 +41:46:10.9: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.76,0.05,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 20260917.3725 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.76 20:52:24.43 +41:47:43.8
82.81423 -1.73527 galactic Cyg Second-epoch detections are separated by 1.7" and 6.0 pix
The object was found in VSX 1" ASASSN-V J205224.36+414743.7
Type: ROT
# Max. Min./Amp. JD0 Period
14.320 g Y 0.160 g 2458753.71200 2.424100000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:24.43 +41:47:43.8: 13.79 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:24.43 +41:47:43.8: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205224.36+414743.7,2461300.8725,12.76,0.05,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
ASASSN-V J205224.36+414743.7 20260917.3725 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.87 20:44:32.93 +42:35:57.7
82.52137 -0.09865 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 | target | 20:44:32.93 +42:35:57.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.579+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:32.93 +42:35:57.7: 13.80 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:32.93 +42:35:57.7: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.87 20:46:52.82 +42:08:59.4
82.43858 -0.71560 galactic Cyg Second-epoch detections are separated by 2.1" and 6.1 pix
The object was found in VSX 0" Gaia DR3 2066283722155903360
Type: ROT
# Max. Min./Amp. JD0 Period
13.600 G 13.630 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:52.82 +42:08:59.4: 13.80 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:52.82 +42:08:59.4: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066283722155903360,2461300.8725,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066283722155903360 20260917.3725 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:51:34.31 +41:25:45.5
82.43244 -1.84866 galactic Cyg Second-epoch detections are separated by 1.0" 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 | 20:51:34.31 +41:25:45.5 (user input) | T | P | (position from user input) J-Ks=0.584+/-0.026 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:34.31 +41:25:45.5: 13.78 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:34.31 +41:25:45.5: 13.89 +/- 0.07 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
target,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.83 20:42:44.73 +43:05:28.7
82.70318 0.46546 galactic Cyg Second-epoch detections are separated by 0.9" 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 | ATO J310.6979+43.0832 | 20:42:44.73 +43:05:28.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.510+/-0.044 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:44.73 +43:05:28.7: 13.79 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:44.73 +43:05:28.7: 13.79 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.6979+43.0832,2461300.8725,12.83,0.05,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 J310.6979+43.0832 20260917.3725 12.83CV 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 09 17.3725 2461300.8725 12.88 20:45:56.57 +42:06:28.5
82.29717 -0.60617 galactic Cyg Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.4850+42.1113 | 20:45:56.57 +42:06:28.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.367+/-0.037 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:56.57 +42:06:28.5: 13.76 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:56.57 +42:06:28.5: 13.94 +/- 0.07 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
ATO J311.4850+42.1113,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.4850+42.1113 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.84 20:49:40.33 +41:56:56.1
82.60881 -1.24477 galactic Cyg Second-epoch detections are separated by 2.0" and 5.4 pix
The object was found in VSX21" WISE J204939.9+415716
Type: EA
# Max. Min./Amp. JD0 Period
15.629 r Y 2.200 r 2458361.79590 4.876399800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:40.33 +41:56:56.1: 13.78 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:40.33 +41:56:56.1: 13.96 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J204939.9+415716,2461300.8725,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J204939.9+415716 20260917.3725 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.89 20:40:20.93 +44:51:23.4
83.83224 1.88940 galactic Cyg Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:20.93 +44:51:23.4 (user input) | T | P | (position from user input) J-Ks=0.947+/-0.031 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:20.93 +44:51:23.4: 13.74 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:20.93 +44:51:23.4: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.89CV 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 09 17.3725 2461300.8725 12.89 20:38:27.91 +44:52:05.0
83.63817 2.16131 galactic Cyg Second-epoch detections are separated by 1.2" and 5.5 pix
The object was found in VSX 1" ASASSN-V J203827.99+445205.5
Type: SRS
# Max. Min./Amp. JD0 Period
14.150 V 14.290 V 2457550.05300 24.122000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:38:27.91 +44:52:05.0: 13.70 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:38:27.91 +44:52:05.0: 14.08 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J203827.99+445205.5,2461300.8725,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203827.99+445205.5 20260917.3725 12.89CV 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 09 17.3725 2461300.8725 12.92 20:50:58.70 +40:53:04.7
81.94085 -2.10898 galactic Cyg Second-epoch detections are separated by 2.5" 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 | ATO J312.7450+40.8845 | 20:50:58.81 +40:53:04.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M7/9: 1970A&A.....8..315A [A70] 78-0-153 J-Ks=1.851+/-0.029 (Very red!)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:58.70 +40:53:04.7: 13.83 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:58.70 +40:53:04.7: 14.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.7450+40.8845,2461300.8725,12.92,0.05,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
ATO J312.7450+40.8845 20260917.3725 12.92CV 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 09 17.3725 2461300.8725 12.67 20:52:37.80 +42:26:09.8
83.33338 -1.35751 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 J313.1576+42.4363 | 20:52:37.85 +42:26:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.859+/-0.036 (Very red!)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:37.80 +42:26:09.8: 13.77 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:37.80 +42:26:09.8: 14.04 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J313.1576+42.4363,2461300.8725,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J313.1576+42.4363 20260917.3725 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.84 20:39:36.02 +43:14:22.3
82.46860 1.00939 galactic Cyg Second-epoch detections are separated by 0.5" 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 | target | 20:39:36.02 +43:14:22.3 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:36.02 +43:14:22.3: 13.77 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:36.02 +43:14:22.3: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461300.8725,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:44:04.68 +41:55:28.6
81.93816 -0.44900 galactic Cyg Second-epoch detections are separated by 1.6" and 6.0 pix
The object was found in VSX19" Gaia DR3 2066262419117804800
Type: RS
# Max. Min./Amp. JD0 Period
15.170 G 15.360 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:04.68 +41:55:28.6: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:04.68 +41:55:28.6: 13.90 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066262419117804800,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066262419117804800 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.83 20:44:50.38 +42:16:37.9
82.30229 -0.34088 galactic Cyg Second-epoch detections are separated by 0.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:50.38 +42:16:37.9 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.379+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:50.38 +42:16:37.9: 13.74 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:50.38 +42:16:37.9: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461300.8725,12.83,0.05,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
target 20260917.3725 12.83CV 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 09 17.3725 2461300.8725 12.80 20:40:49.30 +42:15:44.3
81.83190 0.23486 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 | 20:40:49.30 +42:15:44.3 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:49.30 +42:15:44.3: 13.76 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:49.30 +42:15:44.3: 13.90 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.80CV 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 09 17.3725 2461300.8725 12.82 20:43:07.37 +42:09:28.8
82.01175 -0.16527 galactic Cyg Second-epoch detections are separated by 2.4" 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 | target | 20:43:07.37 +42:09:28.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.041+/-0.031 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:07.37 +42:09:28.8: 13.76 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:07.37 +42:09:28.8: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.86 20:44:48.18 +42:08:14.9
82.18862 -0.42242 galactic Cyg Second-epoch detections are separated by 1.5" and 5.5 pix
The object was found in VSX 0" Gaia DR3 2066294648552395904
Type: ROT
# Max. Min./Amp. JD0 Period
13.600 G 13.630 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:48.18 +42:08:14.9: 13.78 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:48.18 +42:08:14.9: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066294648552395904,2461300.8725,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066294648552395904 20260917.3725 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.61 20:53:03.69 +41:49:10.1
82.91071 -1.81365 galactic Cyg Second-epoch detections are separated by 1.5" and 5.6 pix
The object was found in VSX 4" Gaia DR3 2065794714358904320
Type: E
# Max. Min./Amp. JD0 Period
18.570 G 19.430 G 1.818090000000
NOTE: the measured mag 12.61 is inconsistent with the record above (maximum 18.57), and the brighter VSX variable Gaia DR3 2065794710061673600 at 24" may be the actual counterpart.
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:03.69 +41:49:10.1: 13.73 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:03.69 +41:49:10.1: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065794714358904320,2461300.8725,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065794714358904320 20260917.3725 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.76 20:52:20.78 +41:13:49.7
82.37200 -2.08746 galactic Cyg Second-epoch detections are separated by 0.7" 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 J313.0855+41.2310 | 20:52:20.78 +41:13:49.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:20.78 +41:13:49.7: 13.75 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:20.78 +41:13:49.7: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.0855+41.2310,2461300.8725,12.76,0.05,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 J313.0855+41.2310 20260917.3725 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.77 20:46:35.38 +41:45:42.9
82.10222 -0.91631 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 | target | 20:46:35.38 +41:45:42.9 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:35.38 +41:45:42.9: 13.74 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:35.38 +41:45:42.9: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.82 20:44:33.34 +42:17:07.7
82.27614 -0.29458 galactic Cyg Second-epoch detections are separated by 1.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:33.34 +42:17:07.7 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.399+/-0.038 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:33.34 +42:17:07.7: 13.73 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:33.34 +42:17:07.7: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:42:36.34 +42:07:28.5
81.92629 -0.11046 galactic Cyg Second-epoch detections are separated by 0.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:42:36.34 +42:07:28.5 (user input) | T | P | (position from user input) SpType: F2.5: 2010ApJ...720..679B [BKH2010] J204236.3+420729 J-Ks=0.398+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:36.34 +42:07:28.5: 13.77 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:36.34 +42:07:28.5: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.73 20:51:39.99 +41:32:07.9
82.52566 -1.79465 galactic Cyg Second-epoch detections are separated by 0.6" 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 J312.9167+41.5355 | 20:51:39.99 +41:32:07.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.441+/-0.027 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:39.99 +41:32:07.9: 13.74 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:39.99 +41:32:07.9: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.9167+41.5355,2461300.8725,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.9167+41.5355 20260917.3725 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.73 20:53:20.07 +40:55:15.5
82.25316 -2.42859 galactic Cyg Second-epoch detections are separated by 0.7" 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 | 20:53:20.07 +40:55:15.5 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.027 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:20.07 +40:55:15.5: 13.75 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:20.07 +40:55:15.5: 13.69 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.81 20:47:49.80 +41:49:50.9
82.30087 -1.05318 galactic Cyg Second-epoch detections are separated by 1.1" 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 | 20:47:49.80 +41:49:50.9 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:49.80 +41:49:50.9: 13.75 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:49.80 +41:49:50.9: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.81CV 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 09 17.3725 2461300.8725 12.85 20:47:24.60 +42:03:13.0
82.42522 -0.85247 galactic Cyg Second-epoch detections are separated by 0.4" 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 | 20:47:24.60 +42:03:13.0 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:24.60 +42:03:13.0: 13.75 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:24.60 +42:03:13.0: 14.01 +/- 0.08 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
target,2461300.8725,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.88 20:48:20.10 +41:34:04.5
82.15578 -1.29183 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 20:48:20.10 +41:34:04.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:20.10 +41:34:04.5: 13.72 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:20.10 +41:34:04.5: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:52:19.42 +40:55:30.8
82.13419 -2.27910 galactic Cyg Second-epoch detections are separated by 0.7" and 5.6 pix
The object was found in VSX25" Gaia DR3 2065552267750559488
Type: RRC
# Max. Min./Amp. JD0 Period
20.540 G 21.060 G 0.313896000000
ATTENTION: measured mag 12.79 is 7.8 mag brighter than the VSX record maximum brightness 20.54 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:19.42 +40:55:30.8: 13.76 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:19.42 +40:55:30.8: 13.82 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065552267750559488,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065552267750559488 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.82 20:46:35.19 +41:48:06.3
82.13292 -0.89093 galactic Cyg Second-epoch detections are separated by 0.5" 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 | ATO J311.6496+41.8012 | 20:46:35.19 +41:48:06.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.363+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:35.19 +41:48:06.3: 13.71 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:35.19 +41:48:06.3: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.6496+41.8012,2461300.8725,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.6496+41.8012 20260917.3725 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.82 20:47:16.87 +42:08:43.6
82.48173 -0.77624 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 20:47:16.87 +42:08:43.6 (user input) | T | P | (position from user input) J-Ks=1.263+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:16.87 +42:08:43.6: 13.72 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:16.87 +42:08:43.6: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.84 20:40:11.15 +43:06:56.4
82.43560 0.84925 galactic Cyg Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:11.15 +43:06:56.4 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:11.15 +43:06:56.4: 13.73 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:11.15 +43:06:56.4: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 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,2461300.8725,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.71 20:52:09.04 +41:23:26.5
82.47192 -1.95689 galactic Cyg Second-epoch detections are separated by 0.5" 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 | ATO J313.0430+41.3899 | 20:52:09.04 +41:23:26.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.525+/-0.035 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:09.04 +41:23:26.5: 13.71 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:09.04 +41:23:26.5: 13.79 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.0430+41.3899,2461300.8725,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.0430+41.3899 20260917.3725 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:46:07.15 +42:55:13.0
82.95197 -0.12426 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 | 20:46:07.15 +42:55:13.0 (user input) | T | P | (position from user input) J-Ks=0.610+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:07.15 +42:55:13.0: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:07.15 +42:55:13.0: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:46:58.63 +41:45:50.4
82.14909 -0.97135 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 | target | 20:46:58.63 +41:45:50.4 (user input) | T | P | (position from user input) J-Ks=0.409+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:58.63 +41:45:50.4: 13.71 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:58.63 +41:45:50.4: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.74 20:44:11.30 +42:12:06.7
82.16838 -0.29316 galactic Cyg Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:11.30 +42:12:06.7 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.029 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:11.30 +42:12:06.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:11.30 +42:12:06.7: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461300.8725,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.74 20:49:07.30 +41:22:59.3
82.10525 -1.52271 galactic Cyg Second-epoch detections are separated by 1.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:07.30 +41:22:59.3 (user input) | T | P | (position from user input) J-Ks=1.336+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:07.30 +41:22:59.3: 13.73 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:07.30 +41:22:59.3: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.62 20:50:54.46 +41:52:21.5
82.69563 -1.47086 galactic Cyg Second-epoch detections are separated by 6.4" and 4.9 pix
The object was found in VSX15" Gaia DR3 2065831066961660928
Type: L
# Max. Min./Amp. JD0 Period
18.430 G 18.690 G
ATTENTION: measured mag 12.62 is 5.8 mag brighter than the VSX record maximum brightness 18.43 - 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:54.46 +41:52:21.5: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:54.46 +41:52:21.5: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 2065831066961660928,2461300.8725,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065831066961660928 20260917.3725 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.76 20:41:24.50 +42:17:34.0
81.92251 0.16781 galactic Cyg Second-epoch detections are separated by 0.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:24.50 +42:17:34.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.396+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:24.50 +42:17:34.0: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:24.50 +42:17:34.0: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.76,0.05,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 20260917.3725 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.69 20:14:23.88 +46:37:02.0
82.64302 6.59901 galactic Cyg Second-epoch detections are separated by 1.9" 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 | ATO J303.5916+46.6065 | 20:14:23.88 +46:37:02.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.854+/-0.034 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:14:23.88 +46:37:02.0: 13.69 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:14:23.88 +46:37:02.0: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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 J303.5916+46.6065,2461300.8725,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.5916+46.6065 20260917.3725 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.75 20:54:56.46 +41:51:14.0
83.16220 -2.05975 galactic Cyg Second-epoch detections are separated by 2.0" 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 | 20:54:56.46 +41:51:14.0 (user input) | T | P | (position from user input) J-Ks=0.553+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:56.46 +41:51:14.0: 13.68 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:56.46 +41:51:14.0: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 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,2461300.8725,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.76 20:48:31.23 +41:23:11.9
82.03683 -1.43299 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 | target | 20:48:31.23 +41:23:11.9 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:31.23 +41:23:11.9: 13.70 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:31.23 +41:23:11.9: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.76,0.05,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 20260917.3725 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.70 20:47:32.84 +41:59:43.0
82.39582 -0.90894 galactic Cyg Second-epoch detections are separated by 1.2" 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 | ATO J311.8912+41.9956 | 20:47:32.84 +41:59:43.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.144+/-0.028 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:32.84 +41:59:43.0: 13.70 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:32.84 +41:59:43.0: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 J311.8912+41.9956,2461300.8725,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.8912+41.9956 20260917.3725 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.75 20:50:12.98 +40:51:23.3
81.82760 -2.01552 galactic Cyg Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:50:12.98 +40:51:23.3 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.031 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:12.98 +40:51:23.3: 13.69 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:12.98 +40:51:23.3: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.68 20:41:35.52 +42:36:03.5
82.18658 0.33029 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 | target | 20:41:35.52 +42:36:03.5 (user input) | T | P | (position from user input) SpType: K2 2010ApJ...720..679B [BKH2010] J204135.5+423603 J-Ks=0.591+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:35.52 +42:36:03.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:35.52 +42:36:03.5: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:46:10.51 +41:33:21.8
81.89311 -0.98458 galactic Cyg Second-epoch detections are separated by 0.9" 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 | 20:46:10.51 +41:33:21.8 (user input) | T | P | (position from user input) J-Ks=1.059+/-0.026 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:10.51 +41:33:21.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:10.51 +41:33:21.8: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.74 20:42:49.44 +42:23:11.6
82.15742 0.01933 galactic Cyg Second-epoch detections are separated by 0.0" 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 | 20:42:49.44 +42:23:11.6 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.339+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:42:49.44 +42:23:11.6: 13.69 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:42:49.44 +42:23:11.6: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 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,2461300.8725,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.73 20:40:46.38 +42:33:32.9
82.06108 0.42373 galactic Cyg Second-epoch detections are separated by 0.9" and 5.8 pix
The object was found in VSX 1" Gaia DR3 2066538362174900992
Type: ROT
# Max. Min./Amp. JD0 Period
13.430 G 13.460 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:46.38 +42:33:32.9: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:46.38 +42:33:32.9: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2066538362174900992,2461300.8725,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2066538362174900992 20260917.3725 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.66 20:52:52.53 +40:56:00.1
82.20713 -2.35406 galactic Cyg Second-epoch detections are separated by 1.0" 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 | 20:52:52.53 +40:56:00.1 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:52.53 +40:56:00.1: 13.68 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:52.53 +40:56:00.1: 13.65 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:46:17.49 +43:09:28.2
83.15711 -0.00040 galactic Cyg Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:46:17.49 +43:09:28.2 (user input) | T | P | (position from user input) J-Ks=1.288+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:17.49 +43:09:28.2: 13.69 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:17.49 +43:09:28.2: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.73 20:52:38.81 +41:37:21.4
82.70982 -1.88018 galactic Cyg Second-epoch detections are separated by 0.4" 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 | ATO J313.1617+41.6226 | 20:52:38.81 +41:37:21.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.281+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:38.81 +41:37:21.4: 13.72 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:38.81 +41:37:21.4: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.1617+41.6226,2461300.8725,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.1617+41.6226 20260917.3725 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.69 20:52:54.02 +42:18:36.1
83.26847 -1.47653 galactic Cyg Second-epoch detections are separated by 0.5" 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 | 20:52:54.02 +42:18:36.1 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.031 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:54.02 +42:18:36.1: 13.66 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:54.02 +42:18:36.1: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:38:16.84 +45:09:49.9
83.85388 2.36650 galactic Cyg Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J309.5698+45.1637 | 20:38:16.84 +45:09:49.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.491+/-0.050 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:38:16.84 +45:09:49.9: 13.68 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:38:16.84 +45:09:49.9: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J309.5698+45.1637,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.5698+45.1637 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.76 20:48:53.16 +41:45:58.7
82.37472 -1.24669 galactic Cyg Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.2214+41.7664 | 20:48:53.16 +41:45:58.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.481+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:53.16 +41:45:58.7: 13.65 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:53.16 +41:45:58.7: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 J312.2214+41.7664,2461300.8725,12.76,0.05,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 J312.2214+41.7664 20260917.3725 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:46:05.41 +42:04:52.9
82.29349 -0.64410 galactic Cyg Second-epoch detections are separated by 0.5" 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 | ATO J311.5090+42.0732 | 20:46:05.41 +42:04:52.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.420+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:05.41 +42:04:52.9: 13.68 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:05.41 +42:04:52.9: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 J311.5090+42.0732,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.5090+42.0732 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.77 20:50:57.25 +42:45:47.6
83.38869 -0.91132 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 | target | 20:50:57.25 +42:45:47.6 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:57.25 +42:45:47.6: 13.67 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:57.25 +42:45:47.6: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 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,2461300.8725,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.79 20:48:44.85 +41:51:16.3
82.42691 -1.17101 galactic Cyg Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:44.85 +41:51:16.3 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.026 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:44.85 +41:51:16.3: 13.68 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:44.85 +41:51:16.3: 13.81 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461300.8725,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.77 20:48:11.25 +40:49:58.8
