This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG
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 17.3736 2461300.8736 10.69 20:57:37.91 +41:58:56.6
83.58470 -2.35779 galactic Cyg Second-epoch detections are separated by 0.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4079+41.9824 | 20:57:37.91 +41:58:56.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.253+/-0.033 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:37.91 +41:58:56.6: 11.74 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:37.91 +41:58:56.6: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.4079+41.9824,2461300.8736,10.69,0.05,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 J314.4079+41.9824 20260917.3736 10.69CV 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 17.3736 2461300.8736 10.86 20:55:02.87 +41:31:54.4
82.92870 -2.28271 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.7620+41.5318 | 20:55:02.88 +41:31:54.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.598+/-0.025 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:02.87 +41:31:54.4: 12.03 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:02.87 +41:31:54.4: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.7620+41.5318,2461300.8736,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.7620+41.5318 20260917.3736 10.86CV 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 17.3736 2461300.8736 10.80 20:55:15.37 +41:41:22.2
83.07444 -2.21070 galactic Cyg Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.8138+41.6894 | 20:55:15.30 +41:41:22.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.792+/-0.025 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:15.37 +41:41:22.2: 12.00 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:15.37 +41:41:22.2: 11.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.8138+41.6894,2461300.8736,10.80,0.05,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 J313.8138+41.6894 20260917.3736 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 10.71 20:55:38.89 +41:41:51.0
83.12785 -2.26140 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9109+41.6971 | 20:55:38.63 +41:41:49.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:38.89 +41:41:51.0: 12.01 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:38.89 +41:41:51.0: 12.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.9109+41.6971,2461300.8736,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.9109+41.6971 20260917.3736 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 10.87 20:56:07.05 +42:02:47.1
83.45067 -2.10229 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065704824984783872 | 20:56:07.03 +42:02:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.388+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:07.05 +42:02:47.1: 11.98 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:07.05 +42:02:47.1: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065704824984783872,2461300.8736,10.87,0.05,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 2065704824984783872 20260917.3736 10.87CV 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 17.3736 2461300.8736 10.81 20:55:47.89 +41:37:34.8
83.09164 -2.32878 galactic Cyg Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065681082405587072 | 20:55:47.89 +41:37:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.029 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:47.89 +41:37:34.8: 11.98 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:47.89 +41:37:34.8: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065681082405587072,2461300.8736,10.81,0.05,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
Gaia DR3 2065681082405587072 20260917.3736 10.81CV 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 17.3736 2461300.8736 10.85 20:58:10.77 +42:28:39.4
84.02672 -2.11194 galactic Cyg Second-epoch detections are separated by 0.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5428+42.4900 | 20:58:10.85 +42:28:40.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:10.77 +42:28:39.4: 11.83 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:10.77 +42:28:39.4: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.5428+42.4900,2461300.8736,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5428+42.4900 20260917.3736 10.85CV 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 17.3736 2461300.8736 10.70 20:57:25.13 +41:55:56.1
83.52081 -2.36035 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3547+41.9322 | 20:57:25.13 +41:55:56.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.214+/-0.034 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:25.13 +41:55:56.1: 11.78 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:25.13 +41:55:56.1: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.3547+41.9322,2461300.8736,10.70,0.05,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 J314.3547+41.9322 20260917.3736 10.70CV 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 17.3736 2461300.8736 10.62 20:55:28.11 +41:17:39.5
82.79808 -2.49621 galactic Cyg Second-epoch detections are separated by 0.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065531450046323328 | 20:55:28.12 +41:17:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.211+/-0.034 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:28.11 +41:17:39.5: 11.71 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:28.11 +41:17:39.5: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065531450046323328,2461300.8736,10.62,0.05,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 2065531450046323328 20260917.3736 10.62CV 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 17.3736 2461300.8736 10.53 20:55:34.56 +41:36:48.0
83.05485 -2.30551 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.8997+41.6111 | 20:55:34.55 +41:36:48.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.248+/-0.029 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:34.56 +41:36:48.0: 11.67 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:34.56 +41:36:48.0: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.8997+41.6111,2461300.8736,10.53,0.05,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 J313.8997+41.6111 20260917.3736 10.53CV 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 17.3736 2461300.8736 12.30 20:56:00.95 +41:39:08.1
83.13775 -2.34303 galactic Cyg Second-epoch detections are separated by 1.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:00.95 +41:39:08.1 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:00.95 +41:39:08.1: 13.64 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:00.95 +41:39:08.1: 13.57 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.54 20:58:47.59 +42:06:12.1
83.81725 -2.44229 galactic Cyg Second-epoch detections are separated by 1.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065672977808766080 | 20:58:50.96 +42:06:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.292+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:47.59 +42:06:12.1: 13.63 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:47.59 +42:06:12.1: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 2065672977808766080,2461300.8736,12.54,0.05,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
Gaia DR3 2065672977808766080 20260917.3736 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 17.3736 2461300.8736 12.76 22:16:36.44 +48:58:57.5
98.53886 -6.41602 galactic Lac Second-epoch detections are separated by 0.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1999690426038064768 | 22:16:32.59 +48:59:04.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.990+/-0.032 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:36.44 +48:58:57.5: 13.68 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:36.44 +48:58:57.5: 13.69 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999690426038064768,2461300.8736,12.76,0.05,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
Gaia DR3 1999690426038064768 20260917.3736 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 17.3736 2461300.8736 12.20 20:54:56.51 +41:51:13.5
83.16219 -2.05996 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:56.51 +41:51:13.5 (user input) | T | P | (position from user input) J-Ks=0.553+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:56.51 +41:51:13.5: 13.66 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:56.51 +41:51:13.5: 13.69 +/- 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,2461300.8736,12.20,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.40 20:57:47.79 +41:54:10.7
83.54433 -2.43274 galactic Cyg Second-epoch detections are separated by 1.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4463+41.9042 | 20:57:47.79 +41:54:10.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.354+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:47.79 +41:54:10.7: 13.69 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:47.79 +41:54:10.7: 13.76 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 J314.4463+41.9042,2461300.8736,12.40,0.05,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 J314.4463+41.9042 20260917.3736 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 17.3736 2461300.8736 12.22 20:56:13.45 +41:11:51.7
82.81625 -2.66703 galactic Cyg Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:13.45 +41:11:51.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:13.45 +41:11:51.7: 13.70 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:13.45 +41:11:51.7: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461300.8736,12.22,0.05,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
target 20260917.3736 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 17.3736 2461300.8736 11.06 20:57:20.29 +41:45:28.2
83.37842 -2.46237 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3345+41.7579 | 20:57:20.29 +41:45:28.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.264+/-0.027 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:20.29 +41:45:28.2: 12.09 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:20.29 +41:45:28.2: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.3345+41.7579,2461300.8736,11.06,0.05,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 J314.3345+41.7579 20260917.3736 11.06CV 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 17.3736 2461300.8736 11.12 20:56:24.99 +42:05:10.5
83.51701 -2.11875 galactic Cyg Second-epoch detections are separated by 0.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065727742930274048 | 20:56:25.01 +42:05:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.033 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:24.99 +42:05:10.5: 12.10 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:24.99 +42:05:10.5: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065727742930274048,2461300.8736,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065727742930274048 20260917.3736 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.74 22:03:57.63 +42:05:36.8
92.66170 -10.72679 galactic Lac Second-epoch detections are separated by 1.2" 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 | 22:03:57.63 +42:05:36.8 (user input) | T | P | (position from user input) J-Ks=0.301+/-0.039 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:03:57.63 +42:05:36.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:03:57.63 +42:05:36.8: 13.85 +/- 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
target,2461300.8736,12.74,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.06 20:58:02.84 +41:43:33.4
83.44040 -2.58354 galactic Cyg Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5266+41.7234 | 20:58:02.89 +41:43:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:02.84 +41:43:33.4: 12.19 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:02.84 +41:43:33.4: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.5266+41.7234,2461300.8736,11.06,0.05,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 J314.5266+41.7234 20260917.3736 11.06CV 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 17.3736 2461300.8736 12.70 20:54:06.44 +42:55:11.7
83.87889 -1.25545 galactic Cyg Second-epoch detections are separated by 0.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.5304+42.9191 | 20:54:06.44 +42:55:11.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:06.44 +42:55:11.7: 13.85 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:06.44 +42:55:11.7: 13.99 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.5304+42.9191,2461300.8736,12.70,0.05,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 J313.5304+42.9191 20260917.3736 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 17.3736 2461300.8736 11.37 20:56:00.61 +42:27:51.7
83.75649 -1.81653 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065924937769600256 | 20:56:04.66 +42:27:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.495+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:00.61 +42:27:51.7: 12.28 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:00.61 +42:27:51.7: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065924937769600256,2461300.8736,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065924937769600256 20260917.3736 11.37CV 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 17.3736 2461300.8736 12.72 21:00:30.78 +42:03:49.4
83.99671 -2.70923 galactic Cyg Second-epoch detections are separated by 1.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:30.78 +42:03:49.4 (user input) | T | P | (position from user input) J-Ks=0.616+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:30.78 +42:03:49.4: 13.91 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:30.78 +42:03:49.4: 13.97 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.72,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.61 20:57:50.13 +41:39:32.6
83.36381 -2.59713 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:50.13 +41:39:32.6 (user input) | T | P | (position from user input) J-Ks=1.111+/-0.032 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:50.13 +41:39:32.6: 13.92 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:50.13 +41:39:32.6: 13.92 +/- 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
target,2461300.8736,12.61,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.62 20:57:54.21 +41:29:55.4
83.25031 -2.71121 galactic Cyg Second-epoch detections are separated by 0.6" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4788+41.4997 | 20:57:54.21 +41:29:55.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.486+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:54.21 +41:29:55.4: 14.00 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:54.21 +41:29:55.4: 14.11 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 J314.4788+41.4997,2461300.8736,12.62,0.05,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 J314.4788+41.4997 20260917.3736 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 17.3736 2461300.8736 12.52 20:57:57.16 +41:45:02.9
83.44775 -2.55395 galactic Cyg Second-epoch detections are separated by 0.6" and 4.7 pix
The object was found in VSX 2" Gaia DR3 2065658684157505152
Type: ROT
# Max. Min./Amp. JD0 Period
13.700 G 13.730 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:57.16 +41:45:02.9: 13.98 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:57.16 +41:45:02.9: 14.03 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 2065658684157505152,2461300.8736,12.52,0.05,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 2065658684157505152 20260917.3736 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 17.3736 2461300.8736 11.62 20:54:53.52 +42:23:51.1
83.57207 -1.70225 galactic Cyg Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.7232+42.3977 | 20:54:53.58 +42:23:51.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:53.52 +42:23:51.1: 12.63 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:53.52 +42:23:51.1: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 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 J313.7232+42.3977,2461300.8736,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.7232+42.3977 20260917.3736 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.66 20:58:42.80 +41:58:57.7
83.71614 -2.50994 galactic Cyg Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6783+41.9827 | 20:58:42.80 +41:58:57.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.470+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:42.80 +41:58:57.7: 14.00 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:42.80 +41:58:57.7: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.6783+41.9827,2461300.8736,12.66,0.05,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 J314.6783+41.9827 20260917.3736 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 17.3736 2461300.8736 12.61 20:56:36.13 +41:59:18.3
83.46485 -2.20843 galactic Cyg Second-epoch detections are separated by 1.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.1496+41.9885 | 20:56:36.13 +41:59:18.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:36.13 +41:59:18.3: 14.07 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:36.13 +41:59:18.3: 14.31 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 J314.1496+41.9885,2461300.8736,12.61,0.05,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 J314.1496+41.9885 20260917.3736 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 17.3736 2461300.8736 11.83 20:54:57.53 +42:14:38.4
83.46266 -1.81070 galactic Cyg Second-epoch detections are separated by 0.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.7272+42.2520 | 20:54:57.53 +42:14:38.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.722+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:57.53 +42:14:38.4: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:57.53 +42:14:38.4: 12.81 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 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 J313.7272+42.2520,2461300.8736,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.7272+42.2520 20260917.3736 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.84 20:54:56.93 +41:42:29.6
83.05172 -2.15479 galactic Cyg Second-epoch detections are separated by 1.4" and 4.6 pix
The object was found in VSX 0" Gaia DR3 2065693387494019840
Type: ROT
# Max. Min./Amp. JD0 Period
13.800 G 13.830 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:56.93 +41:42:29.6: 14.08 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:56.93 +41:42:29.6: 14.04 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 2065693387494019840,2461300.8736,12.84,0.05,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
Gaia DR3 2065693387494019840 20260917.3736 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 17.3736 2461300.8736 11.90 20:58:15.98 +42:09:49.5
83.79917 -2.32889 galactic Cyg Second-epoch detections are separated by 0.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5666+42.1637 | 20:58:15.98 +42:09:49.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.300+/-0.033 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:15.98 +42:09:49.5: 12.95 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:15.98 +42:09:49.5: 12.91 +/- 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
ATO J314.5666+42.1637,2461300.8736,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5666+42.1637 20260917.3736 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.08 21:00:53.90 +42:10:19.1
84.12539 -2.69180 galactic Cyg Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:53.90 +42:10:19.1 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:53.90 +42:10:19.1: 12.97 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:53.90 +42:10:19.1: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.08,0.05,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 20260917.3736 12.08CV 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 17.3736 2461300.8736 12.00 21:01:49.12 +41:30:48.4
83.74283 -3.25489 galactic Cyg Second-epoch detections are separated by 0.2" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.4506+41.5114 | 21:01:49.17 +41:30:47.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.404+/-0.036 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:01:49.12 +41:30:48.4: 12.99 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:01:49.12 +41:30:48.4: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.4506+41.5114,2461300.8736,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.4506+41.5114 20260917.3736 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.84 20:58:06.85 +42:34:52.3
84.09742 -2.03524 galactic Cyg Second-epoch detections are separated by 0.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161818359048949248 | 20:58:06.77 +42:34:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.156+/-0.039 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:06.85 +42:34:52.3: 13.03 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:06.85 +42:34:52.3: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 2161818359048949248,2461300.8736,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161818359048949248 20260917.3736 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.78 20:58:30.53 +41:36:40.8
83.40971 -2.72363 galactic Cyg Second-epoch detections are separated by 0.6" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6333+41.6164 | 20:58:30.53 +41:36:40.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.043+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:30.53 +41:36:40.8: 14.18 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:30.53 +41:36:40.8: 14.09 +/- 0.09 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 J314.6333+41.6164,2461300.8736,12.78,0.05,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 J314.6333+41.6164 20260917.3736 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 17.3736 2461300.8736 11.78 20:55:07.49 +41:59:27.1
83.28900 -1.99753 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:07.49 +41:59:27.1 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:07.49 +41:59:27.1: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:07.49 +41:59:27.1: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.19 20:59:12.48 +42:03:33.2
83.83423 -2.52939 galactic Cyg Second-epoch detections are separated by 4.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.8064+42.0626 | 20:59:12.48 +42:03:33.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.358+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:12.48 +42:03:33.2: 13.23 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:12.48 +42:03:33.2: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.8064+42.0626,2461300.8736,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.8064+42.0626 20260917.3736 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.24 20:59:36.46 +42:27:28.7
84.18424 -2.32401 galactic Cyg Second-epoch detections are separated by 1.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9090+42.4652 | 20:59:36.37 +42:27:28.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.645+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:36.46 +42:27:28.7: 13.30 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:36.46 +42:27:28.7: 13.38 +/- 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 J314.9090+42.4652,2461300.8736,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.9090+42.4652 20260917.3736 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 17.3736 2461300.8736 12.28 20:59:40.06 +42:07:32.2
83.94036 -2.55032 galactic Cyg Second-epoch detections are separated by 1.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9184+42.1260 | 20:59:40.06 +42:07:32.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:40.06 +42:07:32.2: 13.25 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:40.06 +42:07:32.2: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.9184+42.1260,2461300.8736,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.9184+42.1260 20260917.3736 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 17.3736 2461300.8736 12.73 20:57:12.63 +41:19:22.5
83.03202 -2.72690 galactic Cyg Second-epoch detections are separated by 2.6" and 5.0 pix
The object was found in VSX 1" Gaia DR3 2065612367229569920
Type: ROT
# Max. Min./Amp. JD0 Period
14.010 G 14.050 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:12.63 +41:19:22.5: 14.28 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:12.63 +41:19:22.5: 14.19 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.23 +/- 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 2065612367229569920,2461300.8736,12.73,0.05,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 2065612367229569920 20260917.3736 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 17.3736 2461300.8736 12.16 21:00:09.14 +42:24:01.6
84.20682 -2.43760 galactic Cyg Second-epoch detections are separated by 1.2" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0358+42.3983 | 21:00:09.14 +42:24:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.312+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:09.14 +42:24:01.6: 13.30 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:09.14 +42:24:01.6: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 J315.0358+42.3983,2461300.8736,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.0358+42.3983 20260917.3736 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.29 20:56:45.71 +42:49:04.9
84.11554 -1.69247 galactic Cyg Second-epoch detections are separated by 1.5" and 4.7 pix
The object was found in VSX 1" Gaia DR3 2162015347728646656
Type: ROT
# Max. Min./Amp. JD0 Period
13.110 G 13.140 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:45.71 +42:49:04.9: 13.32 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:45.71 +42:49:04.9: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2162015347728646656,2461300.8736,12.29,0.05,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
Gaia DR3 2162015347728646656 20260917.3736 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 17.3736 2461300.8736 13.13 22:16:29.09 +48:56:17.5
98.49704 -6.44157 galactic Lac Second-epoch detections are separated by 2.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.1214+48.9384 | 22:16:29.09 +48:56:17.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.377+/-0.058 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:29.09 +48:56:17.5: 14.37 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:29.09 +48:56:17.5: 14.30 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.33 +/- 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
ATO J334.1214+48.9384,2461300.8736,13.13,0.05,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 J334.1214+48.9384 20260917.3736 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 17.3736 2461300.8736 12.45 20:55:08.53 +42:47:47.7
83.90679 -1.47995 galactic Cyg Second-epoch detections are separated by 2.8" and 4.8 pix
The object was found in VSX 1" Gaia DR3 2065952769157926016
Type: ROT
# Max. Min./Amp. JD0 Period
13.180 G 13.200 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:08.53 +42:47:47.7: 13.36 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:08.53 +42:47:47.7: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065952769157926016,2461300.8736,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065952769157926016 20260917.3736 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 17.3736 2461300.8736 12.26 20:56:18.03 +42:26:25.4
83.77293 -1.87286 galactic Cyg Second-epoch detections are separated by 1.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:18.03 +42:26:25.4 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:18.03 +42:26:25.4: 13.36 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:18.03 +42:26:25.4: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.12 20:54:56.22 +42:06:30.3
83.35637 -1.89505 galactic Cyg Second-epoch detections are separated by 1.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:56.22 +42:06:30.3 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:56.22 +42:06:30.3: 13.38 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:56.22 +42:06:30.3: 13.31 +/- 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
target,2461300.8736,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.28 20:58:09.81 +41:35:31.6
83.35296 -2.68724 galactic Cyg Second-epoch detections are separated by 0.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:09.81 +41:35:31.6 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:09.81 +41:35:31.6: 13.41 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:09.81 +41:35:31.6: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.44 20:59:54.48 +42:17:01.5
84.08906 -2.48017 galactic Cyg Second-epoch detections are separated by 2.1" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9770+42.2839 | 20:59:54.48 +42:17:01.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.429+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:54.48 +42:17:01.5: 13.45 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:54.48 +42:17:01.5: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.9770+42.2839,2461300.8736,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.9770+42.2839 20260917.3736 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 17.3736 2461300.8736 13.22 22:15:24.17 +44:54:45.4
96.04880 -9.66100 galactic Lac Second-epoch detections are separated by 2.1" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:15:24.17 +44:54:45.4 (user input) | T | P | (position from user input) J-Ks=0.495+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:24.17 +44:54:45.4: 14.37 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:24.17 +44:54:45.4: 14.42 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.39 +/- 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,2461300.8736,13.22,0.05,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
target 20260917.3736 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.46 20:54:28.06 +42:37:09.9
83.69140 -1.49946 galactic Cyg Second-epoch detections are separated by 3.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:28.06 +42:37:09.9 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:28.06 +42:37:09.9: 13.46 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:28.06 +42:37:09.9: 13.47 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 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,2461300.8736,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.41 20:59:52.64 +42:13:39.7
84.04299 -2.51267 galactic Cyg Second-epoch detections are separated by 0.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9671+42.2280 | 20:59:52.64 +42:13:39.7 (user input) | LPV (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.362+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:52.64 +42:13:39.7: 13.51 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:52.64 +42:13:39.7: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.9671+42.2280,2461300.8736,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.9671+42.2280 20260917.3736 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.97 20:59:18.39 +41:25:47.8
83.36999 -2.95519 galactic Cyg Second-epoch detections are separated by 3.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:18.39 +41:25:47.8 (user input) | T | P | (position from user input) J-Ks=1.514+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:18.39 +41:25:47.8: 14.47 +/- 0.12 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:18.39 +41:25:47.8: 14.27 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.35 +/- 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,2461300.8736,12.97,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.24 20:54:49.58 +41:53:51.6
83.18191 -2.01521 galactic Cyg Second-epoch detections are separated by 1.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:49.58 +41:53:51.6 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.050 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:49.58 +41:53:51.6: 13.52 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:49.58 +41:53:51.6: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 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,2461300.8736,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.56 21:00:48.42 +42:19:23.1
84.22810 -2.57958 galactic Cyg Second-epoch detections are separated by 1.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.2021+42.3233 | 21:00:48.42 +42:19:23.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.389+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:48.42 +42:19:23.1: 13.54 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:48.42 +42:19:23.1: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2021+42.3233,2461300.8736,12.56,0.05,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
ATO J315.2021+42.3233 20260917.3736 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 17.3736 2461300.8736 12.80 20:58:52.65 +41:34:31.1
83.42748 -2.79935 galactic Cyg Second-epoch detections are separated by 3.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:52.65 +41:34:31.1 (user input) | T | P | (position from user input) J-Ks=1.280+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:52.65 +41:34:31.1: 14.44 +/- 0.13 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:52.65 +41:34:31.1: 14.31 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.80,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.86 20:56:00.82 +41:37:23.6
83.11534 -2.36151 galactic Cyg Second-epoch detections are separated by 2.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9901+41.6179 | 20:56:00.82 +41:37:23.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.494+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:00.82 +41:37:23.6: 14.44 +/- 0.13 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:00.82 +41:37:23.6: 14.29 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.35 +/- 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
ATO J313.9901+41.6179,2461300.8736,12.86,0.05,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
ATO J313.9901+41.6179 20260917.3736 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 17.3736 2461300.8736 12.42 20:59:14.01 +41:40:39.5
83.54855 -2.78274 galactic Cyg Second-epoch detections are separated by 1.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.8083+41.6776 | 20:59:14.01 +41:40:39.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.532+/-0.027 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:14.01 +41:40:39.5: 13.57 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:14.01 +41:40:39.5: 13.70 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.8083+41.6776,2461300.8736,12.42,0.05,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 J314.8083+41.6776 20260917.3736 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 17.3736 2461300.8736 12.62 21:00:18.52 +41:55:39.7
83.86910 -2.77003 galactic Cyg Second-epoch detections are separated by 1.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0651+41.9312 | 21:00:18.52 +41:55:39.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.264+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:18.52 +41:55:39.7: 13.56 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:18.52 +41:55:39.7: 13.79 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0651+41.9312,2461300.8736,12.62,0.05,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 J315.0651+41.9312 20260917.3736 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 17.3736 2461300.8736 12.63 21:04:49.29 +41:34:45.2
84.16568 -3.63150 galactic Cyg Second-epoch detections are separated by 0.7" and 4.8 pix
The object was found in VSX 4" Gaia DR3 1969330710972137984
Type: ROT
# Max. Min./Amp. JD0 Period
13.600 G 13.640 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:04:49.29 +41:34:45.2: 13.54 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:04:49.29 +41:34:45.2: 13.63 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1969330710972137984,2461300.8736,12.63,0.05,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 1969330710972137984 20260917.3736 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 17.3736 2461300.8736 12.37 20:55:43.24 +42:45:59.4
83.95244 -1.58039 galactic Cyg Second-epoch detections are separated by 1.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:43.24 +42:45:59.4 (user input) | T | P | (position from user input) J-Ks=0.921+/-0.032 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:43.24 +42:45:59.4: 13.53 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:43.24 +42:45:59.4: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461300.8736,12.37,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.31 20:56:33.34 +42:14:09.4
83.64778 -2.04132 galactic Cyg Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:33.34 +42:14:09.4 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:33.34 +42:14:09.4: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:33.34 +42:14:09.4: 13.48 +/- 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,2461300.8736,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.54 20:58:39.87 +41:12:46.8
83.12670 -3.00581 galactic Cyg Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:39.87 +41:12:46.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:39.87 +41:12:46.8: 13.89 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:39.87 +41:12:46.8: 13.77 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.54,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.50 22:19:28.94 +45:01:49.1
96.72149 -9.96934 galactic Lac Second-epoch detections are separated by 1.2" and 4.6 pix
The object was found in VSX 1" Gaia DR3 1962118361363464960
Type: ROT
# Max. Min./Amp. JD0 Period
13.170 G 13.230 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:28.94 +45:01:49.1: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:28.94 +45:01:49.1: 13.53 +/- 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 1962118361363464960,2461300.8736,12.50,0.05,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 1962118361363464960 20260917.3736 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 17.3736 2461300.8736 12.31 20:56:46.94 +41:53:07.6
83.40819 -2.30074 galactic Cyg Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.2114+41.8873 | 20:56:46.94 +41:53:07.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.562+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:46.94 +41:53:07.6: 13.54 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:46.94 +41:53:07.6: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 J314.2114+41.8873,2461300.8736,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.2114+41.8873 20260917.3736 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.17 20:55:02.24 +41:53:13.0
83.19905 -2.05214 galactic Cyg Second-epoch detections are separated by 1.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:02.24 +41:53:13.0 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:02.24 +41:53:13.0: 13.51 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:02.24 +41:53:13.0: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 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,2461300.8736,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.66 22:17:52.11 +44:17:05.3
96.05623 -10.42698 galactic Lac Second-epoch detections are separated by 0.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:52.11 +44:17:05.3 (user input) | T | P | (position from user input) J-Ks=0.761+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:52.11 +44:17:05.3: 13.51 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:52.11 +44:17:05.3: 13.66 +/- 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
target,2461300.8736,12.66,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.65 22:19:19.10 +44:52:39.4
96.61071 -10.08005 galactic Lac Second-epoch detections are separated by 0.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:19.10 +44:52:39.4 (user input) | T | P | (position from user input) J-Ks=0.584+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:19.10 +44:52:39.4: 13.47 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:19.10 +44:52:39.4: 13.57 +/- 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,2461300.8736,12.65,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.41 20:56:32.08 +42:12:05.9
83.61913 -2.06061 galactic Cyg Second-epoch detections are separated by 1.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.1338+42.2016 | 20:56:32.08 +42:12:05.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.554+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:32.08 +42:12:05.9: 13.48 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:32.08 +42:12:05.9: 13.50 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 J314.1338+42.2016,2461300.8736,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.1338+42.2016 20260917.3736 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.20 22:03:25.35 +42:10:18.6
92.62911 -10.60411 galactic Lac Second-epoch detections are separated by 3.7" 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 | 22:03:25.35 +42:10:18.6 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:03:25.35 +42:10:18.6: 14.43 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:03:25.35 +42:10:18.6: 14.32 +/- 0.09 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,2461300.8736,13.20,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.48 20:59:06.17 +42:38:30.9
84.26236 -2.13326 galactic Cyg Second-epoch detections are separated by 0.5" and 4.5 pix
The object was found in VSX 2" V1496 Cyg
Type: UV
# Max. Min./Amp. JD0 Period
12.500 U 16.500 U
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:06.17 +42:38:30.9: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:06.17 +42:38:30.9: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1496 Cyg,2461300.8736,12.48,0.05,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
V1496 Cyg 20260917.3736 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 17.3736 2461300.8736 12.84 20:58:05.62 +41:16:45.6
83.10695 -2.88121 galactic Cyg Second-epoch detections are separated by 3.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5265+41.2820 | 20:58:05.62 +41:16:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.539+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:05.62 +41:16:45.6: 14.38 +/- 0.12 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:05.62 +41:16:45.6: 14.07 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.19 +/- 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 J314.5265+41.2820,2461300.8736,12.84,0.05,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
ATO J314.5265+41.2820 20260917.3736 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 17.3736 2461300.8736 12.10 20:56:28.62 +41:38:12.5
83.18182 -2.41867 galactic Cyg Second-epoch detections are separated by 2.2" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.1334+41.6365 | 20:56:28.62 +41:38:12.5 (user input) | DBH (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.995+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:28.62 +41:38:12.5: 13.48 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:28.62 +41:38:12.5: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.1334+41.6365,2461300.8736,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.1334+41.6365 20260917.3736 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.14 20:55:54.50 +41:43:32.9
83.18088 -2.28013 galactic Cyg Second-epoch detections are separated by 1.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:54.50 +41:43:32.9 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:54.50 +41:43:32.9: 13.46 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:54.50 +41:43:32.9: 13.50 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.18 20:57:38.66 +41:49:09.2
83.46225 -2.46577 galactic Cyg Second-epoch detections are separated by 1.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:38.66 +41:49:09.2 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:38.66 +41:49:09.2: 13.45 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:38.66 +41:49:09.2: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461300.8736,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.85 20:57:55.44 +41:58:48.0
83.61828 -2.40055 galactic Cyg Second-epoch detections are separated by 0.6" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:55.44 +41:58:48.0 (user input) | T | P | (position from user input) J-Ks=1.077+/-0.031 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:55.44 +41:58:48.0: 14.36 +/- 0.12 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:55.44 +41:58:48.0: 14.25 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.30 +/- 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,2461300.8736,12.85,0.05,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 20260917.3736 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 17.3736 2461300.8736 13.36 22:17:39.81 +44:53:29.3
96.37185 -9.90462 galactic Lac Second-epoch detections are separated by 1.7" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:39.81 +44:53:29.3 (user input) | T | P | (position from user input) J-Ks=0.533+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:39.81 +44:53:29.3: 14.99 +/- 0.17 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:39.81 +44:53:29.3: 14.74 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 13.36CV 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 17.3736 2461300.8736 12.48 20:54:55.65 +43:02:37.1
84.07020 -1.29049 galactic Cyg Second-epoch detections are separated by 1.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:55.65 +43:02:37.1 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:55.65 +43:02:37.1: 13.43 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:55.65 +43:02:37.1: 13.54 +/- 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,2461300.8736,12.48,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.85 20:55:03.71 +42:03:54.8
83.33829 -1.94061 galactic Cyg Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ZTF J205505.30+420335.3 | 20:55:05.30 +42:03:35.3 (Gaia DR3) | SR (local) | 42.046723300000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:03.71 +42:03:54.8: 14.36 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:03.71 +42:03:54.8: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205505.30+420335.3,2461300.8736,12.85,0.05,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
ZTF J205505.30+420335.3 20260917.3736 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 17.3736 2461300.8736 12.09 20:56:11.15 +41:52:46.1
83.33160 -2.22008 galactic Cyg Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:11.15 +41:52:46.1 (user input) | T | P | (position from user input) J-Ks=0.514+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:11.15 +41:52:46.1: 13.43 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:11.15 +41:52:46.1: 13.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.54 20:59:34.34 +42:32:30.0
84.24321 -2.26422 galactic Cyg Second-epoch detections are separated by 1.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.8930+42.5314 | 20:59:34.34 +42:32:30.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.610+/-0.035 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:34.34 +42:32:30.0: 13.44 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:34.34 +42:32:30.0: 13.47 +/- 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
ATO J314.8930+42.5314,2461300.8736,12.54,0.05,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 J314.8930+42.5314 20260917.3736 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 17.3736 2461300.8736 12.28 20:55:33.80 +41:23:10.8