81.56700 -1.73280 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 | target | 20:48:11.25 +40:49:58.8 (user input) | T | P | (position from user input) J-Ks=0.497+/-0.030 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:11.25 +40:49:58.8: 13.68 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:11.25 +40:49:58.8: 13.77 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.68 20:51:17.62 +40:59:40.5
82.06366 -2.08505 galactic Cyg Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:51:17.62 +40:59:40.5 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:17.62 +40:59:40.5: 13.67 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:17.62 +40:59:40.5: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.68 20:41:38.46 +42:24:32.1
82.04057 0.20520 galactic Cyg Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:41:38.46 +42:24:32.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.377+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:38.46 +42:24:32.1: 13.68 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:38.46 +42:24:32.1: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.71 20:40:39.90 +44:46:33.9
83.80284 1.79587 galactic Cyg Second-epoch detections are separated by 2.0" and 5.3 pix
The object was found in VSX 4" ASASSN-V J204040.16+444630.7
Type: SRS
# Max. Min./Amp. JD0 Period
15.140 g Y 0.350 g 2459357.91200 20.025000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:39.90 +44:46:33.9: 13.67 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:39.90 +44:46:33.9: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J204040.16+444630.7,2461300.8725,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J204040.16+444630.7 20260917.3725 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.75 20:54:22.30 +41:59:16.1
83.19642 -1.89248 galactic Cyg Second-epoch detections are separated by 1.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:22.30 +41:59:16.1 (user input) | T | P | (position from user input) J-Ks=1.348+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:54:22.30 +41:59:16.1: 13.71 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:54:22.30 +41:59:16.1: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.78 20:46:00.97 +42:22:19.4
82.51198 -0.45186 galactic Cyg Second-epoch detections are separated by 0.2" 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 | 20:46:00.97 +42:22:19.4 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:46:00.97 +42:22:19.4: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:46:00.97 +42:22:19.4: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.81 20:40:11.55 +43:12:14.3
82.50626 0.90222 galactic Cyg Second-epoch detections are separated by 1.2" 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 | target | 20:40:11.55 +43:12:14.3 (user input) | T | P | (position from user input) J-Ks=0.322+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:11.55 +43:12:14.3: 13.66 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:11.55 +43:12:14.3: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.81CV 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 09 17.3725 2461300.8725 12.71 20:51:48.65 +41:17:21.2
82.35301 -1.97249 galactic Cyg Second-epoch detections are separated by 1.4" 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 | 20:51:48.65 +41:17:21.2 (user input) | T | P | (position from user input) J-Ks=0.666+/-0.026 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:51:48.65 +41:17:21.2: 13.67 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:51:48.65 +41:17:21.2: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.73 20:50:02.38 +42:32:06.5
83.10567 -0.92618 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 | ATO J312.4990+42.5271 | 20:50:02.38 +42:32:06.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.520+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:02.38 +42:32:06.5: 13.68 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:02.38 +42:32:06.5: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.4990+42.5271,2461300.8725,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.4990+42.5271 20260917.3725 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.64 20:45:41.34 +42:11:18.0
82.33065 -0.51923 galactic Cyg Second-epoch detections are separated by 1.4" 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 | ATO J311.4226+42.1874 | 20:45:41.34 +42:11:18.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:41.34 +42:11:18.0: 13.64 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:41.34 +42:11:18.0: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.4226+42.1874,2461300.8725,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.4226+42.1874 20260917.3725 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.73 20:50:05.22 +42:03:00.0
82.73588 -1.24040 galactic Cyg Second-epoch detections are separated by 1.9" and 5.8 pix
The object was found in VSX 1" Gaia DR3 2065848315550440320
Type: ROT
# Max. Min./Amp. JD0 Period
13.550 G 13.570 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:50:05.22 +42:03:00.0: 13.64 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:50:05.22 +42:03:00.0: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065848315550440320,2461300.8725,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065848315550440320 20260917.3725 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.77 20:45:43.04 +42:19:20.1
82.43861 -0.43980 galactic Cyg Second-epoch detections are separated by 2.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:45:43.04 +42:19:20.1 (user input) | T | P | (position from user input) J-Ks=0.446+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:43.04 +42:19:20.1: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:43.04 +42:19:20.1: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.64 20:53:37.43 +42:32:29.4
83.53180 -1.43059 galactic Cyg Second-epoch detections are separated by 0.4" 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 | 20:53:37.43 +42:32:29.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:37.43 +42:32:29.4: 13.64 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:37.43 +42:32:29.4: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461300.8725,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.76 20:44:04.70 +42:18:35.7
82.24054 -0.21019 galactic Cyg Second-epoch detections are separated by 1.2" 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 | 20:44:04.70 +42:18:35.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.382+/-0.033 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:04.70 +42:18:35.7: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:04.70 +42:18:35.7: 13.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8725,12.76,0.05,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 20260917.3725 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.65 20:52:14.50 +41:34:58.4
82.63082 -1.84730 galactic Cyg Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:52:14.50 +41:34:58.4 (user input) | T | P | (position from user input) J-Ks=0.485+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:52:14.50 +41:34:58.4: 13.67 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:52:14.50 +41:34:58.4: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.76 20:56:11.88 +42:36:06.1
83.88360 -1.75395 galactic Cyg Second-epoch detections are separated by 1.2" 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 J314.0494+42.6017 | 20:56:11.88 +42:36:06.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.540+/-0.032 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:56:11.88 +42:36:06.1: 13.64 +/- 0.05 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:56:11.88 +42:36:06.1: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.0494+42.6017,2461300.8725,12.76,0.05,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 J314.0494+42.6017 20260917.3725 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.66 20:43:27.31 +42:14:35.9
82.11685 -0.16092 galactic Cyg Second-epoch detections are separated by 0.5" 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 | target | 20:43:27.31 +42:14:35.9 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=0.842+/-0.028 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:27.31 +42:14:35.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:27.31 +42:14:35.9: 13.83 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461300.8725,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.66 20:41:21.77 +44:39:58.7
83.79196 1.63065 galactic Cyg Second-epoch detections are separated by 4.8" and 6.3 pix
The object was found in VSX 7" ZTF J204121.38+443952.6
Type: RS
# Max. Min./Amp. JD0 Period
13.555 r Y 0.080 r 2458370.77530 16.690472800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:41:21.77 +44:39:58.7: 13.59 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:41:21.77 +44:39:58.7: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J204121.38+443952.6,2461300.8725,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J204121.38+443952.6 20260917.3725 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.69 20:47:52.66 +42:21:25.5
82.71577 -0.72923 galactic Cyg Second-epoch detections are separated by 1.8" 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 | ATO J311.9692+42.3569 | 20:47:52.66 +42:21:25.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.589+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:52.66 +42:21:25.5: 13.61 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:52.66 +42:21:25.5: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.9692+42.3569,2461300.8725,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.9692+42.3569 20260917.3725 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.77 20:37:28.44 +43:21:45.0
82.33150 1.39148 galactic Cyg Second-epoch detections are separated by 0.5" 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 | 20:37:28.44 +43:21:45.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.450+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:37:28.44 +43:21:45.0: 13.62 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:37:28.44 +43:21:45.0: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.67 20:47:36.07 +41:57:04.7
82.36788 -0.94434 galactic Cyg Second-epoch detections are separated by 2.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.9001+41.9508 | 20:47:36.07 +41:57:04.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:36.07 +41:57:04.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:36.07 +41:57:04.7: 13.64 +/- 0.05 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
ATO J311.9001+41.9508,2461300.8725,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.9001+41.9508 20260917.3725 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.72 20:43:50.53 +41:58:52.6
81.95547 -0.37947 galactic Cyg Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:43:50.53 +41:58:52.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:43:50.53 +41:58:52.6: 13.62 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:43:50.53 +41:58:52.6: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.66 20:47:33.81 +42:06:42.9
82.48849 -0.83804 galactic Cyg Second-epoch detections are separated by 0.9" 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 J311.8904+42.1116 | 20:47:33.81 +42:06:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.636+/-0.033 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:33.81 +42:06:42.9: 13.64 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:33.81 +42:06:42.9: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.8904+42.1116,2461300.8725,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.8904+42.1116 20260917.3725 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.68 20:48:34.51 +41:28:44.8
82.11511 -1.38268 galactic Cyg Second-epoch detections are separated by 0.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:48:34.51 +41:28:44.8 (user input) | T | P | (position from user input) J-Ks=0.506+/-0.029 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:48:34.51 +41:28:44.8: 13.61 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:48:34.51 +41:28:44.8: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.73 20:53:54.47 +42:24:53.1
83.46826 -1.55214 galactic Cyg Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:53:54.47 +42:24:53.1 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.044 (K)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:53:54.47 +42:24:53.1: 13.61 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:53:54.47 +42:24:53.1: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.56 20:47:47.62 +42:36:22.9
82.89991 -0.56048 galactic Cyg Second-epoch detections are separated by 2.0" 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 | 20:47:47.62 +42:36:22.9 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.035 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:47:47.62 +42:36:22.9: 13.60 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:47:47.62 +42:36:22.9: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8725,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.66 20:45:44.30 +43:09:42.4
83.09720 0.08086 galactic Cyg Second-epoch detections are separated by 1.3" 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 | 20:45:44.30 +43:09:42.4 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.353+/-0.036 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:45:44.30 +43:09:42.4: 13.58 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:45:44.30 +43:09:42.4: 13.65 +/- 0.05 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
target,2461300.8725,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.66 20:44:04.13 +44:00:50.1
83.57659 0.84749 galactic Cyg Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:04.13 +44:00:50.1 (user input) | T | P | (position from user input) SpType: A2V (LAMOST DR5) J-Ks=0.435+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:04.13 +44:00:50.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:04.13 +44:00:50.1: 13.60 +/- 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,2461300.8725,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.69 20:39:03.16 +44:46:47.9
83.63139 2.02505 galactic Cyg Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:39:03.16 +44:46:47.9 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:39:03.16 +44:46:47.9: 13.60 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:39:03.16 +44:46:47.9: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461300.8725,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.60 20:49:43.24 +41:48:30.8
82.50581 -1.34058 galactic Cyg Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:49:43.24 +41:48:30.8 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.028 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:49:43.24 +41:48:30.8: 13.59 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:49:43.24 +41:48:30.8: 13.67 +/- 0.05 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
target,2461300.8725,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.71 20:40:37.73 +42:45:48.6
82.20647 0.56978 galactic Cyg Second-epoch detections are separated by 1.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:40:37.73 +42:45:48.6 (user input) | T | P | (position from user input) J-Ks=1.099+/-0.028 (M)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:40:37.73 +42:45:48.6: 13.59 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:40:37.73 +42:45:48.6: 13.80 +/- 0.05 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,2461300.8725,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3725 2461300.8725 12.70 20:44:17.75 +42:14:55.4
82.21748 -0.27970 galactic Cyg Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:44:17.75 +42:14:55.4 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.358+/-0.030 (G)
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits at 20:44:17.75 +42:14:55.4: 13.57 +/- 0.04 detection
Forced photometry on wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits at 20:44:17.75 +42:14:55.4: 13.64 +/- 0.05 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,2461300.8725,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3725 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461234.79643095 13.07.2026 07:06:41.634 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
First image: 2461234.79643095 13.07.2026 07:06:41.634 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
Last image: 2461300.87275804 17.09.2026 08:56:36.295 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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: 6 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): 30956
Objects passed selection criteria: 30849
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: 19753
Average stars matched: 19220.5 (97.3042 %)
Memory usage VmPeak: 255276 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 17 04:01:25 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461234.79643095 13.07.2026 07:06:41.634 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
First image: 2461234.79643095 13.07.2026 07:06:41.634 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
Last image: 2461300.87275804 17.09.2026 08:56:36.295 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 579
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.16
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 52 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): 205913
Objects passed selection criteria: 205180
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 139037
Average stars matched: 132256 (95.1231 %)
Memory usage VmPeak: 602564 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 17 04:03:03 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
SExtractor catalog cache: saved Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.cat to cache
SExtractor catalog cache: saved Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461300.87216147
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits exists and is non-empty
wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits exists and is non-empty
wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits exists and is non-empty
wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits (1st reference image)
verification OK: wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:24:00.714 +46:00:47.35 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-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits (1st new image)
verification OK: wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
Image size: 941.6'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: 20:24:14.977 +46:00:56.80 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:24:00.714 +46:00:47.35
Second-epoch image center 20:24:14.977 +46:00:56.80
Angular distance between the image centers 0.0414 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits (2nd new image)
verification OK: wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
Image size: 941.6'x626.7' 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: 20:24:15.181 +46:00:22.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:24:00.714 +46:00:47.35
Second-epoch image center 20:24:15.181 +46:00:22.90
Angular distance between the image centers 0.0424 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 20:24:14.977 +46:00:56.80
Second-epoch second image center 20:24:15.181 +46:00:22.90
Angular distance between the image centers 0.00944 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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits &> /tmp/tmp.KrPITWxGhm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits &> /tmp/tmp.pdFfY7rTjK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits &> /tmp/tmp.GVjWk642NU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits &> /tmp/tmp.d0yFePwtl6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits and wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits and wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat
Found non-empty wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits and wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat
The reference image (wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits) and catalog (wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat) found
'wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat' -> 'wcsmag.cat'
Read 34950 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 293.6869 to 318.2780 deg, Dec +40.3373 to +51.2765 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 293.6869 to 318.2780 deg, Dec 40.3373 to 51.2765 deg
Loaded 23388 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): 15752 out of 17614 total matches.
Matched with Tycho-2 17614 out of 34950 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.662450
a=0.000000 b=1.000000 c=22.662450
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34950 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 293.6869 to 318.2780 deg, Dec +40.3373 to +51.2765 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 293.6869 to 318.2780 deg, Dec 40.3373 to 51.2765 deg
Loaded 23388 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): 15752 out of 17614 total matches.
Matched with Tycho-2 17614 out of 34950 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
Forced-photometry filter: calibrated wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits -> calib.txt_param_ref_wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits (aperture=6.5)
Read 32659 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 293.6887 to 318.2868 deg, Dec +40.2710 to +51.2608 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 293.6887 to 318.2868 deg, Dec 40.2710 to 51.2608 deg
Loaded 23539 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): 15620 out of 17285 total matches.
Matched with Tycho-2 17285 out of 32659 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
Forced-photometry filter: calibrated wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits -> calib.txt_param_ref_wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
2.3 pix Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
2.4 pix fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
2.4 pix fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
Limiting magnitude estimates:
15.2 mag. Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
15.1 mag. Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
13.2 mag. fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
13.4 mag. fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.8 (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.KrPITWxGhm (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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.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_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits' -> 'wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
WCS-calibrated image found: wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
Checking if the catalog wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits
WCS catalog name: wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.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=4106, bad_region=0, passed=34950
Got 34950 stars (including 30805 good ones) from the SExtractor catalog wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat
util/solve_plate_with_UCAC5 got 34950 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 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
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 4900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 34950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 34950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 34950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4899 stars left (next iteration limit 5390)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits N_match=4899 sigma_overall_arcsec=0.548 sigma_q1_arcsec=0.481 sigma_q2_arcsec=0.546 sigma_q3_arcsec=0.499 sigma_q4_arcsec=0.586 n_q1=1263 n_q2=1201 n_q3=1132 n_q4=1303 worst_quadrant_to_overall_ratio=1.069
The image catalog is written to wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits -region wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.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.pdFfY7rTjK (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-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.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_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.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-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.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-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits' -> 'wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.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-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
WCS-calibrated image found: wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
Checking if the catalog wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits.wcscat corresponding to the image wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits.wcscat corresponding to the image wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits
WCS catalog name: wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.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=3708, bad_region=0, passed=32659
Got 32659 stars (including 28911 good ones) from the SExtractor catalog wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits.wcscat
util/solve_plate_with_UCAC5 got 32659 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 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 4911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 32659 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 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 32659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 32659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 4911 stars left (next iteration limit 5402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits N_match=4911 sigma_overall_arcsec=0.578 sigma_q1_arcsec=0.478 sigma_q2_arcsec=0.656 sigma_q3_arcsec=0.575 sigma_q4_arcsec=0.630 n_q1=1242 n_q2=1274 n_q3=1090 n_q4=1305 worst_quadrant_to_overall_ratio=1.136
The image catalog is written to wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits -region wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.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.GVjWk642NU (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_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.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_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
Checking if the catalog wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat corresponding to the image wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat corresponding to the image wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
WCS catalog name: wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.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=283, bad_region=0, passed=5847
Got 5847 stars (including 5554 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat
util/solve_plate_with_UCAC5 got 5847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 4843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 5836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 5836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 5836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4852 stars left (next iteration limit 5336)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4852 robust_rms=4.726 arcsec worst_quadrant_rms=32.518 arcsec
SIP_REFIT: SIP order 3 trial: matched=4852 robust_rms=0.395 arcsec worst_quadrant_rms=0.501 arcsec
SIP_REFIT: SIP order 5 trial: matched=4852 robust_rms=0.324 arcsec worst_quadrant_rms=0.383 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4852 robust_rms_before=0.598 arcsec robust_rms_before_corrected=0.393 arcsec robust_rms_after=0.324 arcsec worst_quadrant_rms_before=0.459 worst_quadrant_rms_after=0.383
verification OK: wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
verification OK: wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
Image size: 941.7'x626.7' 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: 20:24:14.989 +46:00:57.06 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5847 stars ###
'wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/correct_sextractor_wcs_catalog_usingxy2sky912746.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.598 -> 0.324 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4852 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4686 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4686 pairs (4852 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4686 robust_rms=4.469 arcsec worst_quadrant_rms=31.454 arcsec
SIP_REFIT: SIP order 3 trial: matched=4686 robust_rms=0.385 arcsec worst_quadrant_rms=0.480 arcsec
SIP_REFIT: SIP order 5 trial: matched=4686 robust_rms=0.315 arcsec worst_quadrant_rms=0.381 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4686 robust_rms_before=0.318 arcsec robust_rms_before_corrected=0.318 arcsec robust_rms_after=0.315 arcsec worst_quadrant_rms_before=0.379 worst_quadrant_rms_after=0.381
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.381 vs 0.379 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: 4686 matched stars entering correct_measured_positions(), 5836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4686 matched stars entering correct_measured_positions(), 5836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
WCS_QUALITY_DIAG: file=fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits N_match=4686 sigma_overall_arcsec=0.328 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.295 sigma_q4_arcsec=0.347 n_q1=822 n_q2=950 n_q3=2104 n_q4=810 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits -region wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.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.d0yFePwtl6 (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_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.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_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
WCS-calibrated image found: wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
Checking if the catalog wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits.wcscat corresponding to the image wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits.wcscat corresponding to the image wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
WCS catalog name: wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.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=294, bad_region=0, passed=6208
Got 6208 stars (including 5903 good ones) from the SExtractor catalog wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits.wcscat
util/solve_plate_with_UCAC5 got 6208 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 4857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 6198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 6199 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 6199 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4862 stars left (next iteration limit 5348)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4862 robust_rms=7.439 arcsec worst_quadrant_rms=8.971 arcsec
SIP_REFIT: SIP order 3 trial: matched=4862 robust_rms=0.390 arcsec worst_quadrant_rms=0.527 arcsec
SIP_REFIT: SIP order 5 trial: matched=4862 robust_rms=0.333 arcsec worst_quadrant_rms=0.421 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4862 robust_rms_before=0.574 arcsec robust_rms_before_corrected=0.374 arcsec robust_rms_after=0.333 arcsec worst_quadrant_rms_before=0.453 worst_quadrant_rms_after=0.421
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.453 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits N_match=4862 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.394 sigma_q2_arcsec=0.445 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.434 n_q1=833 n_q2=952 n_q3=2142 n_q4=935 worst_quadrant_to_overall_ratio=1.182
The image catalog is written to wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits -region wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.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-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits to local_wcs_cache/
'wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits' -> 'local_wcs_cache/wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits'
Saving the final (post-refit) wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits to local_wcs_cache/
'wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits' -> 'local_wcs_cache/wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits'
Saving the final (post-refit) wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits to local_wcs_cache/
'wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits' -> 'local_wcs_cache/wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits'
Saving the final (post-refit) wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits to local_wcs_cache/
'wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits' -> 'local_wcs_cache/wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits sigma_overall=0.548 worst_q_ratio=1.069
ref2=Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits sigma_overall=0.578 worst_q_ratio=1.136
new1=fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits sigma_overall=0.328 worst_q_ratio=1.210
new2=fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits sigma_overall=0.376 worst_q_ratio=1.182
reference average sigma_overall=0.563 worst_q_ratio=1.1025
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090_astrometric_residuals.png (4899 matched stars from wcs_Cyg-03-Q1b1x1_2026-07-13_02-06-41_20.00sec_4.90C_LIGHT_0090.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127_astrometric_residuals.png (4911 matched stars from wcs_Cyg-03-Q1b1x1_2026-07-24_02-44-09_20.00sec_5.00C_LIGHT_0127.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008_astrometric_residuals.png (4686 matched stars from wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009_astrometric_residuals.png (4862 matched stars from wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-55-44_20.00sec_-0.00C_LIGHTs_0008.fits'
Saving fully-calibrated image wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-03-Q1b1x1_035719_TTUQ1b1x1_792545_mkvnnzvi/wcs_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009.fits'
Preparing the HTML report for the field Cyg-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 51925_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 51925_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:38:58.58 +45:05:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02014_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 02014_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:52:37.48 +41:04:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08273_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 08273_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264298_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264298_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264304_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264304_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:49:58.74 +47:16:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264307_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264307_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:20:49.79 +44:51:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264308_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264308_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264310_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264310_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264313_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264313_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264314_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264314_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264317_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264317_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264319_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264319_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264324_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264324_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264325_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264325_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 19:56:12.09 +44:51:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264327_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264327_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:59:31.73 +40:28:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264331_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264331_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:31:23.27 +44:02:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264332_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264332_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 19:53:09.50 +48:56:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264336_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264336_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 19:52:01.21 +50:13:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264339_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264339_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264341_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264341_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 19:43:27.55 +49:48:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264342_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264342_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264344_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264344_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 19:42:24.87 +50:19:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264346_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264346_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264353_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264353_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264715_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264715_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 264930_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264930_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:40:00.88 +43:29:20.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 264941_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 264941_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:41:21.14 +45:13:13.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 265097_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265097_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (43.7") between the two second-epoch detections
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Considering the candidate 265237_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265237_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 21:02:36.47 +41:18:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265280_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265280_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265292_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265292_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:09.20 +40:54:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265294_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265294_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265443_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265443_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:50:14.45 +44:03:47.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265507_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265507_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265512_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265512_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:34:02.45 +45:06:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265524_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265524_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265533_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265533_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:15:20.28 +47:40:35.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 265534_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265534_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:59:20.47 +42:18:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265561_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265561_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265587_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265587_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265593_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265593_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265642_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265642_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:47:13.31 +45:33:36.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265687_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265687_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 19:43:16.94 +41:57:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265771_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265771_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:14.82 +41:10:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265799_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265799_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265825_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265825_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:48:28.21 +42:14:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265839_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265839_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265864_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265864_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 265904_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265904_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:28:33.93 +48:56:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265933_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265933_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:20:00.87 +43:58:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265974_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 265974_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 266118_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 266118_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 266160_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 266160_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:55:04.75 +42:43:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266176_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 266176_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 266186_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 266186_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 266237_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 266237_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:04:36.40 +48:13:10.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266262_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 266262_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 266276_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 266276_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:42:28.74 +45:48:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266281_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 266281_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:32:45.97 +43:10:51.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 83477_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 83477_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 19300_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19300_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 17991_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 17991_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24081_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24081_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 101589_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 101589_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 10935_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 10935_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21922_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21922_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32795_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32795_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 19094_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19094_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33652_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33652_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 124596_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 124596_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 44631_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 44631_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32885_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32885_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 63121_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 63121_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 83845_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 83845_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22710_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22710_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 52963_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 52963_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 42274_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 42274_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 26002_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 26002_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35272_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 35272_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:41:53.23 +42:32:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.370 2066532246141441408 310.47145890275 +42.54726326342 13.8985 13.3593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 25145_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25145_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 42843_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 42843_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 26243_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 26243_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28110_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28110_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28882_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28882_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 126250_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 126250_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 71695_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 71695_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 11869_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 11869_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33020_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33020_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 42730_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 42730_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20102_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20102_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 65749_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 65749_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 44535_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 44535_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33784_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33784_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33832_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33832_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33653_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33653_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20170_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20170_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21422_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21422_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 246205_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 246205_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:38:54.91 +44:54:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35321_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35321_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29701_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29701_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30943_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30943_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35684_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35684_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31472_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31472_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31681_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31681_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33241_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33241_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25457_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25457_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35954_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35954_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 34887_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 34887_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:24.58 +42:22:46.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 19914_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19914_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31098_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31098_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 13731_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 13731_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 26207_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 26207_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32920_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32920_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 74576_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 74576_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23110_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23110_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22350_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22350_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 37826_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 37826_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 24551_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24551_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36872_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36872_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 49084_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 49084_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 19445_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19445_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 150895_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 150895_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 25627_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25627_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23349_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23349_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20415_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20415_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18329_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 18329_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:06.60 +41:28:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35705_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35705_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 38825_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38825_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 05269_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 05269_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:50:28.32 +40:49:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25805_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25805_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36334_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36334_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33444_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33444_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 59244_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 59244_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 123598_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 123598_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:07:14.52 +46:33:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37731_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 37731_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22021_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22021_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 37148_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 37148_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28111_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28111_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23402_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23402_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 06809_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 06809_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 13763_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 13763_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:33.06 +41:12:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33661_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33661_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 71398_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 71398_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 39867_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 39867_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 76634_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 76634_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 34966_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 34966_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 19555_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19555_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 14108_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 14108_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24110_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 24110_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:52:52.49 +41:48:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23058_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23058_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32375_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32375_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 07544_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 07544_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23995_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23995_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22980_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22980_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 43868_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 43868_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 126662_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 126662_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:13:21.25 +46:42:38.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 32858_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32858_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 61271_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 61271_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25727_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25727_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 17637_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 17637_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 40880_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 40880_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21132_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21132_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35510_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35510_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 37294_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 37294_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20103_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20103_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 74433_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 74433_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21721_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21721_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 10324_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 10324_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32696_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32696_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29638_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29638_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24270_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24270_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21534_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21534_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 17925_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 17925_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:47.29 +41:26:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28758_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28758_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28913_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28913_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32373_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32373_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 249871_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 249871_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (34.5") between the two second-epoch detections