82.87991 -2.45036 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.8874+41.3845 | 20:55:33.80 +41:23:10.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.367+/-0.050 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:33.80 +41:23:10.8: 13.42 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:33.80 +41:23:10.8: 13.56 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.8874+41.3845,2461300.8736,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.8874+41.3845 20260917.3736 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 17.3736 2461300.8736 12.57 22:19:03.86 +45:01:23.1
96.65512 -9.93421 galactic Lac Second-epoch detections are separated by 1.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:03.86 +45:01:23.1 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:03.86 +45:01:23.1: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:03.86 +45:01:23.1: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.57,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.85 21:00:09.79 +41:15:21.8
83.34402 -3.19060 galactic Cyg Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:09.79 +41:15:21.8 (user input) | T | P | (position from user input) J-Ks=1.418+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:09.79 +41:15:21.8: 14.37 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:09.79 +41:15:21.8: 14.12 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.22 +/- 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,2461300.8736,12.85,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.44 22:19:33.89 +45:00:34.7
96.72213 -9.99462 galactic Lac Second-epoch detections are separated by 1.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:33.89 +45:00:34.7 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:33.89 +45:00:34.7: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:33.89 +45:00:34.7: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.44,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.34 20:54:26.88 +42:48:48.8
83.83765 -1.37168 galactic Cyg Second-epoch detections are separated by 3.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.6104+42.8103 | 20:54:26.88 +42:48:48.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.439+/-0.034 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:26.88 +42:48:48.8: 13.43 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:26.88 +42:48:48.8: 13.38 +/- 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
ATO J313.6104+42.8103,2461300.8736,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.6104+42.8103 20260917.3736 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.12 20:58:06.27 +41:43:25.6
83.44571 -2.59304 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5266+41.7234 | 20:58:02.89 +41:43:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.487+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:06.27 +41:43:25.6: 13.43 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:06.27 +41:43:25.6: 13.41 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.5266+41.7234,2461300.8736,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5266+41.7234 20260917.3736 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.53 22:04:00.87 +42:11:01.3
92.72526 -10.66103 galactic Lac Second-epoch detections are separated by 0.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1959898206868507264 | 22:03:56.81 +42:11:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.387+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:00.87 +42:11:01.3: 13.41 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:00.87 +42:11:01.3: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959898206868507264,2461300.8736,12.53,0.05,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
Gaia DR3 1959898206868507264 20260917.3736 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 17.3736 2461300.8736 12.23 20:55:37.91 +41:14:30.9
82.77789 -2.55348 galactic Cyg Second-epoch detections are separated by 0.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9084+41.2514 | 20:55:37.91 +41:14:30.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.343+/-0.034 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:37.91 +41:14:30.9: 13.42 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:37.91 +41:14:30.9: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.9084+41.2514,2461300.8736,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.9084+41.2514 20260917.3736 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 17.3736 2461300.8736 12.47 21:00:37.22 +42:04:36.4
84.01968 -2.71564 galactic Cyg Second-epoch detections are separated by 1.8" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1547+42.0768 | 21:00:37.22 +42:04:36.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.754+/-0.037 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:37.22 +42:04:36.4: 13.41 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:37.22 +42:04:36.4: 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
ATO J315.1547+42.0768,2461300.8736,12.47,0.05,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
ATO J315.1547+42.0768 20260917.3736 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 17.3736 2461300.8736 12.86 20:56:55.24 +41:25:51.6
83.07895 -2.61536 galactic Cyg Second-epoch detections are separated by 2.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:55.24 +41:25:51.6 (user input) | T | P | (position from user input) J-Ks=0.813+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:55.24 +41:25:51.6: 14.38 +/- 0.12 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:55.24 +41:25:51.6: 14.24 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.30 +/- 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,2461300.8736,12.86,0.05,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 20260917.3736 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 17.3736 2461300.8736 13.12 22:04:08.55 +42:05:35.9
92.68892 -10.74739 galactic Lac Second-epoch detections are separated by 1.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:08.55 +42:05:35.9 (user input) | T | P | (position from user input) J-Ks=0.698+/-0.034 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:08.55 +42:05:35.9: 14.39 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:08.55 +42:05:35.9: 14.22 +/- 0.08 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,2461300.8736,13.12,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.54 21:01:34.59 +42:35:32.2
84.52436 -2.50880 galactic Cyg Second-epoch detections are separated by 0.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161777367881094016 | 21:01:34.48 +42:35:32.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.576+/-0.041 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:01:34.59 +42:35:32.2: 13.41 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:01:34.59 +42:35:32.2: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161777367881094016,2461300.8736,12.54,0.05,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
Gaia DR3 2161777367881094016 20260917.3736 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 17.3736 2461300.8736 12.09 20:55:54.94 +41:55:53.9
83.33883 -2.14800 galactic Cyg Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:54.94 +41:55:53.9 (user input) | T | P | (position from user input) J-Ks=0.846+/-0.032 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:54.94 +41:55:53.9: 13.42 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:54.94 +41:55:53.9: 13.45 +/- 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
target,2461300.8736,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.32 20:59:08.34 +42:33:13.3
84.19998 -2.19604 galactic Cyg Second-epoch detections are separated by 0.2" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:08.34 +42:33:13.3 (user input) | T | P | (position from user input) J-Ks=0.409+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:08.34 +42:33:13.3: 13.40 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:08.34 +42:33:13.3: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.45 20:54:42.67 +42:35:24.6
83.69790 -1.55257 galactic Cyg Second-epoch detections are separated by 2.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.6882+42.5801 | 20:54:42.67 +42:35:24.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.551+/-0.036 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:42.67 +42:35:24.6: 13.40 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:42.67 +42:35:24.6: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 J313.6882+42.5801,2461300.8736,12.45,0.05,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 J313.6882+42.5801 20260917.3736 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 17.3736 2461300.8736 12.21 20:57:49.24 +41:20:12.2
83.11711 -2.80493 galactic Cyg Second-epoch detections are separated by 1.4" 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 | 20:57:49.24 +41:20:12.2 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.037 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:49.24 +41:20:12.2: 13.37 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:49.24 +41:20:12.2: 13.21 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.20 20:55:22.28 +41:59:48.4
83.32311 -2.02869 galactic Cyg Second-epoch detections are separated by 1.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:22.28 +41:59:48.4 (user input) | T | P | (position from user input) J-Ks=0.466+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:22.28 +41:59:48.4: 13.38 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:22.28 +41:59:48.4: 13.43 +/- 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
target,2461300.8736,12.20,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.29 20:55:03.80 +42:22:40.6
83.57752 -1.73906 galactic Cyg Second-epoch detections are separated by 0.8" and 4.7 pix
The object was found in VSX 1" Gaia DR3 2065903084976647808
Type: ROT
# Max. Min./Amp. JD0 Period
13.030 G 13.070 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:03.80 +42:22:40.6: 13.38 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:03.80 +42:22:40.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065903084976647808,2461300.8736,12.29,0.05,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
Gaia DR3 2065903084976647808 20260917.3736 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 17.3736 2461300.8736 12.55 22:02:15.24 +42:04:09.9
92.39073 -10.55380 galactic Lac Second-epoch detections are separated by 0.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:15.24 +42:04:09.9 (user input) | T | P | (position from user input) J-Ks=0.633+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:02:15.24 +42:04:09.9: 13.39 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:02:15.24 +42:04:09.9: 13.52 +/- 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,2461300.8736,12.55,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.41 22:16:03.15 +44:55:13.3
96.14935 -9.71987 galactic Lac Second-epoch detections are separated by 0.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.0069+44.9317 | 22:16:03.15 +44:55:13.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.716+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:03.15 +44:55:13.3: 13.39 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:03.15 +44:55:13.3: 13.29 +/- 0.03 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 J334.0069+44.9317,2461300.8736,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.0069+44.9317 20260917.3736 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.12 20:58:00.70 +42:01:11.8
83.65923 -2.38686 galactic Cyg Second-epoch detections are separated by 1.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4991+42.0183 | 20:58:00.70 +42:01:11.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.567+/-0.050 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:00.70 +42:01:11.8: 13.39 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:00.70 +42:01:11.8: 13.37 +/- 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
ATO J314.4991+42.0183,2461300.8736,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.4991+42.0183 20260917.3736 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.30 20:58:35.06 +42:11:54.0
83.86388 -2.35093 galactic Cyg Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:35.06 +42:11:54.0 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:35.06 +42:11:54.0: 13.39 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:35.06 +42:11:54.0: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.18 20:58:30.99 +42:19:45.7
83.95497 -2.25584 galactic Cyg Second-epoch detections are separated by 1.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:30.99 +42:19:45.7 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.035 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:30.99 +42:19:45.7: 13.38 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:30.99 +42:19:45.7: 13.31 +/- 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
target,2461300.8736,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.71 21:00:48.91 +41:30:11.0
83.61098 -3.12046 galactic Cyg Second-epoch detections are separated by 0.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:48.91 +41:30:11.0 (user input) | T | P | (position from user input) J-Ks=0.812+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:48.91 +41:30:11.0: 14.35 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:48.91 +41:30:11.0: 14.24 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.29 +/- 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,2461300.8736,12.71,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.54 21:00:21.34 +42:35:11.4
84.37183 -2.34358 galactic Cyg Second-epoch detections are separated by 0.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:21.34 +42:35:11.4 (user input) | T | P | (position from user input) J-Ks=1.194+/-0.043 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:21.34 +42:35:11.4: 13.38 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:21.34 +42:35:11.4: 13.57 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.54,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.49 22:14:44.34 +44:56:23.1
95.96648 -9.57181 galactic Lac Second-epoch detections are separated by 1.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:14:44.34 +44:56:23.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:14:44.34 +44:56:23.1: 13.36 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:14:44.34 +44:56:23.1: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.49,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.47 22:04:07.37 +42:07:51.6
92.70914 -10.71515 galactic Lac Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:07.37 +42:07:51.6 (user input) | T | P | (position from user input) J-Ks=0.669+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:07.37 +42:07:51.6: 13.36 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:07.37 +42:07:51.6: 13.32 +/- 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
target,2461300.8736,12.47,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.44 22:19:28.79 +44:49:14.8
96.60273 -10.14320 galactic Lac Second-epoch detections are separated by 0.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:28.79 +44:49:14.8 (user input) | T | P | (position from user input) J-Ks=0.496+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:28.79 +44:49:14.8: 13.37 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:28.79 +44:49:14.8: 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,2461300.8736,12.44,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.31 20:55:22.31 +42:18:43.0
83.56391 -1.82520 galactic Cyg Second-epoch detections are separated by 1.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:22.31 +42:18:43.0 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:22.31 +42:18:43.0: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:22.31 +42:18:43.0: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.23 22:17:07.59 +45:08:30.6
96.43508 -9.64422 galactic Lac Second-epoch detections are separated by 1.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:07.59 +45:08:30.6 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:07.59 +45:08:30.6: 14.32 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:07.59 +45:08:30.6: 14.44 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.38 +/- 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,2461300.8736,13.23,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.38 21:00:06.38 +42:10:03.6
84.02553 -2.58408 galactic Cyg Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.0239+42.1634 | 21:00:06.38 +42:10:03.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.454+/-0.052 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:06.38 +42:10:03.6: 13.35 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:06.38 +42:10:03.6: 13.39 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.0239+42.1634,2461300.8736,12.38,0.05,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 J315.0239+42.1634 20260917.3736 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 17.3736 2461300.8736 12.24 20:56:14.98 +42:06:14.1
83.51040 -2.08373 galactic Cyg Second-epoch detections are separated by 1.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:14.98 +42:06:14.1 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:14.98 +42:06:14.1: 13.34 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:14.98 +42:06:14.1: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.43 22:17:20.92 +45:03:21.2
96.41890 -9.73733 galactic Lac Second-epoch detections are separated by 0.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:20.92 +45:03:21.2 (user input) | T | P | (position from user input) J-Ks=0.774+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:20.92 +45:03:21.2: 13.36 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:20.92 +45:03:21.2: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.31 20:56:04.61 +42:43:29.8
83.96309 -1.65714 galactic Cyg Second-epoch detections are separated by 1.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.0196+42.7239 | 20:56:04.61 +42:43:29.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:04.61 +42:43:29.8: 13.32 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:04.61 +42:43:29.8: 13.35 +/- 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 J314.0196+42.7239,2461300.8736,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.0196+42.7239 20260917.3736 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.23 21:00:20.06 +41:11:05.9
83.31149 -3.26155 galactic Cyg Second-epoch detections are separated by 2.4" 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 | 21:00:20.06 +41:11:05.9 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:20.06 +41:11:05.9: 13.34 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:20.06 +41:11:05.9: 13.47 +/- 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
target,2461300.8736,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.76 20:58:02.99 +42:28:18.1
84.00662 -2.09768 galactic Cyg Second-epoch detections are separated by 1.7" and 4.3 pix
The object was found in VSX22" Gaia DR3 2161816336129124480
Type: YSO
# Max. Min./Amp. JD0 Period
15.860 G 15.940 G
ATTENTION: measured mag 12.76 is 3.1 mag brighter than the VSX record maximum brightness 15.86 - 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-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:02.99 +42:28:18.1: 14.31 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:02.99 +42:28:18.1: 14.19 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 2161816336129124480,2461300.8736,12.76,0.05,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
Gaia DR3 2161816336129124480 20260917.3736 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 17.3736 2461300.8736 12.44 22:17:03.89 +44:56:05.7
96.30772 -9.80907 galactic Lac Second-epoch detections are separated by 1.1" and 4.7 pix
The object was found in VSX 0" Gaia DR3 1962207971561724160
Type: ROT
# Max. Min./Amp. JD0 Period
13.050 G 13.130 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:03.89 +44:56:05.7: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:03.89 +44:56:05.7: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1962207971561724160,2461300.8736,12.44,0.05,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
Gaia DR3 1962207971561724160 20260917.3736 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 17.3736 2461300.8736 12.37 21:00:01.86 +42:20:43.6
84.15058 -2.45682 galactic Cyg Second-epoch detections are separated by 0.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:01.86 +42:20:43.6 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:01.86 +42:20:43.6: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:01.86 +42:20:43.6: 13.35 +/- 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
target,2461300.8736,12.37,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.46 21:04:41.86 +41:42:31.5
84.24691 -3.52787 galactic Cyg Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:04:41.86 +41:42:31.5 (user input) | T | P | (position from user input) J-Ks=0.447+/-0.026 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:04:41.86 +41:42:31.5: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:04:41.86 +41:42:31.5: 13.45 +/- 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,2461300.8736,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.12 20:58:05.54 +42:02:32.7
83.68606 -2.38357 galactic Cyg Second-epoch detections are separated by 1.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:05.54 +42:02:32.7 (user input) | T | P | (position from user input) J-Ks=0.508+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:05.54 +42:02:32.7: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:05.54 +42:02:32.7: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.39 22:02:00.14 +42:13:18.8
92.44762 -10.40449 galactic Lac Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:00.14 +42:13:18.8 (user input) | T | P | (position from user input) J-Ks=0.739+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:02:00.14 +42:13:18.8: 13.32 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:02:00.14 +42:13:18.8: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.39,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.06 20:55:57.25 +41:07:24.2
82.72661 -2.67637 galactic Cyg Second-epoch detections are separated by 1.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:57.25 +41:07:24.2 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:57.25 +41:07:24.2: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:57.25 +41:07:24.2: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.36 22:17:44.94 +44:57:56.2
96.42682 -9.85177 galactic Lac Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.4376+44.9657 | 22:17:44.94 +44:57:56.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:44.94 +44:57:56.2: 13.32 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:44.94 +44:57:56.2: 13.38 +/- 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 J334.4376+44.9657,2461300.8736,12.36,0.05,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 J334.4376+44.9657 20260917.3736 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 17.3736 2461300.8736 12.89 20:55:12.11 +41:58:00.1
83.27977 -2.02406 galactic Cyg Second-epoch detections are separated by 1.8" 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 | 20:55:12.11 +41:58:00.1 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.036 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:12.11 +41:58:00.1: 14.29 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:12.11 +41:58:00.1: 14.49 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.89,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.12 20:54:40.82 +42:03:30.7