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Considering the candidate 33504_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33504_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 45227_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 45227_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33115_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33115_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18602_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 18602_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24936_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24936_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32520_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32520_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25567_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25567_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33909_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33909_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 52202_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 52202_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 38397_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38397_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31602_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31602_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 52746_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 52746_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29278_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29278_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30499_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30499_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30080_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30080_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 119618_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 119618_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24908_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24908_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20183_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20183_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 41552_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 41552_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 66887_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 66887_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 70198_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 70198_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:42:08.86 +44:25:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45760_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 45760_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18105_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 18105_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32497_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32497_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30954_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30954_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36039_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36039_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 37369_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 37369_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 84472_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 84472_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:38:58.47 +45:05:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31473_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31473_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 209030_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 209030_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 34731_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 34731_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 34264_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 34264_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22601_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22601_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 74865_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 74865_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 70290_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 70290_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 15303_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 15303_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:41.13 +41:18:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35476_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35476_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18721_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 18721_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29602_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 29602_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 111839_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 111839_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
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Considering the candidate 59317_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 59317_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 17003_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 17003_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33753_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33753_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23217_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23217_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 45707_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 45707_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 38342_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38342_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33207_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 33207_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 23901_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23901_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 15369_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 15369_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 44899_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 44899_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25748_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25748_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 48628_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 48628_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20883_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20883_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 99104_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 99104_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (34.2") between the two second-epoch detections
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Considering the candidate 36699_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36699_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 08790_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 08790_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:45:45.17 +41:02:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72076_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 72076_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33563_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33563_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 170431_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 170431_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (33.7") between the two second-epoch detections
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Considering the candidate 71463_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 71463_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 12358_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 12358_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30536_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30536_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 38646_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38646_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 70234_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 70234_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 13975_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 13975_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22733_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22733_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22285_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22285_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32202_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32202_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 11394_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 11394_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33211_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33211_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25027_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25027_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21996_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 21996_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:06.51 +41:41:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38907_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38907_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 48591_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 48591_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33863_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33863_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 26116_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 26116_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28094_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28094_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35185_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35185_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 03359_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 03359_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18608_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 18608_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32036_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32036_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24450_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24450_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22086_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22086_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 19861_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19861_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35038_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35038_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 37765_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 37765_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 06761_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 06761_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 89469_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 89469_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29117_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29117_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 34607_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 34607_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 09652_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 09652_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 121589_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 121589_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36080_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36080_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 151573_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 151573_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (33.6") between the two second-epoch detections
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Considering the candidate 24723_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24723_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30034_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30034_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 42705_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 42705_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20209_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20209_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 48892_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 48892_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 23218_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23218_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25230_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25230_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 38498_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38498_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30781_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30781_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27843_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27843_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 05213_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 05213_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20246_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 20246_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:07.40 +41:34:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23378_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23378_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 42496_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 42496_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 37274_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 37274_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 40920_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 40920_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33541_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33541_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31630_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31630_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 40351_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 40351_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20095_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20095_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22876_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22876_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 37579_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 37579_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:52:39.50 +42:32:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.529 2065964142231022720 313.16460946184 +42.53927088548 13.6447 12.4100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35069_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35069_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33779_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33779_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 34488_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 34488_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 51845_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 51845_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 05909_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 05909_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:00.32 +40:49:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11213_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 11213_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 16704_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 16704_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:48.89 +41:23:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44570_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 44570_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 39012_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 39012_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18850_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 18850_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 04279_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 04279_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 48504_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 48504_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23063_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23063_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 46003_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 46003_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31267_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31267_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 13738_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 13738_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22634_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22634_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25593_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25593_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33685_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33685_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24056_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24056_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 73813_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 73813_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 09307_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 09307_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:56:20.43 +40:56:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25781_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25781_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23369_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23369_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33007_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 33007_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:39:35.45 +42:26:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.758 2066446071917100288 309.89772140690 +42.44796033542 13.7280 12.4571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32604_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32604_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35155_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35155_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28283_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28283_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36731_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36731_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 54496_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 54496_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 05493_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 05493_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 46125_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 46125_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 07139_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 07139_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:44.23 +40:51:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28599_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28599_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18780_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 18780_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:03.02 +41:31:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26481_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 26481_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:52:45.99 +41:56:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24651_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24651_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18496_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 18496_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25349_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25349_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 15410_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 15410_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:08.90 +41:18:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36778_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36778_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27676_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27676_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 65053_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 65053_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:40:49.80 +44:09:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27662_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27662_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 135915_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 135915_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
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Considering the candidate 39034_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 39034_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24211_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24211_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 39753_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 39753_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 19182_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19182_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 13793_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 13793_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:34.03 +41:14:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39006_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 39006_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21290_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21290_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 39550_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 39550_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 34886_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 34886_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 04732_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 04732_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:56:09.86 +40:42:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40322_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 40322_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 75424_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 75424_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 14336_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 14336_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:39.94 +41:14:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10334_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 10334_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 12726_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 12726_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 40434_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 40434_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 64917_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 64917_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29302_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29302_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31066_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31066_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 14491_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 14491_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32434_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32434_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 03416_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 03416_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30569_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30569_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25718_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25718_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 73525_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 73525_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:41:29.79 +44:36:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35428_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35428_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25144_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25144_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27401_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27401_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25654_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25654_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 34600_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 34600_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 41697_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 41697_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 08567_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 08567_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25286_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25286_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 09335_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 09335_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36298_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36298_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33018_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33018_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 07498_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 07498_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 38163_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38163_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 43214_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 43214_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 40938_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 40938_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33540_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33540_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24736_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24736_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24029_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24029_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 44265_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 44265_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24082_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24082_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 58056_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 58056_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33821_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33821_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 74968_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 74968_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:40:15.20 +44:41:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30028_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30028_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 49192_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 49192_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:43:25.30 +43:11:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06062_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 06062_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:48.53 +40:48:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45301_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 45301_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33374_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33374_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 51914_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 51914_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 71059_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 71059_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23413_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23413_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 11839_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 11839_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25411_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25411_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21105_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21105_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 19524_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19524_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 59970_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 59970_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 06095_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 06095_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:53.67 +40:47:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29783_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29783_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32664_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32664_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 46598_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 46598_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23292_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23292_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 16784_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 16784_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 14524_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 14524_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:48.04 +41:16:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28883_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28883_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27015_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27015_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 03730_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 03730_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 49094_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 49094_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21479_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21479_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 13031_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 13031_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:51.17 +41:11:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11517_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 11517_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:54:46.50 +41:05:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37383_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 37383_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31918_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31918_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 07017_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 07017_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 17636_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 17636_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 61272_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 61272_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23283_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 23283_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:52:50.87 +41:46:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38974_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38974_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21069_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21069_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 