83.28750 -1.89080 galactic Cyg Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:40.82 +42:03:30.7 (user input) | T | P | (position from user input) J-Ks=0.680+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:40.82 +42:03:30.7: 13.31 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:40.82 +42:03:30.7: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.14 20:57:01.53 +42:00:44.6
83.53419 -2.25270 galactic Cyg Second-epoch detections are separated by 0.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:01.53 +42:00:44.6 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:01.53 +42:00:44.6: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:01.53 +42:00:44.6: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.65 20:57:52.04 +41:24:13.7
83.17379 -2.76789 galactic Cyg Second-epoch detections are separated by 2.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:52.04 +41:24:13.7 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:52.04 +41:24:13.7: 14.25 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:52.04 +41:24:13.7: 14.26 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.25 +/- 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,2461300.8736,12.65,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.35 22:04:42.22 +41:56:40.1
92.68210 -10.92897 galactic Lac Second-epoch detections are separated by 0.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.1610+41.9501 | 22:04:42.22 +41:56:40.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.768+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:42.22 +41:56:40.1: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:42.22 +41:56:40.1: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J331.1610+41.9501,2461300.8736,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J331.1610+41.9501 20260917.3736 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 17.3736 2461300.8736 11.96 20:56:31.05 +41:30:42.7
83.09151 -2.50543 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:31.05 +41:30:42.7 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:31.05 +41:30:42.7: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:31.05 +41:30:42.7: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.46 22:05:02.12 +41:56:05.9
92.72642 -10.97370 galactic Lac Second-epoch detections are separated by 0.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:02.12 +41:56:05.9 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:05:02.12 +41:56:05.9: 13.29 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:05:02.12 +41:56:05.9: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.30 20:55:00.46 +42:08:23.8
83.38894 -1.88473 galactic Cyg Second-epoch detections are separated by 2.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.7520+42.1398 | 20:55:00.46 +42:08:23.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.320+/-0.034 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:00.46 +42:08:23.8: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:00.46 +42:08:23.8: 13.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.7520+42.1398,2461300.8736,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.7520+42.1398 20260917.3736 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 17.3736 2461300.8736 13.12 22:03:36.22 +42:03:43.3
92.58863 -10.71183 galactic Lac Second-epoch detections are separated by 2.2" and 4.9 pix
The object was found in VSX 3" ZTF J220336.37+420341.5
Type: SR
# Max. Min./Amp. JD0 Period
13.742 r Y 0.334 r 2458375.47480 53.312913600000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:03:36.22 +42:03:43.3: 14.27 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:03:36.22 +42:03:43.3: 13.99 +/- 0.06 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
ZTF J220336.37+420341.5,2461300.8736,13.12,0.05,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
ZTF J220336.37+420341.5 20260917.3736 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 17.3736 2461300.8736 12.05 20:59:56.09 +41:35:19.7
83.56734 -2.93995 galactic Cyg Second-epoch detections are separated by 1.7" and 4.8 pix
The object was found in VSX19" ZTF J205956.87+413536.1
Type: BY
# Max. Min./Amp. JD0 Period
18.091 r Y 0.093 r 2458332.84300 4.908599000000
ATTENTION: measured mag 12.05 is 5.9 mag brighter than the VSX record maximum brightness 18.00 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:56.09 +41:35:19.7: 13.28 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:56.09 +41:35:19.7: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205956.87+413536.1,2461300.8736,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205956.87+413536.1 20260917.3736 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.77 20:58:54.10 +41:23:20.7
83.28933 -2.92450 galactic Cyg Second-epoch detections are separated by 1.5" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:54.10 +41:23:20.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:54.10 +41:23:20.7: 14.31 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:54.10 +41:23:20.7: 14.49 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.39 +/- 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,2461300.8736,12.77,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.05 20:55:49.47 +41:27:16.5
82.96371 -2.44360 galactic Cyg Second-epoch detections are separated by 0.6" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:49.47 +41:27:16.5 (user input) | T | P | (position from user input) J-Ks=0.605+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:49.47 +41:27:16.5: 13.29 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:49.47 +41:27:16.5: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461300.8736,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.28 20:57:14.99 +42:59:56.5
84.31126 -1.64275 galactic Cyg Second-epoch detections are separated by 1.6" and 4.3 pix
The object was found in VSX 3" ASASSN-V J205714.70+425956.6
Type: SR
# Max. Min./Amp. JD0 Period
14.550 V 14.710 V 2458001.00000 460.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:14.99 +42:59:56.5: 13.31 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:14.99 +42:59:56.5: 13.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205714.70+425956.6,2461300.8736,12.28,0.05,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
ASASSN-V J205714.70+425956.6 20260917.3736 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 17.3736 2461300.8736 12.37 22:04:04.04 +42:08:35.6
92.70831 -10.69919 galactic Lac Second-epoch detections are separated by 0.7" and 4.9 pix
The object was found in VSX10" Gaia DR3 1959897176076125568
Type: ROT
# Max. Min./Amp. JD0 Period
17.110 G 17.160 G K
ATTENTION: measured mag 12.37 is 4.7 mag brighter than the VSX record maximum brightness 17.11 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:04.04 +42:08:35.6: 13.27 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:04.04 +42:08:35.6: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1959897176076125568,2461300.8736,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1959897176076125568 20260917.3736 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 17.3736 2461300.8736 12.23 20:55:45.50 +42:13:26.2
83.54297 -1.93664 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9372+42.2226 | 20:55:45.50 +42:13:26.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.411+/-0.034 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:45.50 +42:13:26.2: 13.26 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:45.50 +42:13:26.2: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.9372+42.2226,2461300.8736,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.9372+42.2226 20260917.3736 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 17.3736 2461300.8736 12.73 21:00:59.48 +42:16:48.9
84.21830 -2.63343 galactic Cyg Second-epoch detections are separated by 0.9" and 4.6 pix
The object was found in VSX25" Gaia DR3 2161740946561635072
Type: E
# Max. Min./Amp. JD0 Period
19.690 G 20.490 G 4.364580000000
ATTENTION: measured mag 12.73 is 7.0 mag brighter than the VSX record maximum brightness 19.69 - 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-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:59.48 +42:16:48.9: 14.24 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:59.48 +42:16:48.9: 14.01 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161740946561635072,2461300.8736,12.73,0.05,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 2161740946561635072 20260917.3736 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 17.3736 2461300.8736 12.30 21:00:31.35 +42:02:48.8
83.98518 -2.72163 galactic Cyg Second-epoch detections are separated by 3.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1261+42.0479 | 21:00:31.35 +42:02:48.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:31.35 +42:02:48.8: 13.27 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:31.35 +42:02:48.8: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1261+42.0479,2461300.8736,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1261+42.0479 20260917.3736 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 17.3736 2461300.8736 12.97 20:56:57.52 +41:35:33.4
83.20662 -2.51586 galactic Cyg Second-epoch detections are separated by 3.9" 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 | ATO J314.2400+41.5922 | 20:56:57.52 +41:35:33.4 (user input) | STOCH (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.549+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:57.52 +41:35:33.4: 14.26 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:57.52 +41:35:33.4: 14.59 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.2400+41.5922,2461300.8736,12.97,0.05,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 J314.2400+41.5922 20260917.3736 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 17.3736 2461300.8736 12.53 20:59:37.07 +41:23:51.2
83.38376 -3.02051 galactic Cyg Second-epoch detections are separated by 2.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:37.07 +41:23:51.2 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:37.07 +41:23:51.2: 14.26 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:37.07 +41:23:51.2: 14.08 +/- 0.08 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
target,2461300.8736,12.53,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.37 20:55:07.44 +42:54:33.0
83.99065 -1.40473 galactic Cyg Second-epoch detections are separated by 2.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:07.44 +42:54:33.0 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.035 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:07.44 +42:54:33.0: 13.25 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:07.44 +42:54:33.0: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.37,0.05,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 20260917.3736 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 17.3736 2461300.8736 13.04 22:04:06.63 +42:06:29.3
92.69323 -10.73199 galactic Lac Second-epoch detections are separated by 1.6" and 5.1 pix
The object was found in VSX14" Gaia DR3 1959894079400259072
Type: S
# Max. Min./Amp. JD0 Period
17.010 G 17.720 G K
ATTENTION: measured mag 13.04 is 4.0 mag brighter than the VSX record maximum brightness 17.01 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:06.63 +42:06:29.3: 14.22 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:06.63 +42:06:29.3: 14.17 +/- 0.08 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
Gaia DR3 1959894079400259072,2461300.8736,13.04,0.05,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 1959894079400259072 20260917.3736 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 17.3736 2461300.8736 13.19 22:02:05.98 +42:12:46.5
92.45659 -10.42259 galactic Lac Second-epoch detections are separated by 2.3" and 4.4 pix
The object was found in VSX 1" Gaia DR3 1960071719248850816
Type: ROT
# Max. Min./Amp. JD0 Period
13.970 G 14.020 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:02:05.98 +42:12:46.5: 14.24 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:02:05.98 +42:12:46.5: 14.30 +/- 0.08 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
Gaia DR3 1960071719248850816,2461300.8736,13.19,0.05,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
Gaia DR3 1960071719248850816 20260917.3736 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 17.3736 2461300.8736 12.00 21:01:07.05 +42:13:22.9
84.19061 -2.68870 galactic Cyg Second-epoch detections are separated by 4.6" and 5.3 pix
The object was found in VSX 6" NSVS J2101074+421319
Type: M
# Max. Min./Amp. JD0 Period
11.106 R1 Y 0.820 R1 255.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:01:07.05 +42:13:22.9: 13.34 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:01:07.05 +42:13:22.9: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2101074+421319,2461300.8736,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2101074+421319 20260917.3736 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.75 20:56:56.89 +41:32:20.4
83.16453 -2.54917 galactic Cyg Second-epoch detections are separated by 0.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.2364+41.5392 | 20:56:56.89 +41:32:20.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.736+/-0.027 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:56.89 +41:32:20.4: 14.31 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:56.89 +41:32:20.4: 14.23 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.27 +/- 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
ATO J314.2364+41.5392,2461300.8736,12.75,0.05,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
ATO J314.2364+41.5392 20260917.3736 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 17.3736 2461300.8736 11.94 20:57:49.40 +41:51:20.1
83.51160 -2.46740 galactic Cyg Second-epoch detections are separated by 0.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4556+41.8553 | 20:57:49.40 +41:51:20.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.958+/-0.031 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:49.40 +41:51:20.1: 13.28 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:49.40 +41:51:20.1: 13.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.4556+41.8553,2461300.8736,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.4556+41.8553 20260917.3736 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.12 20:58:12.68 +41:56:45.2
83.62725 -2.46329 galactic Cyg Second-epoch detections are separated by 1.5" and 4.7 pix
The object was found in VSX18" ZTF J205814.05+415655.1
Type: EW
# Max. Min./Amp. JD0 Period
17.895 r Y 0.110 r 2458306.88380 0.362051000000
ATTENTION: measured mag 12.12 is 5.7 mag brighter than the VSX record maximum brightness 17.79 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:12.68 +41:56:45.2: 13.26 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:12.68 +41:56:45.2: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205814.05+415655.1,2461300.8736,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205814.05+415655.1 20260917.3736 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.27 20:59:06.45 +42:01:23.2
83.79468 -2.53891 galactic Cyg Second-epoch detections are separated by 2.2" 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 | 20:59:06.45 +42:01:23.2 (user input) | T | P | (position from user input) J-Ks=0.239+/-0.039 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:06.45 +42:01:23.2: 13.26 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:06.45 +42:01:23.2: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 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,2461300.8736,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.34 21:02:26.39 +41:04:28.0
83.49000 -3.63257 galactic Cyg Second-epoch detections are separated by 1.4" and 4.9 pix
The object was found in VSX16" ZTF J210226.21+410412.5
Type: SR
# Max. Min./Amp. JD0 Period
16.122 r Y 0.113 r 2458257.77350 31.868914000000
ATTENTION: measured mag 12.34 is 3.7 mag brighter than the VSX record maximum brightness 16.01 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:02:26.39 +41:04:28.0: 13.24 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:02:26.39 +41:04:28.0: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210226.21+410412.5,2461300.8736,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210226.21+410412.5 20260917.3736 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.05 20:58:16.67 +41:52:25.6
83.58062 -2.51970 galactic Cyg Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:16.67 +41:52:25.6 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.045 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:16.67 +41:52:25.6: 13.23 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:16.67 +41:52:25.6: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461300.8736,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.36 22:16:49.85 +44:53:45.0
96.25063 -9.81800 galactic Lac Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:49.85 +44:53:45.0 (user input) | T | P | (position from user input) J-Ks=1.035+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:49.85 +44:53:45.0: 13.23 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:49.85 +44:53:45.0: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.28 22:16:39.87 +45:00:05.2
96.28645 -9.71420 galactic Lac Second-epoch detections are separated by 0.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.1660+45.0014 | 22:16:39.87 +45:00:05.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.121+/-0.033 (A)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:39.87 +45:00:05.2: 13.24 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:39.87 +45:00:05.2: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.1660+45.0014,2461300.8736,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.1660+45.0014 20260917.3736 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 17.3736 2461300.8736 12.15 20:55:49.15 +42:10:30.4
83.51300 -1.97682 galactic Cyg Second-epoch detections are separated by 1.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9580+42.1736 | 20:55:49.15 +42:10:30.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.451+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:49.15 +42:10:30.4: 13.25 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:49.15 +42:10:30.4: 13.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 J313.9580+42.1736,2461300.8736,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.9580+42.1736 20260917.3736 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.21 20:57:47.51 +42:11:08.9
83.75855 -2.24785 galactic Cyg Second-epoch detections are separated by 1.0" and 4.6 pix
The object was found in VSX 1" Gaia DR3 2065720600407099648
Type: ROT
# Max. Min./Amp. JD0 Period
12.970 G 13.000 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:47.51 +42:11:08.9: 13.25 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:47.51 +42:11:08.9: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065720600407099648,2461300.8736,12.21,0.05,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 2065720600407099648 20260917.3736 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 17.3736 2461300.8736 12.20 22:18:47.29 +44:55:33.8
96.55901 -9.98749 galactic Lac Second-epoch detections are separated by 0.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:18:47.29 +44:55:33.8 (user input) | T | P | (position from user input) J-Ks=0.819+/-0.027 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:18:47.29 +44:55:33.8: 13.10 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:18:47.29 +44:55:33.8: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.20,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.22 20:57:41.47 +42:43:43.1
84.15857 -1.88015 galactic Cyg Second-epoch detections are separated by 1.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:41.47 +42:43:43.1 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:41.47 +42:43:43.1: 13.23 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:41.47 +42:43:43.1: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 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,2461300.8736,12.22,0.05,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
target 20260917.3736 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 17.3736 2461300.8736 12.29 22:02:15.09 +42:11:54.7
92.47034 -10.45113 galactic Lac Second-epoch detections are separated by 1.4" 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 | 22:02:15.09 +42:11:54.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:02:15.09 +42:11:54.7: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:02:15.09 +42:11:54.7: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 11.98 20:56:40.49 +41:29:56.6
83.10087 -2.53616 galactic Cyg Second-epoch detections are separated by 1.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:40.49 +41:29:56.6 (user input) | T | P | (position from user input) J-Ks=1.039+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:40.49 +41:29:56.6: 13.22 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:40.49 +41:29:56.6: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.22 22:19:39.17 +44:58:06.5
96.71202 -10.03749 galactic Lac Second-epoch detections are separated by 0.2" and 4.8 pix
The object was found in VSX10" Gaia DR3 1962106026217406080
Type: ROT
# Max. Min./Amp. JD0 Period
14.190 G 14.210 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:39.17 +44:58:06.5: 13.23 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:39.17 +44:58:06.5: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1962106026217406080,2461300.8736,12.22,0.05,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 1962106026217406080 20260917.3736 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 17.3736 2461300.8736 12.11 20:58:58.13 +41:48:30.3
83.61523 -2.65985 galactic Cyg Second-epoch detections are separated by 2.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:58.13 +41:48:30.3 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:58.13 +41:48:30.3: 13.19 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:58.13 +41:48:30.3: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 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,2461300.8736,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.28 22:16:38.46 +44:52:58.0
96.21499 -9.80980 galactic Lac Second-epoch detections are separated by 2.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:38.46 +44:52:58.0 (user input) | T | P | (position from user input) J-Ks=0.451+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:38.46 +44:52:58.0: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:38.46 +44:52:58.0: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.28 22:03:36.58 +42:00:42.4
92.55855 -10.75249 galactic Lac Second-epoch detections are separated by 0.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.8932+42.0077 | 22:03:36.58 +42:00:42.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.471+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:03:36.58 +42:00:42.4: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:03:36.58 +42:00:42.4: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.8932+42.0077,2461300.8736,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.8932+42.0077 20260917.3736 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 17.3736 2461300.8736 11.96 20:57:47.57 +41:34:46.0
83.29813 -2.64292 galactic Cyg Second-epoch detections are separated by 0.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4535+41.5825 | 20:57:47.57 +41:34:46.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.354+/-0.043 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:47.57 +41:34:46.0: 13.24 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:47.57 +41:34:46.0: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.4535+41.5825,2461300.8736,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.4535+41.5825 20260917.3736 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.28 20:56:46.73 +42:50:45.8
84.13889 -1.67664 galactic Cyg Second-epoch detections are separated by 2.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:46.73 +42:50:45.8 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.037 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:46.73 +42:50:45.8: 13.19 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:46.73 +42:50:45.8: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 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,2461300.8736,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.16 20:58:43.11 +42:05:30.7
83.79947 -2.43933 galactic Cyg Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6796+42.0919 | 20:58:43.11 +42:05:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.381+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:43.11 +42:05:30.7: 13.20 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:43.11 +42:05:30.7: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.6796+42.0919,2461300.8736,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.6796+42.0919 20260917.3736 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.98 20:56:27.78 +41:58:25.6
83.43692 -2.19824 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:27.78 +41:58:25.6 (user input) | T | P | (position from user input) J-Ks=11.752+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:27.78 +41:58:25.6: 13.18 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:27.78 +41:58:25.6: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.12 22:18:37.57 +44:55:40.4
96.53590 -9.96995 galactic Lac Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:18:37.57 +44:55:40.4 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:18:37.57 +44:55:40.4: 14.22 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:18:37.57 +44:55:40.4: 14.20 +/- 0.09 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,2461300.8736,13.12,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.24 20:59:34.26 +42:31:52.8
84.23525 -2.27081 galactic Cyg Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.8930+42.5314 | 20:59:34.26 +42:31:52.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.392+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:34.26 +42:31:52.8: 13.19 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:34.26 +42:31:52.8: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.8930+42.5314,2461300.8736,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.8930+42.5314 20260917.3736 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 17.3736 2461300.8736 12.04 20:58:18.93 +42:31:21.1
84.07714 -2.10162 galactic Cyg Second-epoch detections are separated by 0.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5789+42.5225 | 20:58:18.93 +42:31:21.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.859+/-0.033 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:18.93 +42:31:21.1: 13.19 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:18.93 +42:31:21.1: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.5789+42.5225,2461300.8736,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5789+42.5225 20260917.3736 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 17.3736 2461300.8736 13.09 22:04:45.95 +41:55:14.0
92.67681 -10.95502 galactic Lac Second-epoch detections are separated by 1.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:45.95 +41:55:14.0 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.034 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:45.95 +41:55:14.0: 14.24 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:45.95 +41:55:14.0: 14.18 +/- 0.08 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,2461300.8736,13.09,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.18 22:16:58.49 +44:53:47.8
96.27245 -9.83174 galactic Lac Second-epoch detections are separated by 0.1" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.2411+44.8907 | 22:16:58.49 +44:53:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.555+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:58.49 +44:53:47.8: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:58.49 +44:53:47.8: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.2411+44.8907,2461300.8736,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J334.2411+44.8907 20260917.3736 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.87 20:56:28.25 +41:51:52.0
83.35455 -2.27023 galactic Cyg Second-epoch detections are separated by 0.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:28.25 +41:51:52.0 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.037 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:28.25 +41:51:52.0: 13.15 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:28.25 +41:51:52.0: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 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,2461300.8736,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.22 22:17:08.62 +45:04:57.8
96.40386 -9.69478 galactic Lac Second-epoch detections are separated by 0.5" and 4.9 pix
The object was found in VSX16" ZTF J221709.30+450512.5
Type: BY
# Max. Min./Amp. JD0 Period
16.730 r Y 0.074 r 2458607.97890 2.329554800000
ATTENTION: measured mag 12.22 is 4.4 mag brighter than the VSX record maximum brightness 16.66 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:08.62 +45:04:57.8: 13.15 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:08.62 +45:04:57.8: 13.17 +/- 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
ZTF J221709.30+450512.5,2461300.8736,12.22,0.05,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
ZTF J221709.30+450512.5 20260917.3736 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 17.3736 2461300.8736 12.60 20:58:29.51 +41:54:14.2
83.62952 -2.53019 galactic Cyg Second-epoch detections are separated by 0.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6215+41.9036 | 20:58:29.51 +41:54:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:29.51 +41:54:14.2: 14.15 +/- 0.12 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:29.51 +41:54:14.2: 14.03 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.08 +/- 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
ATO J314.6215+41.9036,2461300.8736,12.60,0.05,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 J314.6215+41.9036 20260917.3736 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 17.3736 2461300.8736 12.13 20:59:16.63 +42:15:24.9
83.99220 -2.40964 galactic Cyg Second-epoch detections are separated by 1.4" and 4.8 pix
The object was found in VSX17" ZTF J205916.91+421508.1
Type: RS
# Max. Min./Amp. JD0 Period
20.247 g Y 0.331 g 2458425.61250 0.874710500000
ATTENTION: measured mag 12.13 is 7.8 mag brighter than the VSX record maximum brightness 19.92 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:16.63 +42:15:24.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:16.63 +42:15:24.9: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205916.91+421508.1,2461300.8736,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205916.91+421508.1 20260917.3736 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.79 20:58:36.15 +41:37:09.6
83.42722 -2.73167 galactic Cyg Second-epoch detections are separated by 2.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:36.15 +41:37:09.6 (user input) | T | P | (position from user input) J-Ks=0.489+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:36.15 +41:37:09.6: 14.25 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:36.15 +41:37:09.6: 14.19 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.22 +/- 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,2461300.8736,12.79,0.05,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 20260917.3736 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 17.3736 2461300.8736 13.01 22:16:45.86 +44:55:37.8
96.25871 -9.78549 galactic Lac Second-epoch detections are separated by 2.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:45.86 +44:55:37.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:45.86 +44:55:37.8: 14.17 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:45.86 +44:55:37.8: 14.10 +/- 0.07 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,2461300.8736,13.01,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.15 20:55:56.05 +42:48:25.4
84.00873 -1.58401 galactic Cyg Second-epoch detections are separated by 1.1" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9810+42.8098 | 20:55:56.05 +42:48:25.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.336+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:56.05 +42:48:25.4: 13.13 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:56.05 +42:48:25.4: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.9810+42.8098,2461300.8736,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.9810+42.8098 20260917.3736 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.11 20:56:41.50 +42:23:13.5
83.77918 -1.96239 galactic Cyg Second-epoch detections are separated by 1.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:41.50 +42:23:13.5 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:41.50 +42:23:13.5: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:41.50 +42:23:13.5: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.82 20:57:22.42 +41:31:07.2
83.20085 -2.62292 galactic Cyg Second-epoch detections are separated by 2.8" 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 | 20:57:22.42 +41:31:07.2 (user input) | T | P | (position from user input) J-Ks=0.873+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:22.42 +41:31:07.2: 14.21 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:22.42 +41:31:07.2: 14.48 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.31 +/- 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,2461300.8736,12.82,0.05,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 20260917.3736 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 17.3736 2461300.8736 13.11 22:03:39.75 +42:03:06.8
92.59122 -10.72651 galactic Lac Second-epoch detections are separated by 0.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:39.75 +42:03:06.8 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.034 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:03:39.75 +42:03:06.8: 14.18 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:03:39.75 +42:03:06.8: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.25 +/- 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,2461300.8736,13.11,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.94 20:59:00.38 +41:54:16.0
83.69252 -2.60233 galactic Cyg Second-epoch detections are separated by 3.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.7455+41.8997 | 20:58:59.57 +41:53:33.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:00.38 +41:54:16.0: 13.01 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:00.38 +41:54:16.0: 13.03 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.7455+41.8997,2461300.8736,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.7455+41.8997 20260917.3736 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.06 20:59:39.77 +42:13:37.8
84.01652 -2.48305 galactic Cyg Second-epoch detections are separated by 1.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161749300278490240 | 20:59:42.75 +42:14:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.421+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:39.77 +42:13:37.8: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:39.77 +42:13:37.8: 13.08 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161749300278490240,2461300.8736,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161749300278490240 20260917.3736 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.20 20:59:31.38 +42:28:23.5
84.18550 -2.30224 galactic Cyg Second-epoch detections are separated by 1.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.8955+42.4792 | 20:59:31.38 +42:28:23.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.711+/-0.034 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:31.38 +42:28:23.5: 13.11 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:31.38 +42:28:23.5: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.8955+42.4792,2461300.8736,12.20,0.05,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 J314.8955+42.4792 20260917.3736 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 17.3736 2461300.8736 12.18 22:19:25.06 +44:51:13.3
96.61204 -10.10972 galactic Lac Second-epoch detections are separated by 0.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:25.06 +44:51:13.3 (user input) | T | P | (position from user input) J-Ks=0.744+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:25.06 +44:51:13.3: 13.08 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:25.06 +44:51:13.3: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.83 20:55:53.60 +41:44:23.8
83.18986 -2.26885 galactic Cyg Second-epoch detections are separated by 0.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:53.60 +41:44:23.8 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:53.60 +41:44:23.8: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:53.60 +41:44:23.8: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.08 22:04:37.92 +41:49:51.5
92.60155 -11.01147 galactic Lac Second-epoch detections are separated by 0.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J331.1582+41.8279 | 22:04:37.92 +41:49:51.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.732+/-0.034 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:37.92 +41:49:51.5: 14.19 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:37.92 +41:49:51.5: 14.22 +/- 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
ATO J331.1582+41.8279,2461300.8736,13.08,0.05,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 J331.1582+41.8279 20260917.3736 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 17.3736 2461300.8736 11.77 20:57:13.03 +41:26:00.0
83.11686 -2.65611 galactic Cyg Second-epoch detections are separated by 0.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.2875+41.4218 | 20:57:09.65 +41:25:55.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.570+/-0.034 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:13.03 +41:26:00.0: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:13.03 +41:26:00.0: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.2875+41.4218,2461300.8736,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.2875+41.4218 20260917.3736 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.78 20:56:45.10 +41:37:22.7
83.20460 -2.46671 galactic Cyg Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.1880+41.6230 | 20:56:45.10 +41:37:22.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.298+/-0.027 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:45.10 +41:37:22.7: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:45.10 +41:37:22.7: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.1880+41.6230,2461300.8736,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.1880+41.6230 20260917.3736 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.80 20:57:45.49 +41:31:36.4
83.25389 -2.67229 galactic Cyg Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4389+41.5269 | 20:57:45.49 +41:31:36.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.551+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:45.49 +41:31:36.4: 14.18 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:45.49 +41:31:36.4: 14.32 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 J314.4389+41.5269,2461300.8736,12.80,0.05,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 J314.4389+41.5269 20260917.3736 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 17.3736 2461300.8736 11.81 20:56:13.24 +41:42:57.4
83.21112 -2.33094 galactic Cyg Second-epoch detections are separated by 0.5" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.0596+41.7175 | 20:56:13.24 +41:42:57.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.324+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:13.24 +41:42:57.4: 13.07 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:13.24 +41:42:57.4: 13.10 +/- 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
ATO J314.0596+41.7175,2461300.8736,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.0596+41.7175 20260917.3736 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.63 20:58:50.42 +41:22:12.9
83.26753 -2.92810 galactic Cyg Second-epoch detections are separated by 2.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:50.42 +41:22:12.9 (user input) | T | P | (position from user input) J-Ks=0.903+/-0.027 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:50.42 +41:22:12.9: 14.15 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:50.42 +41:22:12.9: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461300.8736,12.63,0.05,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
target 20260917.3736 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 17.3736 2461300.8736 11.57 20:57:40.11 +41:57:04.3
83.56544 -2.38327 galactic Cyg Second-epoch detections are separated by 1.9" and 5.0 pix
The object was found in VSX 5" NSVS 5877962
Type: SR
# Max. Min./Amp. JD0 Period
12.994 r Y 0.430 r 2458482.07930 133.369166600000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:40.11 +41:57:04.3: 13.06 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:40.11 +41:57:04.3: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5877962,2461300.8736,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 5877962 20260917.3736 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.69 20:59:07.64 +41:35:10.4
83.46634 -2.82756 galactic Cyg Second-epoch detections are separated by 0.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.7814+41.5863 | 20:59:07.64 +41:35:10.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.930+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:07.64 +41:35:10.4: 14.14 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:07.64 +41:35:10.4: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 J314.7814+41.5863,2461300.8736,12.69,0.05,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 J314.7814+41.5863 20260917.3736 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 17.3736 2461300.8736 12.10 22:16:46.95 +44:58:33.9
96.28941 -9.74691 galactic Lac Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:46.95 +44:58:33.9 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:46.95 +44:58:33.9: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:46.95 +44:58:33.9: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.04 22:01:11.78 +42:14:35.7
92.34079 -10.29646 galactic Lac Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:01:11.78 +42:14:35.7 (user input) | T | P | (position from user input) J-Ks=0.553+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:01:11.78 +42:14:35.7: 14.15 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:01:11.78 +42:14:35.7: 14.22 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,13.04,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.20 22:01:38.84 +42:14:35.6
92.40792 -10.34749 galactic Lac Second-epoch detections are separated by 0.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.3968+42.2499 | 22:01:38.84 +42:14:35.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.416+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:01:38.84 +42:14:35.6: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:01:38.84 +42:14:35.6: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J330.3968+42.2499,2461300.8736,12.20,0.05,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 J330.3968+42.2499 20260917.3736 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 17.3736 2461300.8736 11.87 20:55:23.75 +41:57:15.6
83.29362 -2.05958 galactic Cyg Second-epoch detections are separated by 0.6" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:23.75 +41:57:15.6 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:23.75 +41:57:15.6: 13.05 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:23.75 +41:57:15.6: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.98 20:57:02.78 +42:06:31.1
83.60993 -2.19311 galactic Cyg Second-epoch detections are separated by 1.1" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:02.78 +42:06:31.1 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.032 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:02.78 +42:06:31.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:02.78 +42:06:31.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.80 20:56:09.14 +41:56:56.9
83.38069 -2.17022 galactic Cyg Second-epoch detections are separated by 0.5" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:09.14 +41:56:56.9 (user input) | T | P | (position from user input) J-Ks=0.292+/-0.031 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:09.14 +41:56:56.9: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:09.14 +41:56:56.9: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.04 21:00:42.16 +42:08:09.5
84.07436 -2.68820 galactic Cyg Second-epoch detections are separated by 2.2" and 4.8 pix
The object was found in VSX 1" Gaia DR3 2161738339521760768
Type: RS
# Max. Min./Amp. JD0 Period
12.680 G 12.730 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:42.16 +42:08:09.5: 13.03 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:42.16 +42:08:09.5: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161738339521760768,2461300.8736,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161738339521760768 20260917.3736 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 17.3736 2461300.8736 12.07 22:16:31.78 +44:52:39.1
96.19546 -9.80299 galactic Lac Second-epoch detections are separated by 0.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:31.78 +44:52:39.1 (user input) | T | P | (position from user input) J-Ks=0.822+/-0.027 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:31.78 +44:52:39.1: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:31.78 +44:52:39.1: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.06 20:59:33.37 +42:10:02.5
83.95835 -2.50734 galactic Cyg Second-epoch detections are separated by 1.9" and 5.0 pix
The object was found in VSX 4" Gaia DR3 2161747994608415232
Type: YSO
# Max. Min./Amp. JD0 Period
13.730 G 13.760 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:33.37 +42:10:02.5: 13.03 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:33.37 +42:10:02.5: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161747994608415232,2461300.8736,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161747994608415232 20260917.3736 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.94 20:59:22.47 +42:17:42.2
84.03285 -2.39826 galactic Cyg Second-epoch detections are separated by 1.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.8326+42.2971 | 20:59:22.47 +42:17:42.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.398+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:22.47 +42:17:42.2: 13.03 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:22.47 +42:17:42.2: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.8326+42.2971,2461300.8736,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.8326+42.2971 20260917.3736 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.82 20:54:54.95 +41:57:11.0
83.23502 -1.99223 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.7167+41.9547 | 20:54:54.95 +41:57:11.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.322+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:54.95 +41:57:11.0: 13.02 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:54.95 +41:57:11.0: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.7167+41.9547,2461300.8736,11.82,0.05,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 J313.7167+41.9547 20260917.3736 11.82CV 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 17.3736 2461300.8736 13.15 22:15:41.47 +45:01:41.4