44360_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 44360_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27011_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27011_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32718_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32718_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 49450_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 49450_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 70398_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 70398_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28993_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28993_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31934_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 31934_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 17820_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 17820_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21000_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21000_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 15782_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 15782_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 75040_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 75040_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22044_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 22044_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:33.75 +41:41:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23766_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23766_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35874_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35874_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25442_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25442_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 75079_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 75079_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 47438_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 47438_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:46:02.23 +43:08:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21794_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21794_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23577_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23577_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36836_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36836_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28911_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28911_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 16725_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 16725_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 45619_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 45619_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27749_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27749_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 70520_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 70520_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:41:48.67 +44:27:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25708_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25708_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 78251_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 78251_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 78164_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 78164_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 06820_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 06820_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35791_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35791_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20276_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 20276_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:50.53 +41:35:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47735_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 47735_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 24051_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24051_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30845_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30845_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29834_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29834_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28207_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28207_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28176_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28176_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 79572_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 79572_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (33.7") between the two second-epoch detections
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Considering the candidate 24271_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24271_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 13453_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 13453_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21541_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21541_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30942_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30942_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27461_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27461_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18722_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 18722_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 07942_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 07942_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23113_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23113_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27068_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27068_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18382_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 18382_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 07747_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 07747_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22351_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22351_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28912_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28912_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 45618_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 45618_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 16259_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 16259_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 43150_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 43150_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 21661_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 21661_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29218_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29218_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 15334_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 15334_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 16136_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 16136_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:21.29 +41:22:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24617_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 24617_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 78039_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 78039_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:35:12.71 +44:53:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30463_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30463_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 38162_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 38162_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:48:40.10 +42:37:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 0.972 2066647935385748480 312.16706836767 +42.61875800765 13.4609 12.8671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 123534_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 123534_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25435_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25435_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 15169_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 15169_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 26033_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 26033_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 05855_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 05855_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36204_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36204_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 17784_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 17784_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32812_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32812_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35390_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35390_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30659_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 30659_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:46:19.19 +42:14:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08036_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 08036_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 47511_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 47511_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 20635_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 20635_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 33445_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33445_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 05018_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 05018_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:57:33.09 +40:41:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84834_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 84834_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 22225_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 22225_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27377_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27377_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 41507_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 41507_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23767_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23767_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 04839_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 04839_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 08707_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 08707_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32719_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32719_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 76690_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 76690_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27715_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27715_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 32914_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 32914_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 47208_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 47208_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 14329_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 14329_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 36946_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 36946_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29464_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29464_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 27740_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 27740_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31889_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31889_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 38072_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 38072_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 31324_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 31324_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 18948_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 18948_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
**** FOUND 20:53:55.44 +41:30:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19909_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 19909_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 40000_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 40000_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 29944_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 29944_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 75092_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 75092_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 139071_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 139071_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
Rejecting candidate due to large distance (32.5") between the two second-epoch detections
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Considering the candidate 33074_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 33074_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 49670_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 49670_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 25315_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25315_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 41211_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
The candidate 41211_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009 did not pass the final checks
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Considering the candidate 25070_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 25070_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 28313_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 28313_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 16869_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 16869_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 35758_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 35758_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 37697_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 37697_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 47531_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 47531_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 62808_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 62808_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 76390_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 76390_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 23137_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 23137_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 39185_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 39185_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
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Considering the candidate 30203_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
Preparing report for the candidate 30203_fd_Cyg-03-Q1b1x1_2026-09-17_03-56-36_20.00sec_-0.00C_LIGHTs_0009
make_report_in_HTML.sh Phase 2 (HTML assembly): 28s
make_report_in_HTML.sh TOTAL: 696s
Prepared the HTML report for the field Cyg-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:52:53.29 +40:41:38.1
20:46:14.81 +40:46:43.6
20:51:12.93 +40:44:12.7
20:50:35.07 +40:46:12.4
20:48:11.25 +40:49:58.8
20:48:25.24 +40:51:06.1
20:52:50.35 +40:47:52.5
20:50:12.98 +40:51:23.3
20:51:39.83 +40:52:41.3
20:52:11.10 +40:52:50.6
20:50:58.70 +40:53:04.7
20:53:10.15 +40:52:40.3
20:46:57.10 +40:59:06.4
20:50:53.04 +40:56:35.2
20:52:19.42 +40:55:30.8
20:53:20.07 +40:55:15.5
20:52:52.53 +40:56:00.1
20:52:59.23 +40:57:24.1
20:51:17.62 +40:59:40.5
20:48:57.94 +41:03:20.8
20:47:40.50 +41:05:32.6
20:14:58.75 +45:49:56.3
20:46:48.48 +41:08:06.5
20:51:33.96 +41:04:35.6
20:48:11.22 +41:08:48.9
20:49:37.78 +41:08:54.5
20:48:08.95 +41:10:32.1
20:49:30.68 +41:11:17.7
20:52:51.60 +41:08:31.3
20:15:17.99 +46:27:35.3
20:15:48.73 +46:33:24.4
20:14:23.88 +46:37:02.0
20:52:14.80 +41:10:34.8
20:13:29.19 +46:38:35.5
20:52:20.78 +41:13:49.7
20:48:01.31 +41:18:26.8
20:51:43.40 +41:15:39.2
20:51:55.06 +41:15:59.2
20:52:26.11 +41:16:10.2
20:51:48.65 +41:17:21.2
20:46:54.24 +41:21:48.9
20:48:31.23 +41:23:11.9
20:49:07.30 +41:22:59.3
20:47:51.50 +41:24:19.2
20:46:47.72 +41:26:14.2
20:52:09.04 +41:23:26.5
20:51:34.31 +41:25:45.5
20:51:15.82 +41:26:13.7
20:48:34.51 +41:28:44.8
20:48:29.57 +41:29:14.6
20:47:43.59 +41:31:42.6
20:51:49.86 +41:28:19.7
20:46:10.51 +41:33:21.8
20:50:44.32 +41:29:51.2
20:48:47.05 +41:32:05.7
20:45:07.57 +41:35:23.8
20:48:20.10 +41:34:04.5
20:51:51.20 +41:31:29.8
20:51:02.18 +41:32:18.8
20:48:03.25 +41:34:59.4
20:51:30.68 +41:32:16.3
20:51:39.99 +41:32:07.9
20:45:00.48 +41:37:55.1
20:47:01.36 +41:37:09.6
20:44:31.32 +41:39:26.4
20:51:27.24 +41:34:31.8
20:51:46.14 +41:34:27.2
20:52:31.41 +41:34:07.8
20:48:32.20 +41:37:34.3
20:46:22.01 +41:40:26.4
20:52:14.50 +41:34:58.4
20:54:00.19 +41:34:00.3
20:45:37.47 +41:41:31.9
20:47:19.26 +41:40:34.9
20:51:09.25 +41:37:26.0
20:44:38.24 +41:42:35.0
20:51:01.65 +41:37:20.3
20:50:40.96 +41:38:00.9
20:49:39.00 +41:39:42.7
20:52:38.81 +41:37:21.4
20:46:39.35 +41:43:16.8
20:50:55.68 +41:40:20.2
20:47:44.97 +41:43:20.9
20:48:33.09 +41:42:36.7
20:49:24.04 +41:41:59.4
20:48:09.51 +41:43:30.3
20:48:54.03 +41:43:31.6
20:44:27.01 +41:46:44.9
20:49:38.36 +41:42:49.3
20:46:35.38 +41:45:42.9
20:46:58.63 +41:45:50.4
20:50:20.72 +41:43:22.4
20:46:49.32 +41:46:10.9
20:50:51.53 +41:43:36.2
20:47:05.03 +41:46:42.6
20:44:05.94 +41:49:10.2
20:48:53.16 +41:45:58.7
20:42:53.48 +41:50:22.5
20:43:32.97 +41:50:10.8
20:46:35.19 +41:48:06.3
20:51:18.70 +41:45:29.5
20:42:12.27 +41:52:14.3
20:48:18.79 +41:48:05.0
20:50:01.41 +41:46:18.5
20:42:44.26 +41:52:40.5
20:50:25.72 +41:47:32.1
20:48:53.30 +41:48:49.1
20:49:51.50 +41:48:17.7
20:51:05.07 +41:46:59.9
20:47:49.80 +41:49:50.9
20:49:43.24 +41:48:30.8
20:48:41.07 +41:49:47.2
20:49:06.85 +41:49:21.7
20:51:22.15 +41:47:39.9
20:50:41.16 +41:48:29.3
20:50:48.69 +41:48:13.7
20:48:40.13 +41:50:15.6
20:50:11.34 +41:48:51.0
20:44:46.86 +41:53:09.3
20:52:24.43 +41:47:43.8
20:43:41.55 +41:54:54.4
20:48:44.85 +41:51:16.3
20:50:03.84 +41:50:52.3
20:48:23.46 +41:52:15.1
20:42:46.37 +41:56:29.2
20:44:04.68 +41:55:28.6
20:48:36.18 +41:52:31.9
20:48:54.68 +41:52:08.3
20:49:44.05 +41:51:30.8
20:44:19.10 +41:55:48.8
20:51:17.31 +41:50:44.9
20:53:03.69 +41:49:10.1
20:50:20.20 +41:52:25.6
20:42:56.03 +41:57:52.2
20:50:54.46 +41:52:21.5
20:53:37.73 +41:50:07.6
20:55:43.79 +41:47:35.7
20:51:51.65 +41:52:04.8
20:50:43.06 +41:53:42.4
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20:48:59.55 +41:55:26.5
20:43:50.53 +41:58:52.6
20:54:30.76 +41:50:56.2
20:58:08.83 +41:47:10.6
20:48:57.73 +41:55:54.9
20:50:57.06 +41:54:30.1
20:47:36.07 +41:57:04.7
20:47:00.83 +41:57:50.4
20:53:43.21 +41:52:38.1
20:54:56.46 +41:51:14.0
20:55:11.39 +41:51:15.9
20:43:48.63 +42:00:25.1
20:47:51.49 +41:57:28.1
20:50:28.78 +41:56:06.7
20:51:19.07 +41:55:31.4
20:49:31.65 +41:57:07.4
20:49:40.33 +41:56:56.1
20:44:39.24 +42:00:53.6
20:48:39.23 +41:57:07.3
20:47:09.04 +41:59:16.3
20:45:42.96 +42:00:25.1
20:51:56.14 +41:55:20.1
20:49:14.17 +41:58:17.0
20:47:32.84 +41:59:43.0
20:42:33.74 +42:03:31.4
20:54:49.61 +41:53:51.9
20:46:30.43 +42:01:03.3
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20:54:12.96 +41:57:07.9
20:47:24.60 +42:03:13.0
20:46:05.41 +42:04:52.9
20:52:47.87 +41:59:28.7
20:42:36.34 +42:07:28.5
20:52:12.43 +42:00:58.9
20:44:14.98 +42:07:12.8
20:54:22.30 +41:59:16.1
20:50:05.22 +42:03:00.0
20:45:56.57 +42:06:28.5
20:46:23.97 +42:06:23.3
20:40:42.64 +42:10:43.2
20:42:51.54 +42:09:19.9
20:43:28.61 +42:08:56.5
20:44:48.18 +42:08:14.9
20:43:07.37 +42:09:28.8
20:41:18.00 +42:10:57.5
20:47:33.81 +42:06:42.9
20:45:30.80 +42:09:03.0
20:41:52.91 +42:11:50.4
20:39:56.24 +42:13:27.5
20:48:26.11 +42:07:56.8
20:46:52.82 +42:08:59.4
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20:40:41.72 +42:13:22.5
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20:44:11.30 +42:12:06.7
20:43:30.49 +42:12:43.6
20:49:46.03 +42:08:00.9
20:45:41.34 +42:11:18.0
20:45:32.53 +42:12:28.1
20:48:13.02 +42:09:53.6
20:54:29.35 +42:05:12.8
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20:43:27.31 +42:14:35.9
20:54:02.41 +42:06:27.6
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20:44:28.34 +42:14:08.7
20:44:17.75 +42:14:55.4
20:41:24.50 +42:17:34.0
20:45:20.32 +42:15:12.9
20:53:16.86 +42:09:03.0
20:47:08.92 +42:14:20.3
20:41:24.25 +42:18:49.5
20:44:50.38 +42:16:37.9
20:44:33.34 +42:17:07.7
20:49:44.10 +42:13:14.1
20:48:47.96 +42:14:18.9
20:53:29.11 +42:10:19.8
20:53:10.52 +42:10:28.5
20:47:42.36 +42:15:51.3
20:44:04.70 +42:18:35.7
20:39:29.97 +42:21:52.0
20:46:01.52 +42:17:52.8
20:46:00.19 +42:18:21.6
20:45:44.41 +42:18:37.9
20:41:38.95 +42:20:53.0
20:45:43.04 +42:19:20.1
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20:41:50.65 +42:22:13.8
20:44:43.68 +42:20:56.9
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20:53:32.74 +42:14:22.0
20:44:38.55 +42:21:56.0
20:43:13.54 +42:22:47.0
20:40:11.51 +42:24:38.9
20:51:14.23 +42:16:58.7
20:40:03.89 +42:25:12.7
20:41:05.93 +42:24:42.0
20:41:19.77 +42:24:44.6
20:41:38.46 +42:24:32.1
20:50:04.64 +42:18:47.6
20:42:49.44 +42:23:11.6
20:46:57.01 +42:21:26.2
20:41:29.42 +42:25:04.6
20:46:00.97 +42:22:19.4
20:47:25.54 +42:21:01.8
20:43:52.11 +42:24:05.9
20:48:06.75 +42:21:03.5
20:47:52.66 +42:21:25.5
20:43:06.16 +42:25:20.9
20:43:03.84 +42:25:15.8
20:41:43.44 +42:26:21.8
20:38:52.74 +42:28:01.6
20:40:56.22 +42:27:26.1
20:52:54.02 +42:18:36.1
20:43:56.67 +42:25:37.2
20:41:33.41 +42:27:22.5
20:42:04.38 +42:27:06.1
20:41:28.21 +42:27:29.9
20:49:46.94 +42:22:03.4
20:51:57.23 +42:20:13.0
20:41:20.93 +42:27:53.5
20:49:35.86 +42:22:16.8
20:43:37.19 +42:26:25.2
20:42:40.42 +42:27:08.9
20:44:05.30 +42:26:28.8
20:43:45.89 +42:26:49.2
20:41:42.50 +42:28:19.1
20:38:49.39 +42:29:54.2
20:53:21.23 +42:19:15.9
20:41:36.24 +42:29:14.6
20:41:31.87 +42:30:25.9
20:38:29.33 +42:32:11.1
20:44:24.85 +42:29:04.4
20:49:49.81 +42:25:12.6
20:45:22.25 +42:29:22.1
20:43:48.81 +42:30:50.9
20:50:51.21 +42:25:34.6
20:53:10.61 +42:23:32.5
20:41:29.08 +42:32:38.2
20:53:06.23 +42:24:01.2
20:41:37.97 +42:32:55.5
20:40:46.38 +42:33:32.9
20:46:35.79 +42:30:17.7
20:40:33.71 +42:33:42.3
20:40:39.24 +42:33:46.5
20:42:23.84 +42:34:02.8
20:41:07.89 +42:34:21.4
20:53:54.47 +42:24:53.1
20:52:37.80 +42:26:09.8
20:51:46.20 +42:27:04.2
20:39:14.40 +42:36:13.9
20:42:18.04 +42:34:26.4
20:51:09.00 +42:28:31.3
20:41:35.52 +42:36:03.5
20:52:05.62 +42:28:27.9
20:51:03.76 +42:29:30.0
20:41:41.09 +42:37:35.5
20:40:57.66 +42:37:51.9
20:41:04.52 +42:38:07.3
20:44:32.93 +42:35:57.7
20:42:10.39 +42:37:32.6
20:50:02.38 +42:32:06.5
20:39:41.84 +42:39:33.3
20:48:58.68 +42:34:19.3
20:52:06.36 +42:31:31.5
20:38:30.98 +42:40:59.5
20:53:24.99 +42:30:38.5
20:47:47.62 +42:36:22.9
20:53:11.56 +42:31:53.6
20:41:04.28 +42:41:02.7
20:53:37.43 +42:32:29.4
20:51:38.47 +42:34:34.4
20:50:58.16 +42:36:05.0
20:46:54.96 +42:39:27.0
20:48:16.50 +42:38:47.2
20:45:12.41 +42:41:22.6
20:47:59.59 +42:39:40.4
20:40:04.49 +42:45:08.1
20:46:59.57 +42:40:45.8
20:53:00.18 +42:36:15.5
20:47:06.59 +42:38:55.8
20:54:35.22 +42:34:50.3
20:40:37.73 +42:45:48.6
20:40:30.87 +42:46:56.2
20:47:26.96 +42:43:10.6
20:56:11.88 +42:36:06.1
20:41:41.21 +42:49:09.8
20:51:11.95 +42:42:18.7
20:47:03.33 +42:47:09.3
20:50:59.21 +42:44:17.0
20:42:18.15 +42:50:32.1
20:50:57.25 +42:45:47.6
20:43:22.33 +42:52:06.8
20:46:34.17 +42:50:10.4
20:39:25.17 +42:56:24.0
20:43:46.66 +42:54:51.7
20:47:24.57 +42:53:04.9
20:41:06.41 +42:57:17.8
20:40:09.79 +42:57:36.9
20:46:07.15 +42:55:13.0
20:39:21.47 +42:59:33.2
20:38:25.48 +43:01:53.3
20:47:27.94 +42:57:38.2
20:46:12.54 +42:59:23.5
20:46:19.49 +42:59:59.7
20:41:43.19 +43:03:05.0
20:46:43.86 +42:59:43.9
20:50:00.64 +42:58:09.8
20:46:56.69 +43:01:26.9
20:45:12.88 +43:03:09.7
20:40:11.15 +43:06:56.4
20:42:44.73 +43:05:28.7
20:50:03.95 +43:00:11.4
20:41:43.82 +43:06:18.7
20:46:10.36 +43:04:35.2
20:42:13.97 +43:07:33.8
20:46:07.80 +43:06:31.8
20:40:11.55 +43:12:14.3
20:46:17.49 +43:09:28.2
20:45:44.30 +43:09:42.4
20:39:36.02 +43:14:22.3
20:40:18.24 +43:16:36.7
20:45:17.66 +43:13:15.4
20:46:13.93 +43:12:46.4
20:42:16.86 +43:17:16.3
20:40:53.22 +43:18:20.9
20:42:00.63 +43:18:43.4
20:37:28.44 +43:21:45.0
20:36:47.07 +43:29:11.2
20:41:21.08 +43:27:15.4
20:40:58.64 +43:27:45.7
20:37:34.46 +43:31:51.0
20:40:38.00 +43:31:06.6
20:42:57.95 +43:34:25.0
20:40:15.41 +43:47:43.5
20:39:59.71 +43:51:28.4
20:43:39.89 +43:49:55.4
20:35:49.43 +43:55:31.6
20:34:39.22 +44:00:04.4
20:43:56.21 +43:55:58.2
20:44:04.13 +44:00:50.1
20:44:32.41 +44:01:35.5
20:41:10.32 +44:09:31.8
20:42:49.40 +44:11:19.2
20:42:32.70 +44:14:46.6
20:41:20.73 +44:26:46.9
20:41:08.20 +44:26:50.2
20:39:49.84 +44:27:58.5
20:42:22.22 +44:28:53.4
20:39:55.86 +44:31:04.8
20:41:32.33 +44:30:23.9
20:40:26.66 +44:31:56.9
20:41:21.14 +44:32:39.7
20:41:13.45 +44:38:12.3
20:40:48.41 +44:40:10.2
20:40:18.25 +44:40:33.5
20:40:29.54 +44:41:45.8
20:41:21.37 +44:41:30.9
20:39:42.16 +44:42:30.0
20:41:21.77 +44:39:58.7
20:39:24.63 +44:43:29.3
20:39:03.16 +44:46:47.9
20:39:41.40 +44:46:56.4
20:40:39.90 +44:46:33.9
20:38:27.91 +44:52:05.0
20:40:20.93 +44:51:23.4
20:32:36.71 +45:08:02.4
20:38:29.43 +45:07:16.0
20:38:16.84 +45:09:49.9
20:18:26.77 +45:24:20.3
########### Completed Cyg-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
20:32:36.71 +45:08:02.4
20:51:27.24 +41:34:31.8
20:48:47.05 +41:32:05.7
20:48:54.68 +41:52:08.3
20:14:58.75 +45:49:56.3
20:48:11.22 +41:08:48.9
20:50:51.53 +41:43:36.2
20:50:04.64 +42:18:47.6
20:47:01.36 +41:37:09.6
20:49:46.94 +42:22:03.4
20:13:29.19 +46:38:35.5
20:46:43.86 +42:59:43.9
20:41:29.42 +42:25:04.6
20:44:32.41 +44:01:35.5
20:38:29.43 +45:07:16.0
20:48:18.79 +41:48:05.0
20:40:38.00 +43:31:06.6
20:39:25.17 +42:56:24.0
20:49:14.17 +41:58:17.0
20:58:08.83 +41:47:10.6
20:40:09.79 +42:57:36.9
20:46:30.43 +42:01:03.3
20:42:51.54 +42:09:19.9
20:39:56.24 +42:13:27.5
20:40:26.66 +44:31:56.9
20:52:51.60 +41:08:31.3
20:48:06.75 +42:21:03.5
20:41:06.41 +42:57:17.8
20:47:19.26 +41:40:34.9
20:42:49.40 +44:11:19.2
20:46:19.49 +42:59:59.7
20:44:05.30 +42:26:28.8
20:41:42.50 +42:28:19.1
20:51:57.23 +42:20:13.0
20:44:38.24 +41:42:35.0
20:48:54.03 +41:43:31.6
20:41:37.97 +42:32:55.5
20:48:13.02 +42:09:53.6
20:49:44.10 +42:13:14.1
20:42:23.84 +42:34:02.8
20:39:29.97 +42:21:52.0
20:41:38.95 +42:20:53.0
20:41:43.44 +42:26:21.8
20:43:48.63 +42:00:25.1
20:39:14.40 +42:36:13.9
20:54:00.19 +41:34:00.3
20:53:10.52 +42:10:28.5
20:48:01.31 +41:18:26.8
20:54:49.61 +41:53:51.9
20:47:25.54 +42:21:01.8
20:40:18.25 +44:40:33.5
20:51:05.07 +41:46:59.9
20:43:32.97 +41:50:10.8
20:42:56.03 +41:57:52.2
20:42:10.39 +42:37:32.6
20:42:16.86 +43:17:16.3
20:51:46.14 +41:34:27.2
20:51:19.07 +41:55:31.4
20:50:41.16 +41:48:29.3
20:49:39.00 +41:39:42.7
20:41:07.89 +42:34:21.4
20:47:59.59 +42:39:40.4
20:51:56.14 +41:55:20.1
20:51:03.76 +42:29:30.0
20:40:56.22 +42:27:26.1
20:39:59.71 +43:51:28.4
20:53:11.56 +42:31:53.6
20:47:05.03 +41:46:42.6
20:39:41.84 +42:39:33.3
20:43:28.61 +42:08:56.5
20:50:11.34 +41:48:51.0
20:52:11.10 +40:52:50.6
20:41:20.93 +42:27:53.5
20:39:55.86 +44:31:04.8
20:39:41.40 +44:46:56.4
20:43:48.81 +42:30:50.9
20:48:32.20 +41:37:34.3
20:52:26.11 +41:16:10.2
20:48:53.30 +41:48:49.1
20:53:32.74 +42:14:22.0
20:50:53.04 +40:56:35.2
20:48:23.46 +41:52:15.1
20:50:25.72 +41:47:32.1
20:38:25.48 +43:01:53.3
20:46:57.01 +42:21:26.2
20:34:39.22 +44:00:04.4
20:48:39.23 +41:57:07.3
20:51:49.86 +41:28:19.7
20:47:03.33 +42:47:09.3
20:49:24.04 +41:41:59.4
20:40:39.24 +42:33:46.5
20:52:06.36 +42:31:31.5
20:51:09.25 +41:37:26.0
20:40:48.41 +44:40:10.2
20:50:20.72 +41:43:22.4
20:46:48.48 +41:08:06.5
20:41:05.93 +42:24:42.0
20:45:32.53 +42:12:28.1
20:51:17.31 +41:50:44.9
20:49:38.36 +41:42:49.3
20:41:52.91 +42:11:50.4
20:50:43.74 +42:05:55.4
20:43:43.35 +42:21:50.5
20:43:56.67 +42:25:37.2
20:46:56.69 +43:01:26.9
20:43:06.16 +42:25:20.9
20:51:02.18 +41:32:18.8
20:51:27.41 +41:53:07.5
20:40:11.51 +42:24:38.9
20:47:51.49 +41:57:28.1
20:53:21.23 +42:19:15.9
20:40:58.64 +43:27:45.7
20:46:54.96 +42:39:27.0
20:46:00.19 +42:18:21.6
20:37:34.46 +43:31:51.0
20:43:30.49 +42:12:43.6
20:45:20.32 +42:15:12.9
20:44:28.34 +42:14:08.7
20:15:17.99 +46:27:35.3
20:50:43.06 +41:53:42.4
20:51:01.65 +41:37:20.3
20:43:22.33 +42:52:06.8
20:42:32.70 +44:14:46.6
20:41:43.82 +43:06:18.7
20:45:07.57 +41:35:23.8
20:43:13.54 +42:22:47.0
20:48:47.96 +42:14:18.9
20:42:18.04 +42:34:26.4
20:38:30.98 +42:40:59.5
20:46:01.52 +42:17:52.8
20:49:49.81 +42:25:12.6
20:41:36.24 +42:29:14.6
20:51:18.70 +41:45:29.5
20:40:29.54 +44:41:45.8
20:41:08.20 +44:26:50.2
20:40:33.71 +42:33:42.3
20:51:30.68 +41:32:16.3
20:43:39.89 +43:49:55.4
20:48:29.57 +41:29:14.6
20:43:37.19 +42:26:25.2
20:48:41.07 +41:49:47.2
20:50:03.95 +43:00:11.4
20:50:58.16 +42:36:05.0
20:50:03.84 +41:50:52.3
20:47:51.50 +41:24:19.2
20:50:00.64 +42:58:09.8
20:47:09.04 +41:59:16.3
20:46:13.93 +43:12:46.4
20:46:39.35 +41:43:16.8
20:41:41.09 +42:37:35.5
20:41:21.14 +44:32:39.7
20:41:28.21 +42:27:29.9
20:41:32.33 +44:30:23.9
20:52:14.80 +41:10:34.8
20:53:16.86 +42:09:03.0
20:45:12.41 +42:41:22.6
20:41:20.73 +44:26:46.9
20:51:55.06 +41:15:59.2
20:50:01.41 +41:46:18.5
20:42:53.48 +41:50:22.5
20:44:43.68 +42:20:56.9
20:48:08.95 +41:10:32.1
20:43:03.84 +42:25:15.8
20:48:59.55 +41:55:26.5
20:40:04.49 +42:45:08.1
20:45:17.66 +43:13:15.4
20:38:49.39 +42:29:54.2
20:42:33.74 +42:03:31.4
20:40:42.64 +42:10:43.2
20:53:06.23 +42:24:01.2
20:52:53.29 +40:41:38.1
20:48:03.25 +41:34:59.4
20:41:50.65 +42:22:13.8
20:50:20.20 +41:52:25.6
20:44:05.94 +41:49:10.2
20:46:22.01 +41:40:26.4
20:50:51.21 +42:25:34.6
20:41:04.28 +42:41:02.7
20:51:39.83 +40:52:41.3
20:18:26.77 +45:24:20.3
20:43:55.84 +42:11:44.3
20:44:24.85 +42:29:04.4
20:47:40.50 +41:05:32.6
20:15:48.73 +46:33:24.4
20:51:09.00 +42:28:31.3
20:55:43.79 +41:47:35.7
20:45:36.47 +42:13:42.1
20:47:24.57 +42:53:04.9