96.15793 -9.59483 galactic Lac Second-epoch detections are separated by 2.4" and 5.1 pix
The object was found in VSX 1" Gaia DR3 1962221715456843008
Type: ROT
# Max. Min./Amp. JD0 Period
13.770 G 13.820 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:41.47 +45:01:41.4: 14.14 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:41.47 +45:01:41.4: 14.21 +/- 0.08 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
Gaia DR3 1962221715456843008,2461300.8736,13.15,0.05,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
Gaia DR3 1962221715456843008 20260917.3736 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 17.3736 2461300.8736 11.88 20:57:49.40 +42:02:53.3
83.65782 -2.34196 galactic Cyg Second-epoch detections are separated by 0.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4520+42.0456 | 20:57:49.40 +42:02:53.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.376+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:49.40 +42:02:53.3: 12.98 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:49.40 +42:02:53.3: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.4520+42.0456,2461300.8736,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.4520+42.0456 20260917.3736 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.79 20:57:14.11 +42:01:20.3
83.56706 -2.27585 galactic Cyg Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3030+42.0193 | 20:57:14.02 +42:01:19.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.164+/-0.034 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:14.11 +42:01:20.3: 13.01 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:14.11 +42:01:20.3: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.3030+42.0193,2461300.8736,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.3030+42.0193 20260917.3736 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.61 20:55:05.67 +42:03:37.2
83.33847 -1.94840 galactic Cyg Second-epoch detections are separated by 1.2" and 4.9 pix
The object was found in VSX 4" ZTF J205505.30+420335.3
Type: SR
# Max. Min./Amp. JD0 Period
13.868 r Y 0.199 r 2458365.49350 42.046723300000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:05.67 +42:03:37.2: 14.07 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:05.67 +42:03:37.2: 14.03 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205505.30+420335.3,2461300.8736,12.61,0.05,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
ZTF J205505.30+420335.3 20260917.3736 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 17.3736 2461300.8736 12.82 20:56:15.78 +41:08:56.4
82.78383 -2.70413 galactic Cyg Second-epoch detections are separated by 2.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.0653+41.1491 | 20:56:15.78 +41:08:56.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.628+/-0.038 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:15.78 +41:08:56.4: 14.11 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:15.78 +41:08:56.4: 14.38 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.21 +/- 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 J314.0653+41.1491,2461300.8736,12.82,0.05,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 J314.0653+41.1491 20260917.3736 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 17.3736 2461300.8736 12.67 20:58:30.68 +41:48:13.2
83.55586 -2.59841 galactic Cyg Second-epoch detections are separated by 3.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6352+41.7956 | 20:58:30.68 +41:48:13.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.629+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:30.68 +41:48:13.2: 14.13 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:30.68 +41:48:13.2: 14.37 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.22 +/- 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
ATO J314.6352+41.7956,2461300.8736,12.67,0.05,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 J314.6352+41.7956 20260917.3736 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 17.3736 2461300.8736 11.66 20:58:22.97 +41:53:43.5
83.60980 -2.52039 galactic Cyg Second-epoch detections are separated by 1.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5948+41.8952 | 20:58:22.77 +41:53:42.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.385+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:22.97 +41:53:43.5: 12.99 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:22.97 +41:53:43.5: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 J314.5948+41.8952,2461300.8736,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5948+41.8952 20260917.3736 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.74 20:58:23.91 +42:35:14.8
84.13634 -2.07082 galactic Cyg Second-epoch detections are separated by 0.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161818638231602176 | 20:58:23.57 +42:35:10.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2.5V 2015A&A...577A.128A G 212- 12
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:23.91 +42:35:14.8: 12.97 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:23.91 +42:35:14.8: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 2161818638231602176,2461300.8736,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161818638231602176 20260917.3736 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.78 20:58:05.81 +41:12:50.1
83.05766 -2.92429 galactic Cyg Second-epoch detections are separated by 1.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5241+41.2141 | 20:58:05.81 +41:12:50.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.913+/-0.033 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:05.81 +41:12:50.1: 14.22 +/- 0.11 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:05.81 +41:12:50.1: 14.19 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.21 +/- 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 J314.5241+41.2141,2461300.8736,12.78,0.05,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 J314.5241+41.2141 20260917.3736 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 17.3736 2461300.8736 13.15 22:17:51.75 +44:46:13.2
96.33243 -10.02467 galactic Lac Second-epoch detections are separated by 0.9" and 4.9 pix
The object was found in VSX14" Gaia DR3 1962015866263380992
Type: ROT
# Max. Min./Amp. JD0 Period
16.950 G 17.050 G K
ATTENTION: measured mag 13.15 is 3.8 mag brighter than the VSX record maximum brightness 16.95 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:51.75 +44:46:13.2: 14.14 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:51.75 +44:46:13.2: 14.26 +/- 0.08 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
Gaia DR3 1962015866263380992,2461300.8736,13.15,0.05,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
Gaia DR3 1962015866263380992 20260917.3736 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 17.3736 2461300.8736 11.81 20:57:39.93 +41:43:10.6
83.38913 -2.53361 galactic Cyg Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:39.93 +41:43:10.6 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:39.93 +41:43:10.6: 12.97 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:39.93 +41:43:10.6: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.86 20:56:39.61 +42:10:22.7
83.61239 -2.09690 galactic Cyg Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:39.61 +42:10:22.7 (user input) | T | P | (position from user input) J-Ks=0.324+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:39.61 +42:10:22.7: 12.96 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:39.61 +42:10:22.7: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.04 20:58:40.93 +42:38:54.0
84.21658 -2.07055 galactic Cyg Second-epoch detections are separated by 1.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6746+42.6464 | 20:58:40.93 +42:38:54.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.366+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:40.93 +42:38:54.0: 12.96 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:40.93 +42:38:54.0: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.6746+42.6464,2461300.8736,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.6746+42.6464 20260917.3736 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 17.3736 2461300.8736 11.95 20:57:38.63 +42:25:57.3
83.92810 -2.06636 galactic Cyg Second-epoch detections are separated by 0.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4108+42.4325 | 20:57:38.63 +42:25:57.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.552+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:38.63 +42:25:57.3: 12.94 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:38.63 +42:25:57.3: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.4108+42.4325,2461300.8736,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.4108+42.4325 20260917.3736 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.89 20:54:56.38 +42:27:16.4
83.62135 -1.67219 galactic Cyg Second-epoch detections are separated by 0.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.7349+42.4545 | 20:54:56.38 +42:27:16.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.417+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:56.38 +42:27:16.4: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:56.38 +42:27:16.4: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.7349+42.4545,2461300.8736,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.7349+42.4545 20260917.3736 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.03 20:54:10.89 +42:56:21.0
83.90237 -1.25346 galactic Cyg Second-epoch detections are separated by 1.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:54:10.89 +42:56:21.0 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:10.89 +42:56:21.0: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:10.89 +42:56:21.0: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.15 22:02:42.05 +42:13:03.4
92.54930 -10.48661 galactic Lac Second-epoch detections are separated by 1.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:42.05 +42:13:03.4 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.050 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:02:42.05 +42:13:03.4: 14.12 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:02:42.05 +42:13:03.4: 14.37 +/- 0.09 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,2461300.8736,13.15,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.75 20:56:23.70 +41:55:38.1
83.39326 -2.21877 galactic Cyg Second-epoch detections are separated by 1.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:23.70 +41:55:38.1 (user input) | T | P | (position from user input) J-Ks=0.665+/-0.026 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:23.70 +41:55:38.1: 14.12 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:23.70 +41:55:38.1: 14.03 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461300.8736,12.75,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.94 20:59:15.00 +42:08:08.2
83.89713 -2.48527 galactic Cyg Second-epoch detections are separated by 0.9" and 4.7 pix
The object was found in VSX 1" Gaia DR3 2161747135614976768
Type: ROT
# Max. Min./Amp. JD0 Period
12.740 G 12.760 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:15.00 +42:08:08.2: 12.88 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:15.00 +42:08:08.2: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161747135614976768,2461300.8736,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161747135614976768 20260917.3736 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.11 22:18:09.88 +44:51:41.6
96.42943 -9.97919 galactic Lac Second-epoch detections are separated by 1.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:18:09.88 +44:51:41.6 (user input) | T | P | (position from user input) J-Ks=0.781+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:18:09.88 +44:51:41.6: 14.08 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:18:09.88 +44:51:41.6: 14.45 +/- 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,2461300.8736,13.11,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.69 20:55:36.69 +41:18:26.2
82.82536 -2.50833 galactic Cyg Second-epoch detections are separated by 0.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:36.69 +41:18:26.2 (user input) | T | P | (position from user input) J-Ks=0.340+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:36.69 +41:18:26.2: 12.90 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:36.69 +41:18:26.2: 12.97 +/- 0.04 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
target,2461300.8736,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.88 20:58:44.69 +42:19:33.4
83.97998 -2.29002 galactic Cyg Second-epoch detections are separated by 0.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:44.69 +42:19:33.4 (user input) | T | P | (position from user input) J-Ks=0.522+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:44.69 +42:19:33.4: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:44.69 +42:19:33.4: 12.83 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 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,2461300.8736,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.65 20:55:40.61 +41:19:25.0
82.84577 -2.50714 galactic Cyg Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065532893155328384 | 20:55:40.46 +41:19:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.332+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:40.61 +41:19:25.0: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:40.61 +41:19:25.0: 12.96 +/- 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
Gaia DR3 2065532893155328384,2461300.8736,11.65,0.05,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
Gaia DR3 2065532893155328384 20260917.3736 11.65CV 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 17.3736 2461300.8736 11.83 20:58:14.27 +42:13:28.4
83.84184 -2.28521 galactic Cyg Second-epoch detections are separated by 1.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5593+42.2247 | 20:58:14.27 +42:13:28.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.348+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:14.27 +42:13:28.4: 12.87 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:14.27 +42:13:28.4: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 J314.5593+42.2247,2461300.8736,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5593+42.2247 20260917.3736 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.66 20:57:26.05 +41:05:44.1
82.88641 -2.90662 galactic Cyg Second-epoch detections are separated by 0.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:26.05 +41:05:44.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:26.05 +41:05:44.1: 14.03 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:26.05 +41:05:44.1: 14.12 +/- 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
target,2461300.8736,12.66,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.71 20:58:05.35 +41:21:50.6
83.17074 -2.82535 galactic Cyg Second-epoch detections are separated by 0.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5168+41.3654 | 20:58:05.23 +41:21:49.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.259+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:05.35 +41:21:50.6: 12.88 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:05.35 +41:21:50.6: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.5168+41.3654,2461300.8736,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5168+41.3654 20260917.3736 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.10 22:16:20.00 +44:49:09.2
96.13288 -9.83141 galactic Lac Second-epoch detections are separated by 1.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:20.00 +44:49:09.2 (user input) | T | P | (position from user input) J-Ks=0.819+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:20.00 +44:49:09.2: 14.06 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:20.00 +44:49:09.2: 14.18 +/- 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,2461300.8736,13.10,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.71 20:58:11.77 +41:19:28.3
83.15383 -2.86635 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:11.77 +41:19:28.3 (user input) | T | P | (position from user input) J-Ks=0.510+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:11.77 +41:19:28.3: 14.07 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:11.77 +41:19:28.3: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.71,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.93 20:55:27.68 +42:22:06.2
83.61771 -1.80136 galactic Cyg Second-epoch detections are separated by 1.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.8616+42.3624 | 20:55:27.68 +42:22:06.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.596+/-0.035 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:27.68 +42:22:06.2: 12.86 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:27.68 +42:22:06.2: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.8616+42.3624,2461300.8736,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.8616+42.3624 20260917.3736 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 17.3736 2461300.8736 12.93 20:57:57.64 +41:36:27.6
83.34003 -2.64835 galactic Cyg Second-epoch detections are separated by 2.7" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:57.64 +41:36:27.6 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:57.64 +41:36:27.6: 14.09 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:57.64 +41:36:27.6: 14.43 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.21 +/- 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,2461300.8736,12.93,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.83 20:58:34.61 +42:03:26.2
83.75608 -2.44202 galactic Cyg Second-epoch detections are separated by 1.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:34.61 +42:03:26.2 (user input) | T | P | (position from user input) J-Ks=0.553+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:34.61 +42:03:26.2: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:34.61 +42:03:26.2: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.78 20:58:10.26 +42:29:24.0
84.03509 -2.10267 galactic Cyg Second-epoch detections are separated by 0.2" and 4.5 pix
The object was found in VSX 0" Gaia DR3 2161804718232818688
Type: ROT
# Max. Min./Amp. JD0 Period
12.610 G 12.640 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:10.26 +42:29:24.0: 12.80 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:10.26 +42:29:24.0: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161804718232818688,2461300.8736,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161804718232818688 20260917.3736 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.73 20:58:59.80 +41:47:43.1
83.60870 -2.67235 galactic Cyg Second-epoch detections are separated by 0.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:59.80 +41:47:43.1 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:59.80 +41:47:43.1: 12.80 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:59.80 +41:47:43.1: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.84 20:59:54.32 +42:04:51.2
83.93551 -2.61293 galactic Cyg Second-epoch detections are separated by 1.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9785+42.0852 | 20:59:54.32 +42:04:51.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.382+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:54.32 +42:04:51.2: 12.80 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:54.32 +42:04:51.2: 12.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.9785+42.0852,2461300.8736,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.9785+42.0852 20260917.3736 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.59 20:55:28.89 +41:54:16.6
83.26594 -2.10386 galactic Cyg Second-epoch detections are separated by 1.4" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:28.89 +41:54:16.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:28.89 +41:54:16.6: 14.07 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:28.89 +41:54:16.6: 14.08 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461300.8736,12.59,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.49 20:55:19.89 +41:23:02.8
82.85010 -2.41859 galactic Cyg Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.8327+41.3838 | 20:55:19.89 +41:23:02.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.992+/-0.033 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:19.89 +41:23:02.8: 14.08 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:19.89 +41:23:02.8: 14.03 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 J313.8327+41.3838,2461300.8736,12.49,0.05,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
ATO J313.8327+41.3838 20260917.3736 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 17.3736 2461300.8736 12.68 20:57:22.47 +41:24:18.3
83.11456 -2.69688 galactic Cyg Second-epoch detections are separated by 1.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3433+41.4051 | 20:57:22.47 +41:24:18.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.464+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:22.47 +41:24:18.3: 14.03 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:22.47 +41:24:18.3: 14.03 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.3433+41.4051,2461300.8736,12.68,0.05,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
ATO J314.3433+41.4051 20260917.3736 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 17.3736 2461300.8736 12.35 21:00:08.60 +41:58:28.7
83.88432 -2.71602 galactic Cyg Second-epoch detections are separated by 1.7" and 4.9 pix
The object was found in VSX 2" ZTF J210008.42+415828.2
Type: SR
# Max. Min./Amp. JD0 Period
13.572 r Y 0.234 r 2458257.12450 31.116381400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:08.60 +41:58:28.7: 14.02 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:08.60 +41:58:28.7: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J210008.42+415828.2,2461300.8736,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210008.42+415828.2 20260917.3736 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 17.3736 2461300.8736 12.85 22:19:18.17 +44:58:06.3
96.65975 -10.00310 galactic Lac Second-epoch detections are separated by 1.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:18.17 +44:58:06.3 (user input) | T | P | (position from user input) J-Ks=0.757+/-0.036 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:18.17 +44:58:06.3: 14.02 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:18.17 +44:58:06.3: 14.09 +/- 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,2461300.8736,12.85,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.79 20:59:12.41 +41:55:47.1
83.73611 -2.61397 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:12.41 +41:55:47.1 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:12.41 +41:55:47.1: 12.76 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:12.41 +41:55:47.1: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.66 20:57:53.52 +41:51:09.7
83.51774 -2.47898 galactic Cyg Second-epoch detections are separated by 3.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:53.52 +41:51:09.7 (user input) | T | P | (position from user input) J-Ks=0.978+/-0.033 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:53.52 +41:51:09.7: 14.08 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:53.52 +41:51:09.7: 14.10 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461300.8736,12.66,0.05,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 20260917.3736 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 17.3736 2461300.8736 13.03 22:17:34.86 +44:11:40.0
95.96125 -10.47273 galactic Lac Second-epoch detections are separated by 2.6" 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 | 22:17:34.86 +44:11:40.0 (user input) | T | P | (position from user input) J-Ks=0.552+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:34.86 +44:11:40.0: 14.02 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:34.86 +44:11:40.0: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,13.03,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.65 20:58:36.39 +41:31:56.9
83.36185 -2.78895 galactic Cyg Second-epoch detections are separated by 2.4" 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 | 20:58:36.39 +41:31:56.9 (user input) | T | P | (position from user input) J-Ks=0.577+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:36.39 +41:31:56.9: 14.05 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:36.39 +41:31:56.9: 14.24 +/- 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
target,2461300.8736,12.65,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.64 20:54:40.40 +42:05:49.7
83.31620 -1.86493 galactic Cyg Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.6685+42.0971 | 20:54:40.40 +42:05:49.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.399+/-0.038 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:40.40 +42:05:49.7: 12.73 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:40.40 +42:05:49.7: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.6685+42.0971,2461300.8736,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.6685+42.0971 20260917.3736 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.79 20:57:28.30 +41:43:39.1
83.37159 -2.50099 galactic Cyg Second-epoch detections are separated by 2.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3663+41.7246 | 20:57:28.30 +41:43:39.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.668+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:28.30 +41:43:39.1: 14.04 +/- 0.10 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:28.30 +41:43:39.1: 14.29 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.13 +/- 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
ATO J314.3663+41.7246,2461300.8736,12.79,0.05,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 J314.3663+41.7246 20260917.3736 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 17.3736 2461300.8736 11.47 20:57:22.01 +41:43:35.2
83.35803 -2.48684 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was found in VSX15" Gaia DR3 2065638068314088576
Type: ROT
# Max. Min./Amp. JD0 Period
14.900 G 14.920 G K
ATTENTION: measured mag 11.47 is 3.4 mag brighter than the VSX record maximum brightness 14.90 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:22.01 +41:43:35.2: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:22.01 +41:43:35.2: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065638068314088576,2461300.8736,11.47,0.05,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 2065638068314088576 20260917.3736 11.47CV 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 17.3736 2461300.8736 11.71 20:55:12.97 +42:36:18.6
83.76934 -1.61391 galactic Cyg Second-epoch detections are separated by 0.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.8035+42.6051 | 20:55:12.86 +42:36:18.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.087+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:12.97 +42:36:18.6: 12.73 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:12.97 +42:36:18.6: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.8035+42.6051,2461300.8736,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.8035+42.6051 20260917.3736 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.73 20:56:27.57 +42:32:59.9
83.87541 -1.82413 galactic Cyg Second-epoch detections are separated by 1.1" and 4.8 pix
The object was found in VSX19" Gaia DR3 2065931328680938240
Type: YSO
# Max. Min./Amp. JD0 Period
17.360 G 17.510 G K
ATTENTION: measured mag 11.73 is 5.6 mag brighter than the VSX record maximum brightness 17.36 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:27.57 +42:32:59.9: 12.70 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:27.57 +42:32:59.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065931328680938240,2461300.8736,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065931328680938240 20260917.3736 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.75 20:57:59.10 +42:39:28.6
84.14013 -1.96717 galactic Cyg Second-epoch detections are separated by 1.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4993+42.6537 | 20:57:57.65 +42:38:51.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F/G 1952IzKry...9...82G BD+42 3921 J-Ks=0.397+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:59.10 +42:39:28.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:59.10 +42:39:28.6: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 J314.4993+42.6537,2461300.8736,11.75,0.05,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
ATO J314.4993+42.6537 20260917.3736 11.75CV 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 17.3736 2461300.8736 12.49 20:55:38.01 +41:37:59.2
83.07691 -2.30092 galactic Cyg Second-epoch detections are separated by 1.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:38.01 +41:37:59.2 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:38.01 +41:37:59.2: 14.02 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:38.01 +41:37:59.2: 14.07 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.05 +/- 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,2461300.8736,12.49,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.71 20:58:40.76 +42:40:09.5
84.23212 -2.05644 galactic Cyg Second-epoch detections are separated by 0.6" and 4.5 pix
The object was found in VSX 0" Gaia DR3 2161824822984514304
Type: ROT
# Max. Min./Amp. JD0 Period
12.450 G 12.480 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:40.76 +42:40:09.5: 12.67 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:40.76 +42:40:09.5: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161824822984514304,2461300.8736,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161824822984514304 20260917.3736 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.99 22:16:04.85 +45:09:26.9
96.28969 -9.52725 galactic Lac Second-epoch detections are separated by 2.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:04.85 +45:09:26.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:04.85 +45:09:26.9: 14.01 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:04.85 +45:09:26.9: 13.94 +/- 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,2461300.8736,12.99,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.69 20:55:25.87 +42:16:36.2
83.54410 -1.85633 galactic Cyg Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065898686930077056 | 20:55:25.91 +42:16:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.367+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:25.87 +42:16:36.2: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:25.87 +42:16:36.2: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065898686930077056,2461300.8736,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065898686930077056 20260917.3736 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.50 20:56:12.00 +41:09:26.8
82.78259 -2.68962 galactic Cyg Second-epoch detections are separated by 0.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065527356937406720 | 20:56:12.00 +41:09:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.387+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:12.00 +41:09:26.8: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:12.00 +41:09:26.8: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 2065527356937406720,2461300.8736,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065527356937406720 20260917.3736 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.54 20:55:52.48 +41:50:26.5
83.26449 -2.20102 galactic Cyg Second-epoch detections are separated by 3.0" and 4.8 pix
The object was found in VSX 1" Gaia DR3 2065701015355929088
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-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:52.48 +41:50:26.5: 13.99 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:52.48 +41:50:26.5: 13.76 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065701015355929088,2461300.8736,12.54,0.05,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
Gaia DR3 2065701015355929088 20260917.3736 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 17.3736 2461300.8736 11.45 20:55:39.24 +41:16:53.8
82.81091 -2.53101 galactic Cyg Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065532686996891264 | 20:55:39.14 +41:16:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.942+/-0.034 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:39.24 +41:16:53.8: 12.64 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:39.24 +41:16:53.8: 12.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065532686996891264,2461300.8736,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065532686996891264 20260917.3736 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.62 20:57:51.63 +42:30:51.2
84.01612 -2.04349 galactic Cyg Second-epoch detections are separated by 0.7" and 4.7 pix
The object was found in VSX13" WISE J205752.3+423101
Type: EW|EA
# Max. Min./Amp. JD0 Period
12.208 W1 Y 0.474 W1 0.710241800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:51.63 +42:30:51.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:51.63 +42:30:51.2: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J205752.3+423101,2461300.8736,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J205752.3+423101 20260917.3736 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.62 20:57:35.05 +42:07:09.9
83.68304 -2.26187 galactic Cyg Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065719947572151552 | 20:57:35.04 +42:07:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.347+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:35.05 +42:07:09.9: 12.61 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:35.05 +42:07:09.9: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065719947572151552,2461300.8736,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065719947572151552 20260917.3736 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.99 22:19:08.95 +44:59:11.4
96.64706 -9.97295 galactic Lac Second-epoch detections are separated by 0.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.7888+44.9889 | 22:19:08.95 +44:59:11.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.542+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:08.95 +44:59:11.4: 14.00 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:08.95 +44:59:11.4: 14.18 +/- 0.08 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
ATO J334.7888+44.9889,2461300.8736,12.99,0.05,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 J334.7888+44.9889 20260917.3736 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 17.3736 2461300.8736 12.34 20:55:43.66 +41:47:36.0
83.21062 -2.21076 galactic Cyg Second-epoch detections are separated by 1.7" 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 | 20:55:43.66 +41:47:36.0 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.056 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:43.66 +41:47:36.0: 14.00 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:43.66 +41:47:36.0: 13.88 +/- 0.07 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
target,2461300.8736,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.34 20:55:34.05 +41:56:30.8
83.30475 -2.09198 galactic Cyg Second-epoch detections are separated by 0.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065702454162840064 | 20:55:33.91 +41:56:30.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.056+/-0.029 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:34.05 +41:56:30.8: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:34.05 +41:56:30.8: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065702454162840064,2461300.8736,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065702454162840064 20260917.3736 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.73 20:57:18.20 +41:20:55.9
83.06310 -2.72329 galactic Cyg Second-epoch detections are separated by 2.5" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:18.20 +41:20:55.9 (user input) | T | P | (position from user input) J-Ks=0.488+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:18.20 +41:20:55.9: 13.97 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:18.20 +41:20:55.9: 14.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461300.8736,12.73,0.05,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 20260917.3736 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 17.3736 2461300.8736 13.01 22:02:14.46 +42:15:55.0
92.51011 -10.39700 galactic Lac Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Nazarov-2 | 22:02:16.79 +42:15:26.1 (Gaia DR3) | EW (local) | 0.342800000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.815+/-0.029 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:02:14.46 +42:15:55.0: 13.97 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:02:14.46 +42:15:55.0: 14.15 +/- 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
Nazarov-2,2461300.8736,13.01,0.05,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
Nazarov-2 20260917.3736 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 17.3736 2461300.8736 12.57 20:55:50.22 +41:55:20.1
83.32219 -2.14292 galactic Cyg Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:50.22 +41:55:20.1 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:50.22 +41:55:20.1: 13.99 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:50.22 +41:55:20.1: 13.86 +/- 0.07 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,2461300.8736,12.57,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.41 20:58:06.79 +41:57:19.2
83.62250 -2.44329 galactic Cyg Second-epoch detections are separated by 0.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5279+41.9552 | 20:58:06.72 +41:57:18.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.923+/-0.031 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:06.79 +41:57:19.2: 12.56 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:06.79 +41:57:19.2: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 J314.5279+41.9552,2461300.8736,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5279+41.9552 20260917.3736 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.02 22:17:33.54 +44:44:40.8
96.27253 -10.01563 galactic Lac Second-epoch detections are separated by 2.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.3960+44.7358 | 22:17:33.54 +44:44:40.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.847+/-0.027 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:33.54 +44:44:40.8: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:33.54 +44:44:40.8: 13.97 +/- 0.07 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 J334.3960+44.7358,2461300.8736,13.02,0.05,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 J334.3960+44.7358 20260917.3736 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 17.3736 2461300.8736 13.02 22:22:00.39 +49:00:11.1
99.29370 -6.88790 galactic Lac Second-epoch detections are separated by 1.5" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.5040+48.9923 | 22:22:00.39 +49:00:11.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.305+/-0.033 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:22:00.39 +49:00:11.1: 13.92 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:22:00.39 +49:00:11.1: 13.92 +/- 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 J335.5040+48.9923,2461300.8736,13.02,0.05,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 J335.5040+48.9923 20260917.3736 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 17.3736 2461300.8736 11.29 20:58:18.48 +41:49:25.8
83.54640 -2.55655 galactic Cyg Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5673+41.8234 | 20:58:18.42 +41:49:25.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.265+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:18.48 +41:49:25.8: 12.57 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:18.48 +41:49:25.8: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.5673+41.8234,2461300.8736,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.5673+41.8234 20260917.3736 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.09 22:17:23.38 +44:48:46.1
96.28621 -9.94239 galactic Lac Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:23.38 +44:48:46.1 (user input) | T | P | (position from user input) J-Ks=0.452+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:23.38 +44:48:46.1: 13.98 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:23.38 +44:48:46.1: 14.09 +/- 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,2461300.8736,13.09,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.45 20:55:36.08 +41:29:00.1
82.95864 -2.39310 galactic Cyg Second-epoch detections are separated by 0.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065675589149486592 | 20:55:36.08 +41:29:00.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:36.08 +41:29:00.1: 12.52 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:36.08 +41:29:00.1: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 2065675589149486592,2461300.8736,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065675589149486592 20260917.3736 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.45 20:56:39.36 +41:41:51.3
83.24983 -2.40471 galactic Cyg Second-epoch detections are separated by 1.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:39.36 +41:41:51.3 (user input) | T | P | (position from user input) J-Ks=1.203+/-0.025 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:39.36 +41:41:51.3: 13.95 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:39.36 +41:41:51.3: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.93 22:16:19.95 +45:03:03.1
96.26567 -9.64029 galactic Lac Second-epoch detections are separated by 0.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:19.95 +45:03:03.1 (user input) | T | P | (position from user input) J-Ks=0.547+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:19.95 +45:03:03.1: 13.93 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:19.95 +45:03:03.1: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.93,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.68 20:57:41.85 +41:57:59.0
83.58050 -2.37747 galactic Cyg Second-epoch detections are separated by 2.4" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.4280+41.9662 | 20:57:41.85 +41:57:59.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:41.85 +41:57:59.0: 13.91 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:41.85 +41:57:59.0: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 J314.4280+41.9662,2461300.8736,12.68,0.05,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
ATO J314.4280+41.9662 20260917.3736 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 17.3736 2461300.8736 13.07 22:16:10.06 +48:59:32.8
98.48429 -6.36746 galactic Lac Second-epoch detections are separated by 0.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:10.06 +48:59:32.8 (user input) | T | P | (position from user input) J-Ks=1.028+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:10.06 +48:59:32.8: 13.93 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:10.06 +48:59:32.8: 14.05 +/- 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
target,2461300.8736,13.07,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.22 20:56:23.77 +41:54:31.7
83.37934 -2.23089 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.0981+41.9085 | 20:56:23.55 +41:54:30.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:23.77 +41:54:31.7: 12.48 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:23.77 +41:54:31.7: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.0981+41.9085,2461300.8736,11.22,0.05,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
ATO J314.0981+41.9085 20260917.3736 11.22CV 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 17.3736 2461300.8736 12.74 22:17:16.10 +44:50:48.6
96.28760 -9.90216 galactic Lac Second-epoch detections are separated by 0.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:16.10 +44:50:48.6 (user input) | T | P | (position from user input) J-Ks=0.849+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:16.10 +44:50:48.6: 13.94 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:16.10 +44:50:48.6: 13.77 +/- 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
target,2461300.8736,12.74,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.05 20:55:52.55 +42:24:33.7
83.69849 -1.83324 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was found in VSX 8" NSVS J2055519+422431
Type: L:
# Max. Min./Amp. JD0 Period
10.565 R1 Y 0.267 R1 123.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:52.55 +42:24:33.7: 12.47 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:52.55 +42:24:33.7: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2055519+422431,2461300.8736,11.05,0.05,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
NSVS J2055519+422431 20260917.3736 11.05CV 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 17.3736 2461300.8736 11.51 20:58:55.59 +42:06:13.4
83.83371 -2.46077 galactic Cyg Second-epoch detections are separated by 0.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065670052929553536 | 20:58:55.65 +42:06:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.031 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:55.59 +42:06:13.4: 12.44 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:55.59 +42:06:13.4: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065670052929553536,2461300.8736,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065670052929553536 20260917.3736 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.56 20:55:24.79 +41:23:33.5
82.86652 -2.42478 galactic Cyg Second-epoch detections are separated by 4.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:24.79 +41:23:33.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:24.79 +41:23:33.5: 13.90 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:24.79 +41:23:33.5: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461300.8736,12.56,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.64 20:57:59.10 +42:00:04.5
83.64181 -2.39529 galactic Cyg Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:59.10 +42:00:04.5 (user input) | T | P | (position from user input) J-Ks=1.452+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:59.10 +42:00:04.5: 13.94 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:59.10 +42:00:04.5: 14.16 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.64,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.96 22:15:56.35 +44:48:17.6
96.06617 -9.80364 galactic Lac Second-epoch detections are separated by 0.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:15:56.35 +44:48:17.6 (user input) | T | P | (position from user input) J-Ks=0.874+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:56.35 +44:48:17.6: 13.95 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:56.35 +44:48:17.6: 13.90 +/- 0.07 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,2461300.8736,12.96,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.96 22:16:02.48 +49:08:31.7
98.55162 -6.23197 galactic Lac Second-epoch detections are separated by 1.1" and 4.7 pix
The object was found in VSX 1" Gaia DR3 1999883630848469504
Type: ROT
# Max. Min./Amp. JD0 Period
13.600 G 13.620 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:02.48 +49:08:31.7: 13.98 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:02.48 +49:08:31.7: 13.92 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1999883630848469504,2461300.8736,12.96,0.05,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 1999883630848469504 20260917.3736 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 17.3736 2461300.8736 12.69 20:58:40.23 +41:54:51.6