20:50:40.96 +41:38:00.9
20:49:06.85 +41:49:21.7
20:48:57.73 +41:55:54.9
20:48:16.50 +42:38:47.2
20:41:24.25 +42:18:49.5
20:46:23.97 +42:06:23.3
20:48:25.24 +40:51:06.1
20:48:40.13 +41:50:15.6
20:43:46.66 +42:54:51.7
20:48:58.68 +42:34:19.3
20:50:59.21 +42:44:17.0
20:42:04.38 +42:27:06.1
20:45:44.41 +42:18:37.9
20:41:41.21 +42:49:09.8
20:45:37.47 +41:41:31.9
20:42:44.26 +41:52:40.5
20:53:10.61 +42:23:32.5
20:42:40.42 +42:27:08.9
20:41:31.87 +42:30:25.9
20:36:47.07 +43:29:11.2
20:49:37.78 +41:08:54.5
20:41:43.19 +43:03:05.0
20:47:06.59 +42:38:55.8
20:45:00.48 +41:37:55.1
20:50:35.07 +40:46:12.4
20:40:18.24 +43:16:36.7
20:49:51.50 +41:48:17.7
20:46:10.36 +43:04:35.2
20:47:42.36 +42:15:51.3
20:51:43.40 +41:15:39.2
20:42:12.27 +41:52:14.3
20:50:28.78 +41:56:06.7
20:49:35.86 +42:22:16.8
20:48:36.18 +41:52:31.9
20:41:13.45 +44:38:12.3
20:45:42.96 +42:00:25.1
20:50:48.69 +41:48:13.7
20:51:14.23 +42:16:58.7
20:41:29.08 +42:32:38.2
20:41:18.00 +42:10:57.5
20:40:57.66 +42:37:51.9
20:42:57.95 +43:34:25.0
20:52:50.35 +40:47:52.5
20:42:13.97 +43:07:33.8
20:45:30.80 +42:09:03.0
20:53:37.73 +41:50:07.6
20:51:51.20 +41:31:29.8
20:47:00.83 +41:57:50.4
20:41:04.52 +42:38:07.3
20:44:14.98 +42:07:12.8
20:52:12.43 +42:00:58.9
20:54:35.22 +42:34:50.3
20:44:19.10 +41:55:48.8
20:47:26.96 +42:43:10.6
20:44:31.32 +41:39:26.4
20:53:00.18 +42:36:15.5
20:48:09.51 +41:43:30.3
20:40:30.87 +42:46:56.2
20:45:22.25 +42:29:22.1
20:39:24.63 +44:43:29.3
20:51:33.96 +41:04:35.6
20:51:11.95 +42:42:18.7
20:41:10.32 +44:09:31.8
20:49:46.03 +42:08:00.9
20:53:29.11 +42:10:19.8
20:46:54.24 +41:21:48.9
20:44:38.55 +42:21:56.0
20:46:14.81 +40:46:43.6
20:47:08.92 +42:14:20.3
20:44:39.24 +42:00:53.6
20:46:35.79 +42:30:17.7
20:54:30.76 +41:50:56.2
20:52:47.87 +41:59:28.7
20:49:31.65 +41:57:07.4
20:38:29.33 +42:32:11.1
20:46:34.17 +42:50:10.4
20:52:59.23 +40:57:24.1
20:50:57.06 +41:54:30.1
20:48:57.94 +41:03:20.8
20:52:05.62 +42:28:27.9
20:43:52.11 +42:24:05.9
20:46:57.10 +40:59:06.4
20:51:38.47 +42:34:34.4
20:39:21.47 +42:59:33.2
20:42:18.15 +42:50:32.1
20:41:33.41 +42:27:22.5
20:51:51.65 +41:52:04.8
20:42:46.37 +41:56:29.2
20:47:27.94 +42:57:38.2
20:49:44.05 +41:51:30.8
20:40:15.41 +43:47:43.5
20:43:45.89 +42:26:49.2
20:54:02.41 +42:06:27.6
20:45:12.88 +43:03:09.7
20:38:52.74 +42:28:01.6
20:41:21.08 +43:27:15.4
20:42:22.22 +44:28:53.4
20:44:46.86 +41:53:09.3
20:49:30.68 +41:11:17.7
20:53:43.21 +41:52:38.1
20:48:33.09 +41:42:36.7
20:52:31.41 +41:34:07.8
20:35:49.43 +43:55:31.6
20:54:29.35 +42:05:12.8
20:40:03.89 +42:25:12.7
20:46:07.80 +43:06:31.8
20:51:22.15 +41:47:39.9
20:51:15.82 +41:26:13.7
20:48:26.11 +42:07:56.8
20:54:12.96 +41:57:07.9
20:51:12.93 +40:44:12.7
20:40:53.22 +43:18:20.9
20:44:27.01 +41:46:44.9
20:53:24.99 +42:30:38.5
20:50:43.19 +42:15:26.8
20:53:10.15 +40:52:40.3
20:47:43.59 +41:31:42.6
20:43:56.21 +43:55:58.2
20:46:59.57 +42:40:45.8
20:47:44.97 +41:43:20.9
20:46:12.54 +42:59:23.5
20:45:49.52 +42:03:56.3
20:41:19.77 +42:24:44.6
20:42:00.63 +43:18:43.4
20:39:49.84 +44:27:58.5
20:40:41.72 +42:13:22.5
20:50:44.32 +41:29:51.2
20:50:55.68 +41:40:20.2
20:46:47.72 +41:26:14.2
20:41:21.37 +44:41:30.9
20:43:41.55 +41:54:54.4
20:51:46.20 +42:27:04.2
20:55:11.39 +41:51:15.9
20:39:42.16 +44:42:30.0
20:46:49.32 +41:46:10.9
20:52:24.43 +41:47:43.8
20:44:32.93 +42:35:57.7
20:46:52.82 +42:08:59.4
20:51:34.31 +41:25:45.5
20:42:44.73 +43:05:28.7
20:45:56.57 +42:06:28.5
20:49:40.33 +41:56:56.1
20:40:20.93 +44:51:23.4
20:38:27.91 +44:52:05.0
20:50:58.70 +40:53:04.7
20:52:37.80 +42:26:09.8
20:39:36.02 +43:14:22.3
20:44:04.68 +41:55:28.6
20:44:50.38 +42:16:37.9
20:40:49.30 +42:15:44.3
20:43:07.37 +42:09:28.8
20:44:48.18 +42:08:14.9
20:53:03.69 +41:49:10.1
20:52:20.78 +41:13:49.7
20:46:35.38 +41:45:42.9
20:44:33.34 +42:17:07.7
20:42:36.34 +42:07:28.5
20:51:39.99 +41:32:07.9
20:53:20.07 +40:55:15.5
20:47:49.80 +41:49:50.9
20:47:24.60 +42:03:13.0
20:48:20.10 +41:34:04.5
20:52:19.42 +40:55:30.8
20:46:35.19 +41:48:06.3
20:47:16.87 +42:08:43.6
20:40:11.15 +43:06:56.4
20:52:09.04 +41:23:26.5
20:46:07.15 +42:55:13.0
20:46:58.63 +41:45:50.4
20:44:11.30 +42:12:06.7
20:49:07.30 +41:22:59.3
20:50:54.46 +41:52:21.5
20:41:24.50 +42:17:34.0
20:14:23.88 +46:37:02.0
20:54:56.46 +41:51:14.0
20:48:31.23 +41:23:11.9
20:47:32.84 +41:59:43.0
20:50:12.98 +40:51:23.3
20:41:35.52 +42:36:03.5
20:46:10.51 +41:33:21.8
20:42:49.44 +42:23:11.6
20:40:46.38 +42:33:32.9
20:52:52.53 +40:56:00.1
20:46:17.49 +43:09:28.2
20:52:38.81 +41:37:21.4
20:52:54.02 +42:18:36.1
20:38:16.84 +45:09:49.9
20:48:53.16 +41:45:58.7
20:46:05.41 +42:04:52.9
20:50:57.25 +42:45:47.6
20:48:44.85 +41:51:16.3
20:48:11.25 +40:49:58.8
20:51:17.62 +40:59:40.5
20:41:38.46 +42:24:32.1
20:40:39.90 +44:46:33.9
20:54:22.30 +41:59:16.1
20:46:00.97 +42:22:19.4
20:40:11.55 +43:12:14.3
20:51:48.65 +41:17:21.2
20:50:02.38 +42:32:06.5
20:45:41.34 +42:11:18.0
20:50:05.22 +42:03:00.0
20:45:43.04 +42:19:20.1
20:53:37.43 +42:32:29.4
20:44:04.70 +42:18:35.7
20:52:14.50 +41:34:58.4
20:56:11.88 +42:36:06.1
20:43:27.31 +42:14:35.9
20:41:21.77 +44:39:58.7
20:47:52.66 +42:21:25.5
20:37:28.44 +43:21:45.0
20:47:36.07 +41:57:04.7
20:43:50.53 +41:58:52.6
20:47:33.81 +42:06:42.9
20:48:34.51 +41:28:44.8
20:53:54.47 +42:24:53.1
20:47:47.62 +42:36:22.9
20:45:44.30 +43:09:42.4
20:44:04.13 +44:00:50.1
20:39:03.16 +44:46:47.9
20:49:43.24 +41:48:30.8
20:40:37.73 +42:45:48.6
20:44:17.75 +42:14:55.4
###################################################################################
20:32:36.71 +45:08:02.4 -- not an asteroid (will add it to exclusion list)
20:51:27.24 +41:34:31.8 -- not an asteroid (will add it to exclusion list)
20:48:47.05 +41:32:05.7 -- not an asteroid (will add it to exclusion list)
20:48:54.68 +41:52:08.3 -- not an asteroid (will add it to exclusion list)
20:14:58.75 +45:49:56.3 -- not an asteroid (will add it to exclusion list)
20:48:11.22 +41:08:48.9 -- not an asteroid (will add it to exclusion list)
20:50:51.53 +41:43:36.2 -- not an asteroid (will add it to exclusion list)
20:50:04.64 +42:18:47.6 -- not an asteroid (will add it to exclusion list)
20:47:01.36 +41:37:09.6 -- not an asteroid (will add it to exclusion list)
20:49:46.94 +42:22:03.4 -- not an asteroid (will add it to exclusion list)
20:13:29.19 +46:38:35.5 -- not an asteroid (will add it to exclusion list)
20:46:43.86 +42:59:43.9 -- not an asteroid (will add it to exclusion list)
20:41:29.42 +42:25:04.6 -- not an asteroid (will add it to exclusion list)
20:44:32.41 +44:01:35.5 -- not an asteroid (will add it to exclusion list)
20:38:29.43 +45:07:16.0 -- not an asteroid (will add it to exclusion list)
20:48:18.79 +41:48:05.0 -- not an asteroid (will add it to exclusion list)
20:40:38.00 +43:31:06.6 -- not an asteroid (will add it to exclusion list)
20:39:25.17 +42:56:24.0 -- not an asteroid (will add it to exclusion list)
20:49:14.17 +41:58:17.0 -- not an asteroid (will add it to exclusion list)
20:58:08.83 +41:47:10.6 -- not an asteroid (will add it to exclusion list)
20:40:09.79 +42:57:36.9 -- not an asteroid (will add it to exclusion list)
20:46:30.43 +42:01:03.3 -- not an asteroid (will add it to exclusion list)
20:42:51.54 +42:09:19.9 -- not an asteroid (will add it to exclusion list)
20:39:56.24 +42:13:27.5 -- not an asteroid (will add it to exclusion list)
20:40:26.66 +44:31:56.9 -- not an asteroid (will add it to exclusion list)
20:52:51.60 +41:08:31.3 -- not an asteroid (will add it to exclusion list)
20:48:06.75 +42:21:03.5 -- not an asteroid (will add it to exclusion list)
20:41:06.41 +42:57:17.8 -- not an asteroid (will add it to exclusion list)
20:47:19.26 +41:40:34.9 -- not an asteroid (will add it to exclusion list)
20:42:49.40 +44:11:19.2 -- not an asteroid (will add it to exclusion list)
20:46:19.49 +42:59:59.7 -- not an asteroid (will add it to exclusion list)
20:44:05.30 +42:26:28.8 -- not an asteroid (will add it to exclusion list)
20:41:42.50 +42:28:19.1 -- not an asteroid (will add it to exclusion list)
20:51:57.23 +42:20:13.0 -- not an asteroid (will add it to exclusion list)
20:44:38.24 +41:42:35.0 -- not an asteroid (will add it to exclusion list)
20:48:54.03 +41:43:31.6 -- not an asteroid (will add it to exclusion list)
20:41:37.97 +42:32:55.5 -- not an asteroid (will add it to exclusion list)
20:48:13.02 +42:09:53.6 -- not an asteroid (will add it to exclusion list)
20:49:44.10 +42:13:14.1 -- not an asteroid (will add it to exclusion list)
20:42:23.84 +42:34:02.8 -- not an asteroid (will add it to exclusion list)
20:39:29.97 +42:21:52.0 -- not an asteroid (will add it to exclusion list)
20:41:38.95 +42:20:53.0 -- not an asteroid (will add it to exclusion list)
20:41:43.44 +42:26:21.8 -- not an asteroid (will add it to exclusion list)
20:43:48.63 +42:00:25.1 -- not an asteroid (will add it to exclusion list)
20:39:14.40 +42:36:13.9 -- not an asteroid (will add it to exclusion list)
20:54:00.19 +41:34:00.3 -- not an asteroid (will add it to exclusion list)
20:53:10.52 +42:10:28.5 -- not an asteroid (will add it to exclusion list)
20:48:01.31 +41:18:26.8 -- not an asteroid (will add it to exclusion list)
20:54:49.61 +41:53:51.9 -- not an asteroid (will add it to exclusion list)
20:47:25.54 +42:21:01.8 -- not an asteroid (will add it to exclusion list)
20:40:18.25 +44:40:33.5 -- not an asteroid (will add it to exclusion list)
20:51:05.07 +41:46:59.9 -- not an asteroid (will add it to exclusion list)
20:43:32.97 +41:50:10.8 -- not an asteroid (will add it to exclusion list)
20:42:56.03 +41:57:52.2 -- not an asteroid (will add it to exclusion list)
20:42:10.39 +42:37:32.6 -- not an asteroid (will add it to exclusion list)
20:42:16.86 +43:17:16.3 -- not an asteroid (will add it to exclusion list)
20:51:46.14 +41:34:27.2 -- not an asteroid (will add it to exclusion list)
20:51:19.07 +41:55:31.4 -- not an asteroid (will add it to exclusion list)
20:50:41.16 +41:48:29.3 -- not an asteroid (will add it to exclusion list)
20:49:39.00 +41:39:42.7 -- not an asteroid (will add it to exclusion list)
20:41:07.89 +42:34:21.4 -- not an asteroid (will add it to exclusion list)
20:47:59.59 +42:39:40.4 -- not an asteroid (will add it to exclusion list)
20:51:56.14 +41:55:20.1 -- not an asteroid (will add it to exclusion list)
20:51:03.76 +42:29:30.0 -- not an asteroid (will add it to exclusion list)
20:40:56.22 +42:27:26.1 -- not an asteroid (will add it to exclusion list)
20:39:59.71 +43:51:28.4 -- not an asteroid (will add it to exclusion list)
20:53:11.56 +42:31:53.6 -- not an asteroid (will add it to exclusion list)
20:47:05.03 +41:46:42.6 -- not an asteroid (will add it to exclusion list)
20:39:41.84 +42:39:33.3 -- not an asteroid (will add it to exclusion list)
20:43:28.61 +42:08:56.5 -- not an asteroid (will add it to exclusion list)
20:50:11.34 +41:48:51.0 -- not an asteroid (will add it to exclusion list)
20:52:11.10 +40:52:50.6 -- not an asteroid (will add it to exclusion list)
20:41:20.93 +42:27:53.5 -- not an asteroid (will add it to exclusion list)
20:39:55.86 +44:31:04.8 -- not an asteroid (will add it to exclusion list)
20:39:41.40 +44:46:56.4 -- not an asteroid (will add it to exclusion list)
20:43:48.81 +42:30:50.9 -- not an asteroid (will add it to exclusion list)
20:48:32.20 +41:37:34.3 -- not an asteroid (will add it to exclusion list)
20:52:26.11 +41:16:10.2 -- not an asteroid (will add it to exclusion list)
20:48:53.30 +41:48:49.1 -- not an asteroid (will add it to exclusion list)
20:53:32.74 +42:14:22.0 -- not an asteroid (will add it to exclusion list)
20:50:53.04 +40:56:35.2 -- not an asteroid (will add it to exclusion list)
20:48:23.46 +41:52:15.1 -- not an asteroid (will add it to exclusion list)
20:50:25.72 +41:47:32.1 -- not an asteroid (will add it to exclusion list)
20:38:25.48 +43:01:53.3 -- not an asteroid (will add it to exclusion list)
20:46:57.01 +42:21:26.2 -- not an asteroid (will add it to exclusion list)
20:34:39.22 +44:00:04.4 -- not an asteroid (will add it to exclusion list)
20:48:39.23 +41:57:07.3 -- not an asteroid (will add it to exclusion list)
20:51:49.86 +41:28:19.7 -- not an asteroid (will add it to exclusion list)
20:47:03.33 +42:47:09.3 -- not an asteroid (will add it to exclusion list)
20:49:24.04 +41:41:59.4 -- not an asteroid (will add it to exclusion list)
20:40:39.24 +42:33:46.5 -- not an asteroid (will add it to exclusion list)
20:52:06.36 +42:31:31.5 -- not an asteroid (will add it to exclusion list)
20:51:09.25 +41:37:26.0 -- not an asteroid (will add it to exclusion list)
20:40:48.41 +44:40:10.2 -- not an asteroid (will add it to exclusion list)
20:50:20.72 +41:43:22.4 -- not an asteroid (will add it to exclusion list)
20:46:48.48 +41:08:06.5 -- not an asteroid (will add it to exclusion list)
20:41:05.93 +42:24:42.0 -- not an asteroid (will add it to exclusion list)
20:45:32.53 +42:12:28.1 -- not an asteroid (will add it to exclusion list)
20:51:17.31 +41:50:44.9 -- not an asteroid (will add it to exclusion list)
20:49:38.36 +41:42:49.3 -- not an asteroid (will add it to exclusion list)
20:41:52.91 +42:11:50.4 -- not an asteroid (will add it to exclusion list)
20:50:43.74 +42:05:55.4 -- not an asteroid (will add it to exclusion list)
20:43:43.35 +42:21:50.5 -- not an asteroid (will add it to exclusion list)
20:43:56.67 +42:25:37.2 -- not an asteroid (will add it to exclusion list)
20:46:56.69 +43:01:26.9 -- not an asteroid (will add it to exclusion list)
20:43:06.16 +42:25:20.9 -- not an asteroid (will add it to exclusion list)
20:51:02.18 +41:32:18.8 -- not an asteroid (will add it to exclusion list)
20:51:27.41 +41:53:07.5 -- not an asteroid (will add it to exclusion list)
20:40:11.51 +42:24:38.9 -- not an asteroid (will add it to exclusion list)
20:47:51.49 +41:57:28.1 -- not an asteroid (will add it to exclusion list)
20:53:21.23 +42:19:15.9 -- not an asteroid (will add it to exclusion list)
20:40:58.64 +43:27:45.7 -- not an asteroid (will add it to exclusion list)
20:46:54.96 +42:39:27.0 -- not an asteroid (will add it to exclusion list)
20:46:00.19 +42:18:21.6 -- not an asteroid (will add it to exclusion list)
20:37:34.46 +43:31:51.0 -- not an asteroid (will add it to exclusion list)
20:43:30.49 +42:12:43.6 -- not an asteroid (will add it to exclusion list)
20:45:20.32 +42:15:12.9 -- not an asteroid (will add it to exclusion list)
20:44:28.34 +42:14:08.7 -- not an asteroid (will add it to exclusion list)
20:15:17.99 +46:27:35.3 -- not an asteroid (will add it to exclusion list)
20:50:43.06 +41:53:42.4 -- not an asteroid (will add it to exclusion list)
20:51:01.65 +41:37:20.3 -- not an asteroid (will add it to exclusion list)
20:43:22.33 +42:52:06.8 -- not an asteroid (will add it to exclusion list)
20:42:32.70 +44:14:46.6 -- not an asteroid (will add it to exclusion list)
20:41:43.82 +43:06:18.7 -- not an asteroid (will add it to exclusion list)
20:45:07.57 +41:35:23.8 -- not an asteroid (will add it to exclusion list)
20:43:13.54 +42:22:47.0 -- not an asteroid (will add it to exclusion list)
20:48:47.96 +42:14:18.9 -- not an asteroid (will add it to exclusion list)
20:42:18.04 +42:34:26.4 -- not an asteroid (will add it to exclusion list)
20:38:30.98 +42:40:59.5 -- not an asteroid (will add it to exclusion list)
20:46:01.52 +42:17:52.8 -- not an asteroid (will add it to exclusion list)
20:49:49.81 +42:25:12.6 -- not an asteroid (will add it to exclusion list)
20:41:36.24 +42:29:14.6 -- not an asteroid (will add it to exclusion list)
20:51:18.70 +41:45:29.5 -- not an asteroid (will add it to exclusion list)
20:40:29.54 +44:41:45.8 -- not an asteroid (will add it to exclusion list)
20:41:08.20 +44:26:50.2 -- not an asteroid (will add it to exclusion list)
20:40:33.71 +42:33:42.3 -- not an asteroid (will add it to exclusion list)
20:51:30.68 +41:32:16.3 -- not an asteroid (will add it to exclusion list)
20:43:39.89 +43:49:55.4 -- not an asteroid (will add it to exclusion list)
20:48:29.57 +41:29:14.6 -- not an asteroid (will add it to exclusion list)
20:43:37.19 +42:26:25.2 -- not an asteroid (will add it to exclusion list)
20:48:41.07 +41:49:47.2 -- not an asteroid (will add it to exclusion list)
20:50:03.95 +43:00:11.4 -- not an asteroid (will add it to exclusion list)
20:50:58.16 +42:36:05.0 -- not an asteroid (will add it to exclusion list)
20:50:03.84 +41:50:52.3 -- not an asteroid (will add it to exclusion list)
20:47:51.50 +41:24:19.2 -- not an asteroid (will add it to exclusion list)
20:50:00.64 +42:58:09.8 -- not an asteroid (will add it to exclusion list)
20:47:09.04 +41:59:16.3 -- not an asteroid (will add it to exclusion list)
20:46:13.93 +43:12:46.4 -- not an asteroid (will add it to exclusion list)
20:46:39.35 +41:43:16.8 -- not an asteroid (will add it to exclusion list)
20:41:41.09 +42:37:35.5 -- not an asteroid (will add it to exclusion list)
20:41:21.14 +44:32:39.7 -- not an asteroid (will add it to exclusion list)
20:41:28.21 +42:27:29.9 -- not an asteroid (will add it to exclusion list)
20:41:32.33 +44:30:23.9 -- not an asteroid (will add it to exclusion list)
20:52:14.80 +41:10:34.8 -- not an asteroid (will add it to exclusion list)
20:53:16.86 +42:09:03.0 -- not an asteroid (will add it to exclusion list)
20:45:12.41 +42:41:22.6 -- not an asteroid (will add it to exclusion list)
20:41:20.73 +44:26:46.9 -- not an asteroid (will add it to exclusion list)
20:51:55.06 +41:15:59.2 -- not an asteroid (will add it to exclusion list)
20:50:01.41 +41:46:18.5 -- not an asteroid (will add it to exclusion list)
20:42:53.48 +41:50:22.5 -- not an asteroid (will add it to exclusion list)
20:44:43.68 +42:20:56.9 -- not an asteroid (will add it to exclusion list)
20:48:08.95 +41:10:32.1 -- not an asteroid (will add it to exclusion list)
20:43:03.84 +42:25:15.8 -- not an asteroid (will add it to exclusion list)
20:48:59.55 +41:55:26.5 -- not an asteroid (will add it to exclusion list)
20:40:04.49 +42:45:08.1 -- not an asteroid (will add it to exclusion list)
20:45:17.66 +43:13:15.4 -- not an asteroid (will add it to exclusion list)
20:38:49.39 +42:29:54.2 -- not an asteroid (will add it to exclusion list)
20:42:33.74 +42:03:31.4 -- not an asteroid (will add it to exclusion list)
20:40:42.64 +42:10:43.2 -- not an asteroid (will add it to exclusion list)
20:53:06.23 +42:24:01.2 -- not an asteroid (will add it to exclusion list)
20:52:53.29 +40:41:38.1 -- not an asteroid (will add it to exclusion list)
20:48:03.25 +41:34:59.4 -- not an asteroid (will add it to exclusion list)
20:41:50.65 +42:22:13.8 -- not an asteroid (will add it to exclusion list)
20:50:20.20 +41:52:25.6 -- not an asteroid (will add it to exclusion list)
20:44:05.94 +41:49:10.2 -- not an asteroid (will add it to exclusion list)
20:46:22.01 +41:40:26.4 -- not an asteroid (will add it to exclusion list)
20:50:51.21 +42:25:34.6 -- not an asteroid (will add it to exclusion list)
20:41:04.28 +42:41:02.7 -- not an asteroid (will add it to exclusion list)
20:51:39.83 +40:52:41.3 -- not an asteroid (will add it to exclusion list)
20:18:26.77 +45:24:20.3 -- not an asteroid (will add it to exclusion list)
20:43:55.84 +42:11:44.3 -- not an asteroid (will add it to exclusion list)
20:44:24.85 +42:29:04.4 -- not an asteroid (will add it to exclusion list)
20:47:40.50 +41:05:32.6 -- not an asteroid (will add it to exclusion list)
20:15:48.73 +46:33:24.4 -- not an asteroid (will add it to exclusion list)
20:51:09.00 +42:28:31.3 -- not an asteroid (will add it to exclusion list)
20:55:43.79 +41:47:35.7 -- not an asteroid (will add it to exclusion list)
20:45:36.47 +42:13:42.1 -- not an asteroid (will add it to exclusion list)
20:47:24.57 +42:53:04.9 -- not an asteroid (will add it to exclusion list)
20:50:40.96 +41:38:00.9 -- not an asteroid (will add it to exclusion list)
20:49:06.85 +41:49:21.7 -- not an asteroid (will add it to exclusion list)
20:48:57.73 +41:55:54.9 -- not an asteroid (will add it to exclusion list)
20:48:16.50 +42:38:47.2 -- not an asteroid (will add it to exclusion list)
20:41:24.25 +42:18:49.5 -- not an asteroid (will add it to exclusion list)
20:46:23.97 +42:06:23.3 -- not an asteroid (will add it to exclusion list)
20:48:25.24 +40:51:06.1 -- not an asteroid (will add it to exclusion list)
20:48:40.13 +41:50:15.6 -- not an asteroid (will add it to exclusion list)
20:43:46.66 +42:54:51.7 -- not an asteroid (will add it to exclusion list)
20:48:58.68 +42:34:19.3 -- not an asteroid (will add it to exclusion list)
20:50:59.21 +42:44:17.0 -- not an asteroid (will add it to exclusion list)
20:42:04.38 +42:27:06.1 -- not an asteroid (will add it to exclusion list)
20:45:44.41 +42:18:37.9 -- not an asteroid (will add it to exclusion list)
20:41:41.21 +42:49:09.8 -- not an asteroid (will add it to exclusion list)
20:45:37.47 +41:41:31.9 -- not an asteroid (will add it to exclusion list)
20:42:44.26 +41:52:40.5 -- not an asteroid (will add it to exclusion list)
20:53:10.61 +42:23:32.5 -- not an asteroid (will add it to exclusion list)
20:42:40.42 +42:27:08.9 -- not an asteroid (will add it to exclusion list)
20:41:31.87 +42:30:25.9 -- not an asteroid (will add it to exclusion list)
20:36:47.07 +43:29:11.2 -- not an asteroid (will add it to exclusion list)
20:49:37.78 +41:08:54.5 -- not an asteroid (will add it to exclusion list)
20:41:43.19 +43:03:05.0 -- not an asteroid (will add it to exclusion list)
20:47:06.59 +42:38:55.8 -- not an asteroid (will add it to exclusion list)
20:45:00.48 +41:37:55.1 -- not an asteroid (will add it to exclusion list)
20:50:35.07 +40:46:12.4 -- not an asteroid (will add it to exclusion list)
20:40:18.24 +43:16:36.7 -- not an asteroid (will add it to exclusion list)
20:49:51.50 +41:48:17.7 -- not an asteroid (will add it to exclusion list)
20:46:10.36 +43:04:35.2 -- not an asteroid (will add it to exclusion list)
20:47:42.36 +42:15:51.3 -- not an asteroid (will add it to exclusion list)
20:51:43.40 +41:15:39.2 -- not an asteroid (will add it to exclusion list)
20:42:12.27 +41:52:14.3 -- not an asteroid (will add it to exclusion list)
20:50:28.78 +41:56:06.7 -- not an asteroid (will add it to exclusion list)
20:49:35.86 +42:22:16.8 -- not an asteroid (will add it to exclusion list)
20:48:36.18 +41:52:31.9 -- not an asteroid (will add it to exclusion list)
20:41:13.45 +44:38:12.3 -- not an asteroid (will add it to exclusion list)
20:45:42.96 +42:00:25.1 -- not an asteroid (will add it to exclusion list)
20:50:48.69 +41:48:13.7 -- not an asteroid (will add it to exclusion list)
20:51:14.23 +42:16:58.7 -- not an asteroid (will add it to exclusion list)
20:41:29.08 +42:32:38.2 -- not an asteroid (will add it to exclusion list)
20:41:18.00 +42:10:57.5 -- not an asteroid (will add it to exclusion list)
20:40:57.66 +42:37:51.9 -- not an asteroid (will add it to exclusion list)
20:42:57.95 +43:34:25.0 -- not an asteroid (will add it to exclusion list)
20:52:50.35 +40:47:52.5 -- not an asteroid (will add it to exclusion list)
20:42:13.97 +43:07:33.8 -- not an asteroid (will add it to exclusion list)
20:45:30.80 +42:09:03.0 -- not an asteroid (will add it to exclusion list)
20:53:37.73 +41:50:07.6 -- not an asteroid (will add it to exclusion list)
20:51:51.20 +41:31:29.8 -- not an asteroid (will add it to exclusion list)
20:47:00.83 +41:57:50.4 -- not an asteroid (will add it to exclusion list)
20:41:04.52 +42:38:07.3 -- not an asteroid (will add it to exclusion list)
20:44:14.98 +42:07:12.8 -- not an asteroid (will add it to exclusion list)
20:52:12.43 +42:00:58.9 -- not an asteroid (will add it to exclusion list)
20:54:35.22 +42:34:50.3 -- not an asteroid (will add it to exclusion list)
20:44:19.10 +41:55:48.8 -- not an asteroid (will add it to exclusion list)
20:47:26.96 +42:43:10.6 -- not an asteroid (will add it to exclusion list)
20:44:31.32 +41:39:26.4 -- not an asteroid (will add it to exclusion list)
20:53:00.18 +42:36:15.5 -- not an asteroid (will add it to exclusion list)
20:48:09.51 +41:43:30.3 -- not an asteroid (will add it to exclusion list)
20:40:30.87 +42:46:56.2 -- not an asteroid (will add it to exclusion list)
20:45:22.25 +42:29:22.1 -- not an asteroid (will add it to exclusion list)
20:39:24.63 +44:43:29.3 -- not an asteroid (will add it to exclusion list)
20:51:33.96 +41:04:35.6 -- not an asteroid (will add it to exclusion list)
20:51:11.95 +42:42:18.7 -- not an asteroid (will add it to exclusion list)
20:41:10.32 +44:09:31.8 -- not an asteroid (will add it to exclusion list)
20:49:46.03 +42:08:00.9 -- not an asteroid (will add it to exclusion list)
20:53:29.11 +42:10:19.8 -- not an asteroid (will add it to exclusion list)
20:46:54.24 +41:21:48.9 -- not an asteroid (will add it to exclusion list)
20:44:38.55 +42:21:56.0 -- not an asteroid (will add it to exclusion list)
20:46:14.81 +40:46:43.6 -- not an asteroid (will add it to exclusion list)
20:47:08.92 +42:14:20.3 -- not an asteroid (will add it to exclusion list)
20:44:39.24 +42:00:53.6 -- not an asteroid (will add it to exclusion list)
20:46:35.79 +42:30:17.7 -- not an asteroid (will add it to exclusion list)
20:54:30.76 +41:50:56.2 -- not an asteroid (will add it to exclusion list)
20:52:47.87 +41:59:28.7 -- not an asteroid (will add it to exclusion list)
20:49:31.65 +41:57:07.4 -- not an asteroid (will add it to exclusion list)
20:38:29.33 +42:32:11.1 -- not an asteroid (will add it to exclusion list)
20:46:34.17 +42:50:10.4 -- not an asteroid (will add it to exclusion list)
20:52:59.23 +40:57:24.1 -- not an asteroid (will add it to exclusion list)
20:50:57.06 +41:54:30.1 -- not an asteroid (will add it to exclusion list)
20:48:57.94 +41:03:20.8 -- not an asteroid (will add it to exclusion list)
20:52:05.62 +42:28:27.9 -- not an asteroid (will add it to exclusion list)
20:43:52.11 +42:24:05.9 -- not an asteroid (will add it to exclusion list)
20:46:57.10 +40:59:06.4 -- not an asteroid (will add it to exclusion list)
20:51:38.47 +42:34:34.4 -- not an asteroid (will add it to exclusion list)
20:39:21.47 +42:59:33.2 -- not an asteroid (will add it to exclusion list)
20:42:18.15 +42:50:32.1 -- not an asteroid (will add it to exclusion list)
20:41:33.41 +42:27:22.5 -- not an asteroid (will add it to exclusion list)
20:51:51.65 +41:52:04.8 -- not an asteroid (will add it to exclusion list)
20:42:46.37 +41:56:29.2 -- not an asteroid (will add it to exclusion list)
20:47:27.94 +42:57:38.2 -- not an asteroid (will add it to exclusion list)
20:49:44.05 +41:51:30.8 -- not an asteroid (will add it to exclusion list)
20:40:15.41 +43:47:43.5 -- not an asteroid (will add it to exclusion list)
20:43:45.89 +42:26:49.2 -- not an asteroid (will add it to exclusion list)
20:54:02.41 +42:06:27.6 -- not an asteroid (will add it to exclusion list)
20:45:12.88 +43:03:09.7 -- not an asteroid (will add it to exclusion list)
20:38:52.74 +42:28:01.6 -- not an asteroid (will add it to exclusion list)
20:41:21.08 +43:27:15.4 -- not an asteroid (will add it to exclusion list)
20:42:22.22 +44:28:53.4 -- not an asteroid (will add it to exclusion list)
20:44:46.86 +41:53:09.3 -- not an asteroid (will add it to exclusion list)
20:49:30.68 +41:11:17.7 -- not an asteroid (will add it to exclusion list)
20:53:43.21 +41:52:38.1 -- not an asteroid (will add it to exclusion list)
20:48:33.09 +41:42:36.7 -- not an asteroid (will add it to exclusion list)
20:52:31.41 +41:34:07.8 -- not an asteroid (will add it to exclusion list)
20:35:49.43 +43:55:31.6 -- not an asteroid (will add it to exclusion list)
20:54:29.35 +42:05:12.8 -- not an asteroid (will add it to exclusion list)
20:40:03.89 +42:25:12.7 -- not an asteroid (will add it to exclusion list)
20:46:07.80 +43:06:31.8 -- not an asteroid (will add it to exclusion list)
20:51:22.15 +41:47:39.9 -- not an asteroid (will add it to exclusion list)
20:51:15.82 +41:26:13.7 -- not an asteroid (will add it to exclusion list)
20:48:26.11 +42:07:56.8 -- not an asteroid (will add it to exclusion list)
20:54:12.96 +41:57:07.9 -- not an asteroid (will add it to exclusion list)
20:51:12.93 +40:44:12.7 -- not an asteroid (will add it to exclusion list)
20:40:53.22 +43:18:20.9 -- not an asteroid (will add it to exclusion list)
20:44:27.01 +41:46:44.9 -- not an asteroid (will add it to exclusion list)
20:53:24.99 +42:30:38.5 -- not an asteroid (will add it to exclusion list)
20:50:43.19 +42:15:26.8 -- not an asteroid (will add it to exclusion list)
20:53:10.15 +40:52:40.3 -- not an asteroid (will add it to exclusion list)
20:47:43.59 +41:31:42.6 -- not an asteroid (will add it to exclusion list)
20:43:56.21 +43:55:58.2 -- not an asteroid (will add it to exclusion list)
20:46:59.57 +42:40:45.8 -- not an asteroid (will add it to exclusion list)
20:47:44.97 +41:43:20.9 -- not an asteroid (will add it to exclusion list)
20:46:12.54 +42:59:23.5 -- not an asteroid (will add it to exclusion list)
20:45:49.52 +42:03:56.3 -- not an asteroid (will add it to exclusion list)
20:41:19.77 +42:24:44.6 -- not an asteroid (will add it to exclusion list)
20:42:00.63 +43:18:43.4 -- not an asteroid (will add it to exclusion list)
20:39:49.84 +44:27:58.5 -- not an asteroid (will add it to exclusion list)
20:40:41.72 +42:13:22.5 -- not an asteroid (will add it to exclusion list)
20:50:44.32 +41:29:51.2 -- not an asteroid (will add it to exclusion list)
20:50:55.68 +41:40:20.2 -- not an asteroid (will add it to exclusion list)
20:46:47.72 +41:26:14.2 -- not an asteroid (will add it to exclusion list)
20:41:21.37 +44:41:30.9 -- not an asteroid (will add it to exclusion list)
20:43:41.55 +41:54:54.4 -- not an asteroid (will add it to exclusion list)
20:51:46.20 +42:27:04.2 -- not an asteroid (will add it to exclusion list)
20:55:11.39 +41:51:15.9 -- not an asteroid (will add it to exclusion list)
20:39:42.16 +44:42:30.0 -- not an asteroid (will add it to exclusion list)
20:46:49.32 +41:46:10.9 -- not an asteroid (will add it to exclusion list)
20:52:24.43 +41:47:43.8 -- not an asteroid (will add it to exclusion list)
20:44:32.93 +42:35:57.7 -- not an asteroid (will add it to exclusion list)
20:46:52.82 +42:08:59.4 -- not an asteroid (will add it to exclusion list)
20:51:34.31 +41:25:45.5 -- not an asteroid (will add it to exclusion list)
20:42:44.73 +43:05:28.7 -- not an asteroid (will add it to exclusion list)
20:45:56.57 +42:06:28.5 -- not an asteroid (will add it to exclusion list)
20:49:40.33 +41:56:56.1 -- not an asteroid (will add it to exclusion list)
20:40:20.93 +44:51:23.4 -- not an asteroid (will add it to exclusion list)
20:38:27.91 +44:52:05.0 -- not an asteroid (will add it to exclusion list)
20:50:58.70 +40:53:04.7 -- not an asteroid (will add it to exclusion list)
20:52:37.80 +42:26:09.8 -- not an asteroid (will add it to exclusion list)
20:39:36.02 +43:14:22.3 -- not an asteroid (will add it to exclusion list)
20:44:04.68 +41:55:28.6 -- not an asteroid (will add it to exclusion list)
20:44:50.38 +42:16:37.9 -- not an asteroid (will add it to exclusion list)
20:40:49.30 +42:15:44.3 -- not an asteroid (will add it to exclusion list)
20:43:07.37 +42:09:28.8 -- not an asteroid (will add it to exclusion list)
20:44:48.18 +42:08:14.9 -- not an asteroid (will add it to exclusion list)
20:53:03.69 +41:49:10.1 -- not an asteroid (will add it to exclusion list)
20:52:20.78 +41:13:49.7 -- not an asteroid (will add it to exclusion list)
20:46:35.38 +41:45:42.9 -- not an asteroid (will add it to exclusion list)
20:44:33.34 +42:17:07.7 -- not an asteroid (will add it to exclusion list)
20:42:36.34 +42:07:28.5 -- not an asteroid (will add it to exclusion list)
20:51:39.99 +41:32:07.9 -- not an asteroid (will add it to exclusion list)
20:53:20.07 +40:55:15.5 -- not an asteroid (will add it to exclusion list)
20:47:49.80 +41:49:50.9 -- not an asteroid (will add it to exclusion list)
20:47:24.60 +42:03:13.0 -- not an asteroid (will add it to exclusion list)
20:48:20.10 +41:34:04.5 -- not an asteroid (will add it to exclusion list)
20:52:19.42 +40:55:30.8 -- not an asteroid (will add it to exclusion list)
20:46:35.19 +41:48:06.3 -- not an asteroid (will add it to exclusion list)
20:47:16.87 +42:08:43.6 -- not an asteroid (will add it to exclusion list)
20:40:11.15 +43:06:56.4 -- not an asteroid (will add it to exclusion list)
20:52:09.04 +41:23:26.5 -- not an asteroid (will add it to exclusion list)
20:46:07.15 +42:55:13.0 -- not an asteroid (will add it to exclusion list)
20:46:58.63 +41:45:50.4 -- not an asteroid (will add it to exclusion list)
20:44:11.30 +42:12:06.7 -- not an asteroid (will add it to exclusion list)
20:49:07.30 +41:22:59.3 -- not an asteroid (will add it to exclusion list)
20:50:54.46 +41:52:21.5 -- not an asteroid (will add it to exclusion list)
20:41:24.50 +42:17:34.0 -- not an asteroid (will add it to exclusion list)
20:14:23.88 +46:37:02.0 -- not an asteroid (will add it to exclusion list)
20:54:56.46 +41:51:14.0 -- not an asteroid (will add it to exclusion list)
20:48:31.23 +41:23:11.9 -- not an asteroid (will add it to exclusion list)
20:47:32.84 +41:59:43.0 -- not an asteroid (will add it to exclusion list)
20:50:12.98 +40:51:23.3 -- not an asteroid (will add it to exclusion list)
20:41:35.52 +42:36:03.5 -- not an asteroid (will add it to exclusion list)
20:46:10.51 +41:33:21.8 -- not an asteroid (will add it to exclusion list)
20:42:49.44 +42:23:11.6 -- not an asteroid (will add it to exclusion list)
20:40:46.38 +42:33:32.9 -- not an asteroid (will add it to exclusion list)
20:52:52.53 +40:56:00.1 -- not an asteroid (will add it to exclusion list)
20:46:17.49 +43:09:28.2 -- not an asteroid (will add it to exclusion list)
20:52:38.81 +41:37:21.4 -- not an asteroid (will add it to exclusion list)
20:52:54.02 +42:18:36.1 -- not an asteroid (will add it to exclusion list)
20:38:16.84 +45:09:49.9 -- not an asteroid (will add it to exclusion list)
20:48:53.16 +41:45:58.7 -- not an asteroid (will add it to exclusion list)
20:46:05.41 +42:04:52.9 -- not an asteroid (will add it to exclusion list)
20:50:57.25 +42:45:47.6 -- not an asteroid (will add it to exclusion list)
20:48:44.85 +41:51:16.3 -- not an asteroid (will add it to exclusion list)
20:48:11.25 +40:49:58.8 -- not an asteroid (will add it to exclusion list)
20:51:17.62 +40:59:40.5 -- not an asteroid (will add it to exclusion list)
20:41:38.46 +42:24:32.1 -- not an asteroid (will add it to exclusion list)
20:40:39.90 +44:46:33.9 -- not an asteroid (will add it to exclusion list)
20:54:22.30 +41:59:16.1 -- not an asteroid (will add it to exclusion list)
20:46:00.97 +42:22:19.4 -- not an asteroid (will add it to exclusion list)
20:40:11.55 +43:12:14.3 -- not an asteroid (will add it to exclusion list)
20:51:48.65 +41:17:21.2 -- not an asteroid (will add it to exclusion list)
20:50:02.38 +42:32:06.5 -- not an asteroid (will add it to exclusion list)
20:45:41.34 +42:11:18.0 -- not an asteroid (will add it to exclusion list)
20:50:05.22 +42:03:00.0 -- not an asteroid (will add it to exclusion list)
20:45:43.04 +42:19:20.1 -- not an asteroid (will add it to exclusion list)
20:53:37.43 +42:32:29.4 -- not an asteroid (will add it to exclusion list)
20:44:04.70 +42:18:35.7 -- not an asteroid (will add it to exclusion list)
20:52:14.50 +41:34:58.4 -- not an asteroid (will add it to exclusion list)
20:56:11.88 +42:36:06.1 -- not an asteroid (will add it to exclusion list)
20:43:27.31 +42:14:35.9 -- not an asteroid (will add it to exclusion list)
20:41:21.77 +44:39:58.7 -- not an asteroid (will add it to exclusion list)
20:47:52.66 +42:21:25.5 -- not an asteroid (will add it to exclusion list)
20:37:28.44 +43:21:45.0 -- not an asteroid (will add it to exclusion list)
20:47:36.07 +41:57:04.7 -- not an asteroid (will add it to exclusion list)
20:43:50.53 +41:58:52.6 -- not an asteroid (will add it to exclusion list)
20:47:33.81 +42:06:42.9 -- not an asteroid (will add it to exclusion list)
20:48:34.51 +41:28:44.8 -- not an asteroid (will add it to exclusion list)
20:53:54.47 +42:24:53.1 -- not an asteroid (will add it to exclusion list)
20:47:47.62 +42:36:22.9 -- not an asteroid (will add it to exclusion list)
20:45:44.30 +43:09:42.4 -- not an asteroid (will add it to exclusion list)
20:44:04.13 +44:00:50.1 -- not an asteroid (will add it to exclusion list)
20:39:03.16 +44:46:47.9 -- not an asteroid (will add it to exclusion list)
20:49:43.24 +41:48:30.8 -- not an asteroid (will add it to exclusion list)
20:40:37.73 +42:45:48.6 -- not an asteroid (will add it to exclusion list)
20:44:17.75 +42:14:55.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:13:29.19 +46:38:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:23.88 +46:37:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:58.75 +45:49:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:17.99 +46:27:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:48.73 +46:33:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:26.77 +45:24:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:36.71 +45:08:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:34:39.22 +44:00:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:35:49.43 +43:55:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:36:47.07 +43:29:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:28.44 +43:21:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:37:34.46 +43:31:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:16.84 +45:09:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:25.48 +43:01:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:27.91 +44:52:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:29.33 +42:32:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:29.43 +45:07:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:30.98 +42:40:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:49.39 +42:29:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:52.74 +42:28:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:03.16 +44:46:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:14.40 +42:36:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:21.47 +42:59:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:24.63 +44:43:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:25.17 +42:56:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:29.97 +42:21:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:36.02 +43:14:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:41.40 +44:46:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:41.84 +42:39:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:42.16 +44:42:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:49.84 +44:27:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:55.86 +44:31:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:56.24 +42:13:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:59.71 +43:51:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:03.89 +42:25:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:04.49 +42:45:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:09.79 +42:57:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:11.15 +43:06:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:11.51 +42:24:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:11.55 +43:12:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:15.41 +43:47:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:18.24 +43:16:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:18.25 +44:40:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:20.93 +44:51:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:26.66 +44:31:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:29.54 +44:41:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:30.87 +42:46:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:33.71 +42:33:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:37.73 +42:45:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:38.00 +43:31:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:39.24 +42:33:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:39.90 +44:46:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:41.72 +42:13:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:42.64 +42:10:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:46.38 +42:33:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:48.41 +44:40:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:49.30 +42:15:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:53.22 +43:18:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:56.22 +42:27:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:57.66 +42:37:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:40:58.64 +43:27:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:04.28 +42:41:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:04.52 +42:38:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:05.93 +42:24:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:06.41 +42:57:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:07.89 +42:34:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:08.20 +44:26:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:10.32 +44:09:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:13.45 +44:38:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:18.00 +42:10:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:19.77 +42:24:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:20.73 +44:26:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:20.93 +42:27:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:21.08 +43:27:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:21.14 +44:32:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:21.37 +44:41:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:21.77 +44:39:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:24.25 +42:18:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:24.50 +42:17:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:28.21 +42:27:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:29.08 +42:32:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:29.42 +42:25:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:31.87 +42:30:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:32.33 +44:30:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:33.41 +42:27:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:35.52 +42:36:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:36.24 +42:29:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:37.97 +42:32:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:38.46 +42:24:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:38.95 +42:20:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:41.09 +42:37:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:41.21 +42:49:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:42.50 +42:28:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:43.19 +43:03:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:43.44 +42:26:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:43.82 +43:06:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:50.65 +42:22:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:52.91 +42:11:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:00.63 +43:18:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:04.38 +42:27:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:10.39 +42:37:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:12.27 +41:52:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:13.97 +43:07:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:16.86 +43:17:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:18.04 +42:34:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:18.15 +42:50:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:22.22 +44:28:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:23.84 +42:34:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:32.70 +44:14:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:33.74 +42:03:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:36.34 +42:07:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:40.42 +42:27:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:44.26 +41:52:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:44.73 +43:05:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:46.37 +41:56:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:49.40 +44:11:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:49.44 +42:23:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:51.54 +42:09:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:53.48 +41:50:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:56.03 +41:57:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:57.95 +43:34:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:03.84 +42:25:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:06.16 +42:25:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:07.37 +42:09:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:13.54 +42:22:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:22.33 +42:52:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:27.31 +42:14:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:28.61 +42:08:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:30.49 +42:12:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:32.97 +41:50:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:37.19 +42:26:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:39.89 +43:49:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:41.55 +41:54:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:43.35 +42:21:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:45.89 +42:26:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:46.66 +42:54:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:48.63 +42:00:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:48.81 +42:30:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:50.53 +41:58:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:52.11 +42:24:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:55.84 +42:11:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:56.21 +43:55:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:56.67 +42:25:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:04.13 +44:00:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:04.68 +41:55:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:04.70 +42:18:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:05.30 +42:26:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:05.94 +41:49:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:11.30 +42:12:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:14.98 +42:07:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:17.75 +42:14:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:19.10 +41:55:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:24.85 +42:29:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:27.01 +41:46:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:28.34 +42:14:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:31.32 +41:39:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:32.41 +44:01:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:32.93 +42:35:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:33.34 +42:17:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:38.24 +41:42:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:38.55 +42:21:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:39.24 +42:00:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:43.68 +42:20:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:46.86 +41:53:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:48.18 +42:08:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:50.38 +42:16:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:00.48 +41:37:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:07.57 +41:35:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:12.41 +42:41:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:12.88 +43:03:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:17.66 +43:13:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:20.32 +42:15:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:22.25 +42:29:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:30.80 +42:09:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:32.53 +42:12:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:36.47 +42:13:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:37.47 +41:41:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:41.34 +42:11:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:42.96 +42:00:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:43.04 +42:19:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:44.30 +43:09:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:44.41 +42:18:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:49.52 +42:03:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:56.57 +42:06:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:00.19 +42:18:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:00.97 +42:22:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:01.52 +42:17:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:05.41 +42:04:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:07.15 +42:55:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:07.80 +43:06:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:10.36 +43:04:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:10.51 +41:33:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:12.54 +42:59:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:13.93 +43:12:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:14.81 +40:46:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:17.49 +43:09:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:19.49 +42:59:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:22.01 +41:40:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:23.97 +42:06:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:30.43 +42:01:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:34.17 +42:50:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:35.19 +41:48:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:35.38 +41:45:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:35.79 +42:30:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:39.35 +41:43:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:43.86 +42:59:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:47.72 +41:26:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:48.48 +41:08:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:49.32 +41:46:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:52.82 +42:08:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:54.24 +41:21:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:54.96 +42:39:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:56.69 +43:01:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:57.01 +42:21:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:57.10 +40:59:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:58.63 +41:45:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:59.57 +42:40:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:00.83 +41:57:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:01.36 +41:37:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:03.33 +42:47:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:05.03 +41:46:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:06.59 +42:38:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:08.92 +42:14:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:09.04 +41:59:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:16.87 +42:08:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:19.26 +41:40:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:24.57 +42:53:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:24.60 +42:03:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:25.54 +42:21:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:26.96 +42:43:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:27.94 +42:57:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:32.84 +41:59:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:33.81 +42:06:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:36.07 +41:57:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:40.50 +41:05:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:42.36 +42:15:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:43.59 +41:31:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:44.97 +41:43:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:47.62 +42:36:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:49.80 +41:49:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:51.49 +41:57:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:51.50 +41:24:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:52.66 +42:21:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:59.59 +42:39:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:01.31 +41:18:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:03.25 +41:34:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:06.75 +42:21:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:08.95 +41:10:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:09.51 +41:43:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:11.22 +41:08:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:11.25 +40:49:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:13.02 +42:09:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:16.50 +42:38:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:18.79 +41:48:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:20.10 +41:34:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:23.46 +41:52:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:25.24 +40:51:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:26.11 +42:07:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:29.57 +41:29:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:31.23 +41:23:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:32.20 +41:37:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:33.09 +41:42:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:34.51 +41:28:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:36.18 +41:52:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:39.23 +41:57:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:40.13 +41:50:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:41.07 +41:49:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:44.85 +41:51:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:47.05 +41:32:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:47.96 +42:14:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:53.16 +41:45:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:53.30 +41:48:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:54.03 +41:43:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:54.68 +41:52:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:57.73 +41:55:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:57.94 +41:03:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:58.68 +42:34:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:59.55 +41:55:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:06.85 +41:49:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:07.30 +41:22:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:14.17 +41:58:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:24.04 +41:41:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:30.68 +41:11:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:31.65 +41:57:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:35.86 +42:22:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:37.78 +41:08:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:38.36 +41:42:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:39.00 +41:39:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:40.33 +41:56:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:43.24 +41:48:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:44.05 +41:51:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:44.10 +42:13:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:46.03 +42:08:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:46.94 +42:22:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:49.81 +42:25:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:51.50 +41:48:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:00.64 +42:58:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:01.41 +41:46:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:02.38 +42:32:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:03.84 +41:50:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:03.95 +43:00:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:04.64 +42:18:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:05.22 +42:03:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:11.34 +41:48:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:12.98 +40:51:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:20.20 +41:52:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:20.72 +41:43:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:25.72 +41:47:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:28.78 +41:56:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:35.07 +40:46:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:40.96 +41:38:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:41.16 +41:48:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:43.06 +41:53:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:43.19 +42:15:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:43.74 +42:05:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:44.32 +41:29:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:48.69 +41:48:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:51.21 +42:25:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:51.53 +41:43:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:53.04 +40:56:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:54.46 +41:52:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:55.68 +41:40:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:57.06 +41:54:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:57.25 +42:45:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:58.16 +42:36:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:58.70 +40:53:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:59.21 +42:44:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:01.65 +41:37:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:02.18 +41:32:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:03.76 +42:29:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:05.07 +41:46:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:09.00 +42:28:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:09.25 +41:37:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:11.95 +42:42:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:12.93 +40:44:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:14.23 +42:16:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:15.82 +41:26:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:17.31 +41:50:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:17.62 +40:59:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:18.70 +41:45:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:19.07 +41:55:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:22.15 +41:47:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:27.24 +41:34:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:27.41 +41:53:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:30.68 +41:32:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:33.96 +41:04:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:34.31 +41:25:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:38.47 +42:34:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:39.83 +40:52:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:39.99 +41:32:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:43.40 +41:15:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:46.14 +41:34:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:46.20 +42:27:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:48.65 +41:17:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:49.86 +41:28:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:51.20 +41:31:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:51.65 +41:52:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:55.06 +41:15:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:56.14 +41:55:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:57.23 +42:20:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:05.62 +42:28:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:06.36 +42:31:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:09.04 +41:23:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:11.10 +40:52:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:12.43 +42:00:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:14.50 +41:34:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:14.80 +41:10:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:19.42 +40:55:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:20.78 +41:13:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:24.43 +41:47:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:26.11 +41:16:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:31.41 +41:34:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:37.80 +42:26:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:38.81 +41:37:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:47.87 +41:59:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:50.35 +40:47:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:51.60 +41:08:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:52.53 +40:56:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:53.29 +40:41:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:54.02 +42:18:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:59.23 +40:57:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:00.18 +42:36:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:03.69 +41:49:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:06.23 +42:24:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:10.15 +40:52:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:10.52 +42:10:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:10.61 +42:23:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:11.56 +42:31:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:16.86 +42:09:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:20.07 +40:55:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:21.23 +42:19:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:24.99 +42:30:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:29.11 +42:10:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:32.74 +42:14:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:37.43 +42:32:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:37.73 +41:50:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:43.21 +41:52:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:54.47 +42:24:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:00.19 +41:34:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:02.41 +42:06:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:12.96 +41:57:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:22.30 +41:59:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:29.35 +42:05:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:30.76 +41:50:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:35.22 +42:34:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:49.61 +41:53:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:56.46 +41:51:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:11.39 +41:51:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:43.79 +41:47:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:11.88 +42:36:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:08.83 +41:47:10.6 -- 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)
20:13:29.19 +46:38:35.5 -- a known variable star
20:14:23.88 +46:37:02.0 -- not a known variable star
20:14:58.75 +45:49:56.3 -- not a known variable star
20:15:17.99 +46:27:35.3 -- a known variable star
20:15:48.73 +46:33:24.4 -- not a known variable star
20:18:26.77 +45:24:20.3 -- not a known variable star
20:32:36.71 +45:08:02.4 -- a known variable star
20:34:39.22 +44:00:04.4 -- not a known variable star
20:35:49.43 +43:55:31.6 -- a known variable star
20:36:47.07 +43:29:11.2 -- a known variable star
20:37:28.44 +43:21:45.0 -- not a known variable star
20:37:34.46 +43:31:51.0 -- a known variable star
20:38:16.84 +45:09:49.9 -- not a known variable star
20:38:25.48 +43:01:53.3 -- a known variable star
20:38:27.91 +44:52:05.0 -- a known variable star
20:38:29.33 +42:32:11.1 -- not a known variable star
20:38:29.43 +45:07:16.0 -- not a known variable star
20:38:30.98 +42:40:59.5 -- not a known variable star
20:38:49.39 +42:29:54.2 -- not a known variable star
20:38:52.74 +42:28:01.6 -- not a known variable star
20:39:03.16 +44:46:47.9 -- not a known variable star
20:39:14.40 +42:36:13.9 -- not a known variable star
20:39:21.47 +42:59:33.2 -- a known variable star
20:39:24.63 +44:43:29.3 -- not a known variable star
20:39:25.17 +42:56:24.0 -- not a known variable star
20:39:29.97 +42:21:52.0 -- not a known variable star
20:39:36.02 +43:14:22.3 -- not a known variable star
20:39:41.40 +44:46:56.4 -- not a known variable star
20:39:41.84 +42:39:33.3 -- not a known variable star
20:39:42.16 +44:42:30.0 -- not a known variable star
20:39:49.84 +44:27:58.5 -- not a known variable star
20:39:55.86 +44:31:04.8 -- not a known variable star
20:39:56.24 +42:13:27.5 -- not a known variable star
20:39:59.71 +43:51:28.4 -- not a known variable star
20:40:03.89 +42:25:12.7 -- not a known variable star
20:40:04.49 +42:45:08.1 -- not a known variable star
20:40:09.79 +42:57:36.9 -- not a known variable star
20:40:11.15 +43:06:56.4 -- not a known variable star
20:40:11.51 +42:24:38.9 -- not a known variable star
20:40:11.55 +43:12:14.3 -- not a known variable star
20:40:15.41 +43:47:43.5 -- not a known variable star
20:40:18.24 +43:16:36.7 -- not a known variable star
20:40:18.25 +44:40:33.5 -- not a known variable star
20:40:20.93 +44:51:23.4 -- not a known variable star
20:40:26.66 +44:31:56.9 -- a known variable star
20:40:29.54 +44:41:45.8 -- not a known variable star
20:40:30.87 +42:46:56.2 -- a known variable star
20:40:33.71 +42:33:42.3 -- not a known variable star
20:40:37.73 +42:45:48.6 -- not a known variable star
20:40:38.00 +43:31:06.6 -- not a known variable star
20:40:39.24 +42:33:46.5 -- not a known variable star
20:40:39.90 +44:46:33.9 -- a known variable star
20:40:41.72 +42:13:22.5 -- not a known variable star
20:40:42.64 +42:10:43.2 -- not a known variable star
20:40:46.38 +42:33:32.9 -- a known variable star
20:40:48.41 +44:40:10.2 -- not a known variable star
20:40:49.30 +42:15:44.3 -- not a known variable star
20:40:53.22 +43:18:20.9 -- not a known variable star
20:40:56.22 +42:27:26.1 -- a known variable star
20:40:57.66 +42:37:51.9 -- not a known variable star
20:40:58.64 +43:27:45.7 -- a known variable star
20:41:04.28 +42:41:02.7 -- a known variable star
20:41:04.52 +42:38:07.3 -- not a known variable star
20:41:05.93 +42:24:42.0 -- not a known variable star
20:41:06.41 +42:57:17.8 -- not a known variable star
20:41:07.89 +42:34:21.4 -- not a known variable star
20:41:08.20 +44:26:50.2 -- not a known variable star
20:41:10.32 +44:09:31.8 -- not a known variable star
20:41:13.45 +44:38:12.3 -- not a known variable star
20:41:18.00 +42:10:57.5 -- a known variable star
20:41:19.77 +42:24:44.6 -- not a known variable star
20:41:20.73 +44:26:46.9 -- not a known variable star
20:41:20.93 +42:27:53.5 -- a known variable star
20:41:21.08 +43:27:15.4 -- not a known variable star
20:41:21.14 +44:32:39.7 -- not a known variable star
20:41:21.37 +44:41:30.9 -- not a known variable star
20:41:21.77 +44:39:58.7 -- a known variable star
20:41:24.25 +42:18:49.5 -- not a known variable star
20:41:24.50 +42:17:34.0 -- not a known variable star
20:41:28.21 +42:27:29.9 -- not a known variable star
20:41:29.08 +42:32:38.2 -- not a known variable star
20:41:29.42 +42:25:04.6 -- not a known variable star
20:41:31.87 +42:30:25.9 -- a known variable star
20:41:32.33 +44:30:23.9 -- not a known variable star
20:41:33.41 +42:27:22.5 -- not a known variable star
20:41:35.52 +42:36:03.5 -- not a known variable star
20:41:36.24 +42:29:14.6 -- not a known variable star
20:41:37.97 +42:32:55.5 -- not a known variable star
20:41:38.46 +42:24:32.1 -- not a known variable star
20:41:38.95 +42:20:53.0 -- a known variable star
20:41:41.09 +42:37:35.5 -- not a known variable star
20:41:41.21 +42:49:09.8 -- a known variable star
20:41:42.50 +42:28:19.1 -- not a known variable star
20:41:43.19 +43:03:05.0 -- not a known variable star
20:41:43.44 +42:26:21.8 -- not a known variable star
20:41:43.82 +43:06:18.7 -- a known variable star
20:41:50.65 +42:22:13.8 -- not a known variable star
20:41:52.91 +42:11:50.4 -- not a known variable star
20:42:00.63 +43:18:43.4 -- not a known variable star
20:42:04.38 +42:27:06.1 -- a known variable star
20:42:10.39 +42:37:32.6 -- not a known variable star
20:42:12.27 +41:52:14.3 -- not a known variable star
20:42:13.97 +43:07:33.8 -- not a known variable star
20:42:16.86 +43:17:16.3 -- not a known variable star
20:42:18.04 +42:34:26.4 -- not a known variable star
20:42:18.15 +42:50:32.1 -- not a known variable star
20:42:22.22 +44:28:53.4 -- a known variable star
20:42:23.84 +42:34:02.8 -- a known variable star
20:42:32.70 +44:14:46.6 -- not a known variable star
20:42:33.74 +42:03:31.4 -- not a known variable star
20:42:36.34 +42:07:28.5 -- not a known variable star
20:42:40.42 +42:27:08.9 -- not a known variable star
20:42:44.26 +41:52:40.5 -- a known variable star
20:42:44.73 +43:05:28.7 -- not a known variable star
20:42:46.37 +41:56:29.2 -- not a known variable star
20:42:49.40 +44:11:19.2 -- not a known variable star
20:42:49.44 +42:23:11.6 -- not a known variable star
20:42:51.54 +42:09:19.9 -- not a known variable star
20:42:53.48 +41:50:22.5 -- not a known variable star
20:42:56.03 +41:57:52.2 -- a known variable star
20:42:57.95 +43:34:25.0 -- not a known variable star
20:43:03.84 +42:25:15.8 -- a known variable star
20:43:06.16 +42:25:20.9 -- not a known variable star
20:43:07.37 +42:09:28.8 -- not a known variable star
20:43:13.54 +42:22:47.0 -- not a known variable star
20:43:22.33 +42:52:06.8 -- not a known variable star
20:43:27.31 +42:14:35.9 -- not a known variable star
20:43:28.61 +42:08:56.5 -- not a known variable star
20:43:30.49 +42:12:43.6 -- not a known variable star
20:43:32.97 +41:50:10.8 -- not a known variable star
20:43:37.19 +42:26:25.2 -- not a known variable star
20:43:39.89 +43:49:55.4 -- not a known variable star
20:43:41.55 +41:54:54.4 -- not a known variable star
20:43:43.35 +42:21:50.5 -- not a known variable star
20:43:45.89 +42:26:49.2 -- not a known variable star
20:43:46.66 +42:54:51.7 -- not a known variable star
20:43:48.63 +42:00:25.1 -- not a known variable star
20:43:48.81 +42:30:50.9 -- not a known variable star
20:43:50.53 +41:58:52.6 -- not a known variable star
20:43:52.11 +42:24:05.9 -- not a known variable star
20:43:55.84 +42:11:44.3 -- not a known variable star
20:43:56.21 +43:55:58.2 -- not a known variable star
20:43:56.67 +42:25:37.2 -- not a known variable star
20:44:04.13 +44:00:50.1 -- not a known variable star
20:44:04.68 +41:55:28.6 -- a known variable star
20:44:04.70 +42:18:35.7 -- not a known variable star
20:44:05.30 +42:26:28.8 -- not a known variable star
20:44:05.94 +41:49:10.2 -- not a known variable star
20:44:11.30 +42:12:06.7 -- not a known variable star
20:44:14.98 +42:07:12.8 -- a known variable star
20:44:17.75 +42:14:55.4 -- not a known variable star
20:44:19.10 +41:55:48.8 -- not a known variable star
20:44:24.85 +42:29:04.4 -- not a known variable star
20:44:27.01 +41:46:44.9 -- not a known variable star
20:44:28.34 +42:14:08.7 -- not a known variable star
20:44:31.32 +41:39:26.4 -- not a known variable star
20:44:32.41 +44:01:35.5 -- not a known variable star
20:44:32.93 +42:35:57.7 -- not a known variable star
20:44:33.34 +42:17:07.7 -- not a known variable star
20:44:38.24 +41:42:35.0 -- not a known variable star
20:44:38.55 +42:21:56.0 -- not a known variable star
20:44:39.24 +42:00:53.6 -- not a known variable star
20:44:43.68 +42:20:56.9 -- not a known variable star
20:44:46.86 +41:53:09.3 -- not a known variable star
20:44:48.18 +42:08:14.9 -- a known variable star
20:44:50.38 +42:16:37.9 -- not a known variable star
20:45:00.48 +41:37:55.1 -- a known variable star
20:45:07.57 +41:35:23.8 -- not a known variable star
20:45:12.41 +42:41:22.6 -- not a known variable star
20:45:12.88 +43:03:09.7 -- not a known variable star
20:45:17.66 +43:13:15.4 -- not a known variable star
20:45:20.32 +42:15:12.9 -- not a known variable star
20:45:22.25 +42:29:22.1 -- not a known variable star
20:45:30.80 +42:09:03.0 -- not a known variable star
20:45:32.53 +42:12:28.1 -- not a known variable star
20:45:36.47 +42:13:42.1 -- not a known variable star
20:45:37.47 +41:41:31.9 -- not a known variable star
20:45:41.34 +42:11:18.0 -- not a known variable star
20:45:42.96 +42:00:25.1 -- not a known variable star
20:45:43.04 +42:19:20.1 -- not a known variable star
20:45:44.30 +43:09:42.4 -- not a known variable star
20:45:44.41 +42:18:37.9 -- not a known variable star
20:45:49.52 +42:03:56.3 -- not a known variable star
20:45:56.57 +42:06:28.5 -- not a known variable star
20:46:00.19 +42:18:21.6 -- not a known variable star
20:46:00.97 +42:22:19.4 -- not a known variable star
20:46:01.52 +42:17:52.8 -- not a known variable star
20:46:05.41 +42:04:52.9 -- not a known variable star
20:46:07.15 +42:55:13.0 -- not a known variable star
20:46:07.80 +43:06:31.8 -- a known variable star
20:46:10.36 +43:04:35.2 -- not a known variable star
20:46:10.51 +41:33:21.8 -- not a known variable star
20:46:12.54 +42:59:23.5 -- not a known variable star
20:46:13.93 +43:12:46.4 -- a known variable star
20:46:14.81 +40:46:43.6 -- a known variable star
20:46:17.49 +43:09:28.2 -- not a known variable star
20:46:19.49 +42:59:59.7 -- not a known variable star
20:46:22.01 +41:40:26.4 -- not a known variable star
20:46:23.97 +42:06:23.3 -- not a known variable star
20:46:30.43 +42:01:03.3 -- not a known variable star
20:46:34.17 +42:50:10.4 -- not a known variable star
20:46:35.19 +41:48:06.3 -- not a known variable star
20:46:35.38 +41:45:42.9 -- not a known variable star
20:46:35.79 +42:30:17.7 -- not a known variable star
20:46:39.35 +41:43:16.8 -- a known variable star
20:46:43.86 +42:59:43.9 -- a known variable star
20:46:47.72 +41:26:14.2 -- not a known variable star
20:46:48.48 +41:08:06.5 -- not a known variable star
20:46:49.32 +41:46:10.9 -- not a known variable star
20:46:52.82 +42:08:59.4 -- a known variable star
20:46:54.24 +41:21:48.9 -- a known variable star
20:46:54.96 +42:39:27.0 -- not a known variable star
20:46:56.69 +43:01:26.9 -- not a known variable star
20:46:57.01 +42:21:26.2 -- not a known variable star
20:46:57.10 +40:59:06.4 -- a known variable star
20:46:58.63 +41:45:50.4 -- not a known variable star
20:46:59.57 +42:40:45.8 -- not a known variable star
20:47:00.83 +41:57:50.4 -- not a known variable star
20:47:01.36 +41:37:09.6 -- not a known variable star
20:47:03.33 +42:47:09.3 -- not a known variable star
20:47:05.03 +41:46:42.6 -- not a known variable star
20:47:06.59 +42:38:55.8 -- not a known variable star
20:47:08.92 +42:14:20.3 -- not a known variable star
20:47:09.04 +41:59:16.3 -- not a known variable star
20:47:16.87 +42:08:43.6 -- not a known variable star
20:47:19.26 +41:40:34.9 -- not a known variable star
20:47:24.57 +42:53:04.9 -- not a known variable star
20:47:24.60 +42:03:13.0 -- not a known variable star
20:47:25.54 +42:21:01.8 -- not a known variable star
20:47:26.96 +42:43:10.6 -- not a known variable star
20:47:27.94 +42:57:38.2 -- not a known variable star
20:47:32.84 +41:59:43.0 -- not a known variable star
20:47:33.81 +42:06:42.9 -- not a known variable star
20:47:36.07 +41:57:04.7 -- not a known variable star
20:47:40.50 +41:05:32.6 -- a known variable star
20:47:42.36 +42:15:51.3 -- not a known variable star
20:47:43.59 +41:31:42.6 -- not a known variable star
20:47:44.97 +41:43:20.9 -- not a known variable star
20:47:47.62 +42:36:22.9 -- not a known variable star
20:47:49.80 +41:49:50.9 -- not a known variable star
20:47:51.49 +41:57:28.1 -- not a known variable star
20:47:51.50 +41:24:19.2 -- not a known variable star
20:47:52.66 +42:21:25.5 -- not a known variable star
20:47:59.59 +42:39:40.4 -- not a known variable star
20:48:01.31 +41:18:26.8 -- not a known variable star
20:48:03.25 +41:34:59.4 -- a known variable star
20:48:06.75 +42:21:03.5 -- not a known variable star
20:48:08.95 +41:10:32.1 -- not a known variable star
20:48:09.51 +41:43:30.3 -- not a known variable star
20:48:11.22 +41:08:48.9 -- not a known variable star
20:48:11.25 +40:49:58.8 -- not a known variable star
20:48:13.02 +42:09:53.6 -- a known variable star
20:48:16.50 +42:38:47.2 -- not a known variable star
20:48:18.79 +41:48:05.0 -- a known variable star
20:48:20.10 +41:34:04.5 -- not a known variable star
20:48:23.46 +41:52:15.1 -- not a known variable star
20:48:25.24 +40:51:06.1 -- not a known variable star
20:48:26.11 +42:07:56.8 -- not a known variable star
20:48:29.57 +41:29:14.6 -- not a known variable star
20:48:31.23 +41:23:11.9 -- not a known variable star
20:48:32.20 +41:37:34.3 -- not a known variable star
20:48:33.09 +41:42:36.7 -- not a known variable star
20:48:34.51 +41:28:44.8 -- not a known variable star
20:48:36.18 +41:52:31.9 -- not a known variable star
20:48:39.23 +41:57:07.3 -- not a known variable star
20:48:40.13 +41:50:15.6 -- not a known variable star
20:48:41.07 +41:49:47.2 -- not a known variable star
20:48:44.85 +41:51:16.3 -- not a known variable star
20:48:47.05 +41:32:05.7 -- not a known variable star
20:48:47.96 +42:14:18.9 -- not a known variable star
20:48:53.16 +41:45:58.7 -- not a known variable star
20:48:53.30 +41:48:49.1 -- not a known variable star
20:48:54.03 +41:43:31.6 -- not a known variable star
20:48:54.68 +41:52:08.3 -- not a known variable star
20:48:57.73 +41:55:54.9 -- not a known variable star
20:48:57.94 +41:03:20.8 -- not a known variable star
20:48:58.68 +42:34:19.3 -- not a known variable star
20:48:59.55 +41:55:26.5 -- not a known variable star
20:49:06.85 +41:49:21.7 -- not a known variable star
20:49:07.30 +41:22:59.3 -- not a known variable star
20:49:14.17 +41:58:17.0 -- not a known variable star
20:49:24.04 +41:41:59.4 -- not a known variable star
20:49:30.68 +41:11:17.7 -- not a known variable star
20:49:31.65 +41:57:07.4 -- a known variable star
20:49:35.86 +42:22:16.8 -- not a known variable star
20:49:37.78 +41:08:54.5 -- not a known variable star
20:49:38.36 +41:42:49.3 -- not a known variable star
20:49:39.00 +41:39:42.7 -- not a known variable star
20:49:40.33 +41:56:56.1 -- a known variable star
20:49:43.24 +41:48:30.8 -- not a known variable star
20:49:44.05 +41:51:30.8 -- not a known variable star
20:49:44.10 +42:13:14.1 -- not a known variable star
20:49:46.03 +42:08:00.9 -- not a known variable star
20:49:46.94 +42:22:03.4 -- not a known variable star
20:49:49.81 +42:25:12.6 -- a known variable star
20:49:51.50 +41:48:17.7 -- not a known variable star
20:50:00.64 +42:58:09.8 -- a known variable star
20:50:01.41 +41:46:18.5 -- a known variable star
20:50:02.38 +42:32:06.5 -- not a known variable star
20:50:03.84 +41:50:52.3 -- not a known variable star
20:50:03.95 +43:00:11.4 -- not a known variable star
20:50:04.64 +42:18:47.6 -- not a known variable star
20:50:05.22 +42:03:00.0 -- a known variable star
20:50:11.34 +41:48:51.0 -- not a known variable star
20:50:12.98 +40:51:23.3 -- not a known variable star
20:50:20.20 +41:52:25.6 -- not a known variable star
20:50:20.72 +41:43:22.4 -- not a known variable star
20:50:25.72 +41:47:32.1 -- not a known variable star
20:50:28.78 +41:56:06.7 -- a known variable star
20:50:35.07 +40:46:12.4 -- not a known variable star
20:50:40.96 +41:38:00.9 -- not a known variable star
20:50:41.16 +41:48:29.3 -- not a known variable star
20:50:43.06 +41:53:42.4 -- not a known variable star
20:50:43.19 +42:15:26.8 -- not a known variable star
20:50:43.74 +42:05:55.4 -- not a known variable star
20:50:44.32 +41:29:51.2 -- not a known variable star
20:50:48.69 +41:48:13.7 -- not a known variable star
20:50:51.21 +42:25:34.6 -- not a known variable star
20:50:51.53 +41:43:36.2 -- not a known variable star
20:50:53.04 +40:56:35.2 -- not a known variable star
20:50:54.46 +41:52:21.5 -- a known variable star
20:50:55.68 +41:40:20.2 -- a known variable star
20:50:57.06 +41:54:30.1 -- not a known variable star
20:50:57.25 +42:45:47.6 -- not a known variable star
20:50:58.16 +42:36:05.0 -- not a known variable star
20:50:58.70 +40:53:04.7 -- not a known variable star
20:50:59.21 +42:44:17.0 -- not a known variable star
20:51:01.65 +41:37:20.3 -- not a known variable star
20:51:02.18 +41:32:18.8 -- not a known variable star
20:51:03.76 +42:29:30.0 -- not a known variable star
20:51:05.07 +41:46:59.9 -- not a known variable star
20:51:09.00 +42:28:31.3 -- not a known variable star
20:51:09.25 +41:37:26.0 -- not a known variable star
20:51:11.95 +42:42:18.7 -- not a known variable star
20:51:12.93 +40:44:12.7 -- not a known variable star
20:51:14.23 +42:16:58.7 -- not a known variable star
20:51:15.82 +41:26:13.7 -- not a known variable star
20:51:17.31 +41:50:44.9 -- not a known variable star
20:51:17.62 +40:59:40.5 -- not a known variable star
20:51:18.70 +41:45:29.5 -- not a known variable star
20:51:19.07 +41:55:31.4 -- not a known variable star
20:51:22.15 +41:47:39.9 -- not a known variable star
20:51:27.24 +41:34:31.8 -- a known variable star
20:51:27.41 +41:53:07.5 -- not a known variable star
20:51:30.68 +41:32:16.3 -- not a known variable star
20:51:33.96 +41:04:35.6 -- not a known variable star
20:51:34.31 +41:25:45.5 -- not a known variable star
20:51:38.47 +42:34:34.4 -- not a known variable star
20:51:39.83 +40:52:41.3 -- not a known variable star
20:51:39.99 +41:32:07.9 -- not a known variable star
20:51:43.40 +41:15:39.2 -- not a known variable star
20:51:46.14 +41:34:27.2 -- a known variable star
20:51:46.20 +42:27:04.2 -- a known variable star
20:51:48.65 +41:17:21.2 -- not a known variable star
20:51:49.86 +41:28:19.7 -- not a known variable star
20:51:51.20 +41:31:29.8 -- not a known variable star
20:51:51.65 +41:52:04.8 -- not a known variable star
20:51:55.06 +41:15:59.2 -- not a known variable star
20:51:56.14 +41:55:20.1 -- not a known variable star
20:51:57.23 +42:20:13.0 -- not a known variable star
20:52:05.62 +42:28:27.9 -- not a known variable star
20:52:06.36 +42:31:31.5 -- not a known variable star
20:52:09.04 +41:23:26.5 -- not a known variable star
20:52:11.10 +40:52:50.6 -- not a known variable star
20:52:12.43 +42:00:58.9 -- not a known variable star
20:52:14.50 +41:34:58.4 -- not a known variable star
20:52:14.80 +41:10:34.8 -- not a known variable star
20:52:19.42 +40:55:30.8 -- a known variable star
20:52:20.78 +41:13:49.7 -- not a known variable star
20:52:24.43 +41:47:43.8 -- a known variable star
20:52:26.11 +41:16:10.2 -- not a known variable star
20:52:31.41 +41:34:07.8 -- a known variable star
20:52:37.80 +42:26:09.8 -- not a known variable star
20:52:38.81 +41:37:21.4 -- not a known variable star
20:52:47.87 +41:59:28.7 -- a known variable star
20:52:50.35 +40:47:52.5 -- not a known variable star
20:52:51.60 +41:08:31.3 -- not a known variable star
20:52:52.53 +40:56:00.1 -- not a known variable star
20:52:53.29 +40:41:38.1 -- not a known variable star
20:52:54.02 +42:18:36.1 -- not a known variable star
20:52:59.23 +40:57:24.1 -- not a known variable star
20:53:00.18 +42:36:15.5 -- not a known variable star
20:53:03.69 +41:49:10.1 -- a known variable star
20:53:06.23 +42:24:01.2 -- not a known variable star
20:53:10.15 +40:52:40.3 -- not a known variable star
20:53:10.52 +42:10:28.5 -- a known variable star
20:53:10.61 +42:23:32.5 -- not a known variable star
20:53:11.56 +42:31:53.6 -- a known variable star
20:53:16.86 +42:09:03.0 -- not a known variable star
20:53:20.07 +40:55:15.5 -- not a known variable star
20:53:21.23 +42:19:15.9 -- a known variable star
20:53:24.99 +42:30:38.5 -- not a known variable star
20:53:29.11 +42:10:19.8 -- not a known variable star
20:53:32.74 +42:14:22.0 -- not a known variable star
20:53:37.43 +42:32:29.4 -- not a known variable star
20:53:37.73 +41:50:07.6 -- not a known variable star
20:53:43.21 +41:52:38.1 -- not a known variable star
20:53:54.47 +42:24:53.1 -- not a known variable star
20:54:00.19 +41:34:00.3 -- a known variable star
20:54:02.41 +42:06:27.6 -- not a known variable star
20:54:12.96 +41:57:07.9 -- not a known variable star
20:54:22.30 +41:59:16.1 -- not a known variable star
20:54:29.35 +42:05:12.8 -- not a known variable star
20:54:30.76 +41:50:56.2 -- not a known variable star
20:54:35.22 +42:34:50.3 -- not a known variable star
20:54:49.61 +41:53:51.9 -- not a known variable star
20:54:56.46 +41:51:14.0 -- not a known variable star
20:55:11.39 +41:51:15.9 -- not a known variable star
20:55:43.79 +41:47:35.7 -- not a known variable star
20:56:11.88 +42:36:06.1 -- not a known variable star
20:58:08.83 +41:47:10.6 -- not a known variable star
Found 345 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
411 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 411 (excluding asteroids and hot pixels, 345 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)2461300.87216147 -observatory V36
12:38:38.94 -04:12:42.6 Mercury (-0.4mag)
13:58:10.03 -17:56:48.6 Venus (-4.8mag)
07:40:42.92 +22:13:10.9 Mars (1.2mag)
09:17:08.76 +16:22:46.4 Jupiter (-1.8mag)
00:49:13.91 +02:21:16.0 Saturn (0.4mag)
04:13:37.89 +21:01:51.7 Uranus (5.7mag)
00:12:45.81 -00:09:48.8 Neptune (7.7mag)
20:24:58.29 -23:41:36.1 Pluto (14.5mag)
16:18:08.89 -26:52:22.6 Moon (-9.9mag)
-rw-r--r-- 1 apache apache 362 Sep 17 04:01 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461300.87216147:
09:17:14.44 +16:22:18.4 Io (6.0mag)
09:17:14.46 +16:22:18.6 Europa (6.2mag)
09:16:55.32 +16:23:57.2 Ganymede (5.6mag)
09:17:25.69 +16:21:20.7 Callisto (6.8mag)
09:15:20.21 +16:42:59.6 Himalia (15.7mag)
09:17:12.75 +16:22:27.5 Thebe (16.5mag)
09:14:48.54 +16:37:08.8 Elara (17.7mag)
09:20:44.90 +15:47:43.9 Pasiphae (17.9mag)
09:17:29.80 +16:43:20.8 Carme (18.9mag)
00:49:24.78 +02:20:48.4 Titan (8.3mag)
00:49:13.93 +02:20:55.6 Rhea (9.6mag)
00:49:00.17 +02:22:16.9 Iapetus (11.0mag)
00:49:00.47 +02:21:30.9 Hyperion (14.3mag)
00:47:50.75 +02:10:08.9 Phoebe (16.3mag)
-rw-r--r-- 1 apache apache 568 Sep 17 04:01 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461300.87216147:
23:29:14.03 +10:52:19.6 JWST
16:46:36.18 +43:12:07.1 Chandra
12:04:52.19 -61:32:03.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 17 04:01 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461300.87216147 -observatory V36
03:45:14.37 +19:44:45.6 17.3mag P/1996 R2 (Lagerkvist)
18:07:22.61 -34:01:03.4 14.5mag P/2010 H2 (Vales)
07:26:41.43 -70:52:52.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:32.54 +33:58:06.0 17.7mag C/2017 K2 (PANSTARRS)
05:02:35.76 +46:47:00.3 16.2mag P/2021 N1 (ZTF)
22:05:46.90 +27:22:26.9 17.5mag C/2022 E2 (ATLAS)
07:17:23.32 +25:47:48.9 16.9mag C/2022 N2 (PANSTARRS)
10:58:43.26 +26:53:20.3 17.1mag C/2022 QE78 (ATLAS)
09:54:56.93 +05:10:33.9 18.0mag C/2022 R6 (PANSTARRS)
15:27:37.27 -16:31:45.1 15.0mag C/2023 R1 (PANSTARRS)
08:46:44.30 +33:33:42.0 15.9mag C/2024 E1 (Wierzchos)
15:08:14.56 +15:12:51.7 18.0mag C/2024 G6 (ATLAS)
18:28:32.24 +42:43:45.1 13.7mag C/2024 J3 (ATLAS)
20:13:11.60 +48:37:21.2 17.4mag C/2024 R4 (PANSTARRS)
05:40:23.52 -13:11:04.0 15.0mag C/2024 T5 (ATLAS)
07:14:26.89 +16:28:33.5 17.8mag C/2025 J1 (Borisov)
11:34:33.14 +17:58:08.2 16.6mag C/2025 V2 (Rankin)
13:28:13.10 -00:42:29.5 16.7mag C/2025 Y1 (ATLAS)
17:11:09.05 +72:11:15.4 15.9mag C/2026 A2 (Bok)
02:59:32.33 +45:41:20.2 17.5mag C/2026 B2 (Sun-Gao)
12:22:42.03 +12:06:29.5 17.6mag A/2026 E1
22:34:33.22 -35:08:41.2 13.6mag 10P/Tempel
01:35:10.38 +38:45:59.3 17.5mag 11P/Tempel-Swift-LINEAR
11:54:57.88 -06:14:21.0 16.3mag 29P/Schwassmann-Wachmann
12:28:51.26 -08:14:46.2 17.8mag 63P/Wild
06:58:06.34 +18:24:59.0 17.1mag 78P/Gehrels
03:16:09.09 +15:01:42.8 17.3mag 88P/Howell
06:12:29.57 +32:23:45.5 17.3mag 112P/Urata-Niijima
08:00:53.26 +22:02:53.5 17.8mag 114P/Wiseman-Skiff
10:50:08.72 +18:41:19.4 14.8mag 123P/West-Hartley
13:09:10.79 -24:46:30.1 17.5mag 124P/Mrkos
06:29:01.95 +20:17:51.0 15.8mag 128P/Shoemaker-Holt
01:38:28.47 -15:30:30.1 14.5mag 161P/Hartley-IRAS
09:32:31.53 +08:40:51.8 12.5mag 169P/NEAT
03:30:54.90 +07:31:26.6 14.6mag 220P/McNaught
05:14:13.97 +39:18:21.8 15.3mag 260P/McNaught
08:58:09.77 +34:32:54.7 17.3mag 295P/LINEAR
15:32:11.94 -01:22:09.6 17.9mag 391P/Kowalski
09:36:20.27 +16:20:26.0 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 1.9K Sep 17 04:01 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
22:37:05.59 +34:24:35.70 SN2026aaiv 2026-09-7.22 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
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
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
-rw-r--r-- 1 apache apache 190K Sep 17 04:01 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
23:15:50.170 -00:21:47.12 AT 2026zta 2026-08-18.74 22.24
02:46:12.842 +06:11:52.33 AT 2026zsz 2026-08-23.78 19.3
22:38:13.667 +15:06:36.55 AT 2026zsy 2026-08-19.88 18.99
16:29:10.420 +50:17:23.09 SN 2026zsx 2026-08-23.92 18.643
00:30:37.105 +16:40:45.90 AT 2026zsw 2026-08-22.04 19.582
00:15:59.164 +45:15:18.02 AT 2026zsv 2026-08-15.37 21.2462
18:01:12.850 +23:06:59.14 AT 2026zsu 2026-08-12.17 20.552
16:34:01.788 +10:33:21.97 AT 2026zst 2026-08-05.18 20.8897
07:35:51.970 +14:30:02.34 AT 2026zss 2026-08-23.51 19.3532
12:34:19.746 +36:30:42.03 AT 2026zsr 2026-08-18.15 16.215
13:54:24.090 +08:32:46.11 AT 2026zsq 2026-08-17.15 19.6164
14:02:03.482 +00:12:24.13 AT 2026zsp 2026-08-18.15 20.1377
14:26:57.209 +16:14:29.77 AT 2026zso 2026-08-18.15 19.8733
15:19:36.047 +10:32:58.31 AT 2026zsn 2026-08-24.15 19.7907
14:53:08.508 -01:21:20.01 AT 2026zsm 2026-08-06.17 20.2832
23:26:24.962 -03:37:54.53 AT 2026zsl 2026-08-22.08 20.35
23:49:47.831 -44:13:09.26 AT 2026zsk 2026-08-23.60 17.63
03:00:56.094 +06:15:25.68 SN 2026zsj 2026-08-14.49 20.5067
01:07:44.807 +15:37:35.66 AT 2026zsi 2026-08-16.46 21.3122
01:56:39.058 -03:54:29.73 AT 2026zsh 2026-08-18.46 20.8101
-rw-r--r-- 1 apache apache 89K Sep 17 04:01 tns_transients_list.txt