83.65913 -2.54858 galactic Cyg Second-epoch detections are separated by 1.8" and 4.9 pix
The object was found in VSX 9" ZTF J205839.81+415459.5
Type: EW
# Max. Min./Amp. JD0 Period
17.457 r Y 0.355 r 2458285.91900 0.692792600000
ATTENTION: measured mag 12.69 is 4.4 mag brighter than the VSX record maximum brightness 17.10 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:40.23 +41:54:51.6: 13.94 +/- 0.09 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:40.23 +41:54:51.6: 14.16 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205839.81+415459.5,2461300.8736,12.69,0.05,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
ZTF J205839.81+415459.5 20260917.3736 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 17.3736 2461300.8736 11.35 20:57:19.80 +42:02:12.1
83.58946 -2.27988 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065713449279114624 | 20:57:19.73 +42:02:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:19.80 +42:02:12.1: 12.41 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:19.80 +42:02:12.1: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065713449279114624,2461300.8736,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065713449279114624 20260917.3736 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 13.00 20:57:27.17 +41:51:06.5
83.46378 -2.41748 galactic Cyg Second-epoch detections are separated by 0.6" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3627+41.8516 | 20:57:27.17 +41:51:06.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.794+/-0.029 (Very red!)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:27.17 +41:51:06.5: 14.77 +/- 0.18 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:27.17 +41:51:06.5: 14.92 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J314.3627+41.8516,2461300.8736,13.00,0.05,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 J314.3627+41.8516 20260917.3736 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 17.3736 2461300.8736 11.45 20:55:35.04 +42:19:43.9
83.60218 -1.84420 galactic Cyg Second-epoch detections are separated by 0.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9013+42.3275 | 20:55:34.99 +42:19:43.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.355+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:35.04 +42:19:43.9: 12.37 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:35.04 +42:19:43.9: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.9013+42.3275,2461300.8736,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.9013+42.3275 20260917.3736 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.19 20:56:47.92 +41:35:44.9
83.18962 -2.49103 galactic Cyg Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.2122+41.5895 | 20:56:50.94 +41:35:22.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.026 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:47.92 +41:35:44.9: 12.36 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:47.92 +41:35:44.9: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.2122+41.5895,2461300.8736,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.2122+41.5895 20260917.3736 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.36 20:57:54.05 +42:00:31.7
83.63734 -2.37851 galactic Cyg Second-epoch detections are separated by 1.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065671530398306560 | 20:57:53.99 +42:00:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.401+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:54.05 +42:00:31.7: 12.35 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:54.05 +42:00:31.7: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065671530398306560,2461300.8736,11.36,0.05,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
Gaia DR3 2065671530398306560 20260917.3736 11.36CV 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 17.3736 2461300.8736 12.86 22:11:15.49 +50:23:25.0
98.62537 -4.76606 galactic Lac Second-epoch detections are separated by 1.0" and 4.3 pix
The object was found in VSX15" Gaia DR3 1976797494441609344
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.870 G 14.900 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:11:15.49 +50:23:25.0: 13.92 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:11:15.49 +50:23:25.0: 13.89 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 1976797494441609344,2461300.8736,12.86,0.05,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 1976797494441609344 20260917.3736 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 17.3736 2461300.8736 11.43 20:58:50.88 +42:06:26.9
83.82702 -2.44730 galactic Cyg Second-epoch detections are separated by 0.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065672977808766080 | 20:58:50.96 +42:06:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.289+/-0.038 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:50.88 +42:06:26.9: 12.33 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:50.88 +42:06:26.9: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065672977808766080,2461300.8736,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065672977808766080 20260917.3736 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.62 20:57:14.89 +41:40:24.7
83.30337 -2.50441 galactic Cyg Second-epoch detections are separated by 0.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3207+41.6775 | 20:57:14.89 +41:40:24.7 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.567+/-0.027 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:14.89 +41:40:24.7: 13.92 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:14.89 +41:40:24.7: 14.07 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.98 +/- 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 J314.3207+41.6775,2461300.8736,12.62,0.05,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 J314.3207+41.6775 20260917.3736 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 17.3736 2461300.8736 12.89 22:15:50.94 +45:01:14.9
96.17699 -9.61671 galactic Lac Second-epoch detections are separated by 2.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:15:50.94 +45:01:14.9 (user input) | T | P | (position from user input) J-Ks=0.945+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:50.94 +45:01:14.9: 13.90 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:50.94 +45:01:14.9: 13.88 +/- 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
target,2461300.8736,12.89,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.10 20:55:08.60 +41:43:07.0
83.08309 -2.17583 galactic Cyg Second-epoch detections are separated by 0.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.7861+41.7186 | 20:55:08.67 +41:43:07.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.272+/-0.026 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:08.60 +41:43:07.0: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:08.60 +41:43:07.0: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.7861+41.7186,2461300.8736,11.10,0.05,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 J313.7861+41.7186 20260917.3736 11.10CV 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 17.3736 2461300.8736 11.17 20:57:30.68 +41:49:39.4
83.45248 -2.44150 galactic Cyg Second-epoch detections are separated by 1.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065663013484571136 | 20:57:30.62 +41:49:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.967+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:30.68 +41:49:39.4: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:30.68 +41:49:39.4: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065663013484571136,2461300.8736,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065663013484571136 20260917.3736 11.17CV 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 17.3736 2461300.8736 12.94 22:14:28.69 +48:58:26.0
98.24344 -6.22649 galactic Lac Second-epoch detections are separated by 0.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.6111+48.9720 | 22:14:28.69 +48:58:26.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.096+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:14:28.69 +48:58:26.0: 13.85 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:14:28.69 +48:58:26.0: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.6111+48.9720,2461300.8736,12.94,0.05,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 J333.6111+48.9720 20260917.3736 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 17.3736 2461300.8736 11.35 20:54:41.77 +42:39:36.0
83.74953 -1.50546 galactic Cyg Second-epoch detections are separated by 0.5" and 4.7 pix
The object was found in VSX15" ZTF J205441.15+423922.4
Type: EW
# Max. Min./Amp. JD0 Period
18.472 r Y 0.311 r 2458361.79530 0.383201400000
ATTENTION: measured mag 11.35 is 6.8 mag brighter than the VSX record maximum brightness 18.16 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:54:41.77 +42:39:36.0: 12.26 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:54:41.77 +42:39:36.0: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205441.15+423922.4,2461300.8736,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205441.15+423922.4 20260917.3736 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 11.31 20:56:04.72 +42:27:40.4
83.76228 -1.82819 galactic Cyg Second-epoch detections are separated by 0.2" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065924937769600256 | 20:56:04.66 +42:27:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.309+/-0.028 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:04.72 +42:27:40.4: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:04.72 +42:27:40.4: 12.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065924937769600256,2461300.8736,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065924937769600256 20260917.3736 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.89 22:03:00.63 +42:05:24.9
92.51698 -10.62264 galactic Lac Second-epoch detections are separated by 0.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:00.63 +42:05:24.9 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.034 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:03:00.63 +42:05:24.9: 13.88 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:03:00.63 +42:05:24.9: 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,2461300.8736,12.89,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.22 20:56:48.88 +41:56:10.1
83.45070 -2.27241 galactic Cyg Second-epoch detections are separated by 1.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065714136473885312 | 20:56:48.85 +41:56:10.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.331+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:48.88 +41:56:10.1: 12.23 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:48.88 +41:56:10.1: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065714136473885312,2461300.8736,11.22,0.05,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 2065714136473885312 20260917.3736 11.22CV 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 17.3736 2461300.8736 12.61 20:58:42.53 +42:29:45.5
84.10441 -2.17385 galactic Cyg Second-epoch detections are separated by 2.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:42.53 +42:29:45.5 (user input) | T | P | (position from user input) J-Ks=0.510+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:42.53 +42:29:45.5: 13.90 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:42.53 +42:29:45.5: 13.92 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.61,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.65 20:58:49.44 +42:27:20.7
84.08784 -2.21622 galactic Cyg Second-epoch detections are separated by 3.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:49.44 +42:27:20.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:49.44 +42:27:20.7: 13.58 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:49.44 +42:27:20.7: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461300.8736,12.65,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.56 20:58:09.01 +41:47:11.2
83.49883 -2.55864 galactic Cyg Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:09.01 +41:47:11.2 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:09.01 +41:47:11.2: 13.86 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:09.01 +41:47:11.2: 13.83 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.56,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.12 20:56:55.74 +41:48:40.8
83.36952 -2.36963 galactic Cyg Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.2324+41.8113 | 20:56:55.78 +41:48:41.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.275+/-0.030 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:55.74 +41:48:40.8: 12.21 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:55.74 +41:48:40.8: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.2324+41.8113,2461300.8736,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.2324+41.8113 20260917.3736 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.78 22:15:30.89 +48:53:41.0
98.33980 -6.38798 galactic Lac Second-epoch detections are separated by 0.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J333.8772+48.8933 | 22:15:27.42 +48:53:58.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:30.89 +48:53:41.0: 13.85 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:30.89 +48:53:41.0: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J333.8772+48.8933,2461300.8736,12.78,0.05,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 J333.8772+48.8933 20260917.3736 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 17.3736 2461300.8736 11.31 21:00:31.81 +42:23:51.2
84.25054 -2.49206 galactic Cyg Second-epoch detections are separated by 0.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.1279+42.3937 | 21:00:31.68 +42:23:50.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.709+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:31.81 +42:23:51.2: 12.20 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:31.81 +42:23:51.2: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.1279+42.3937,2461300.8736,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J315.1279+42.3937 20260917.3736 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.73 20:55:08.17 +41:29:45.3
82.91195 -2.31848 galactic Cyg Second-epoch detections are separated by 1.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:08.17 +41:29:45.3 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.034 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:08.17 +41:29:45.3: 13.86 +/- 0.08 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:08.17 +41:29:45.3: 14.03 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461300.8736,12.73,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.81 22:20:07.45 +49:05:58.0
99.08671 -6.63859 galactic Lac Second-epoch detections are separated by 1.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.0181+49.0912 | 22:20:07.45 +49:05:58.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.676+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:20:07.45 +49:05:58.0: 13.85 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:20:07.45 +49:05:58.0: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.0181+49.0912,2461300.8736,12.81,0.05,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 J335.0181+49.0912 20260917.3736 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 17.3736 2461300.8736 12.72 20:59:57.93 +41:43:57.0
83.67968 -2.84999 galactic Cyg Second-epoch detections are separated by 1.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9898+41.7329 | 20:59:57.93 +41:43:57.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:57.93 +41:43:57.0: 13.87 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:57.93 +41:43:57.0: 13.81 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.9898+41.7329,2461300.8736,12.72,0.05,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
ATO J314.9898+41.7329 20260917.3736 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 17.3736 2461300.8736 11.24 20:59:20.43 +41:48:03.8
83.65503 -2.71704 galactic Cyg Second-epoch detections are separated by 2.9" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065650261720265472 | 20:59:19.32 +41:47:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:20.43 +41:48:03.8: 12.14 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:20.43 +41:48:03.8: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065650261720265472,2461300.8736,11.24,0.05,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 2065650261720265472 20260917.3736 11.24CV 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 17.3736 2461300.8736 12.96 22:05:10.90 +42:03:02.0
92.81936 -10.89773 galactic Lac Second-epoch detections are separated by 1.1" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:10.90 +42:03:02.0 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:05:10.90 +42:03:02.0: 13.84 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:05:10.90 +42:03:02.0: 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,2461300.8736,12.96,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.85 22:17:26.71 +44:51:59.7
96.32518 -9.90346 galactic Lac Second-epoch detections are separated by 1.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:26.71 +44:51:59.7 (user input) | T | P | (position from user input) J-Ks=0.903+/-0.027 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:26.71 +44:51:59.7: 13.87 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:26.71 +44:51:59.7: 13.82 +/- 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
target,2461300.8736,12.85,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.77 21:02:22.17 +41:02:48.4
83.46042 -3.64093 galactic Cyg Second-epoch detections are separated by 1.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.5885+41.0461 | 21:02:22.17 +41:02:48.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.389+/-0.038 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:02:22.17 +41:02:48.4: 13.83 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:02:22.17 +41:02:48.4: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.5885+41.0461,2461300.8736,12.77,0.05,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
ATO J315.5885+41.0461 20260917.3736 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 17.3736 2461300.8736 12.89 22:02:10.73 +42:15:16.6
92.49423 -10.39846 galactic Lac Second-epoch detections are separated by 1.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:02:10.73 +42:15:16.6 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.040 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:02:10.73 +42:15:16.6: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:02:10.73 +42:15:16.6: 13.91 +/- 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,2461300.8736,12.89,0.05,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 20260917.3736 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 17.3736 2461300.8736 11.13 20:56:31.29 +42:22:22.9
83.74808 -1.94759 galactic Cyg Second-epoch detections are separated by 0.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065735748752693376 | 20:56:31.30 +42:22:23.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:31.29 +42:22:22.9: 12.08 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:31.29 +42:22:22.9: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065735748752693376,2461300.8736,11.13,0.05,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 2065735748752693376 20260917.3736 11.13CV 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 17.3736 2461300.8736 12.33 20:56:29.07 +41:34:44.9
83.13878 -2.45712 galactic Cyg Second-epoch detections are separated by 2.5" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.1222+41.5806 | 20:56:29.07 +41:34:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:29.07 +41:34:44.9: 13.82 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:29.07 +41:34:44.9: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.1222+41.5806,2461300.8736,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.1222+41.5806 20260917.3736 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.90 22:17:58.52 +45:06:01.8
96.53720 -9.76253 galactic Lac Second-epoch detections are separated by 1.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:58.52 +45:06:01.8 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:58.52 +45:06:01.8: 13.81 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:58.52 +45:06:01.8: 13.75 +/- 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,2461300.8736,12.90,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.59 20:58:14.62 +42:01:00.4
83.68495 -2.42160 galactic Cyg Second-epoch detections are separated by 2.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:14.62 +42:01:00.4 (user input) | T | P | (position from user input) J-Ks=0.651+/-0.038 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:14.62 +42:01:00.4: 13.85 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:14.62 +42:01:00.4: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.59,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.86 22:04:21.21 +41:57:52.9
92.64165 -10.87357 galactic Lac Second-epoch detections are separated by 0.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:21.21 +41:57:52.9 (user input) | T | P | (position from user input) J-Ks=0.533+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:21.21 +41:57:52.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:21.21 +41:57:52.9: 13.78 +/- 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,2461300.8736,12.86,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.98 22:18:12.34 +44:15:00.6
96.08724 -10.48954 galactic Lac Second-epoch detections are separated by 1.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:18:12.34 +44:15:00.6 (user input) | T | P | (position from user input) J-Ks=0.514+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:18:12.34 +44:15:00.6: 13.85 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:18:12.34 +44:15:00.6: 13.92 +/- 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,2461300.8736,12.98,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.89 22:16:05.80 +45:02:12.7
96.22279 -9.62826 galactic Lac Second-epoch detections are separated by 0.6" and 4.8 pix
The object was found in VSX 8" ZTF J221605.48+450219.6
Type: BY
# Max. Min./Amp. JD0 Period
15.296 r Y 0.100 r 2458436.62040 0.804127300000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:05.80 +45:02:12.7: 13.83 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:05.80 +45:02:12.7: 13.91 +/- 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
ZTF J221605.48+450219.6,2461300.8736,12.89,0.05,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
ZTF J221605.48+450219.6 20260917.3736 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 17.3736 2461300.8736 12.76 22:17:55.41 +44:59:01.8
96.46313 -9.85400 galactic Lac Second-epoch detections are separated by 0.7" and 4.7 pix
The object was found in VSX 1" Gaia DR3 1962208933634592000
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.590 G 13.630 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:55.41 +44:59:01.8: 13.80 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:55.41 +44:59:01.8: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1962208933634592000,2461300.8736,12.76,0.05,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
Gaia DR3 1962208933634592000 20260917.3736 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 17.3736 2461300.8736 12.61 20:55:42.76 +42:10:08.9
83.49567 -1.96563 galactic Cyg Second-epoch detections are separated by 1.4" and 4.7 pix
The object was found in VSX 2" Gaia DR3 2065709433491933056
Type: YSO
# Max. Min./Amp. JD0 Period
13.200 G 13.220 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:42.76 +42:10:08.9: 13.81 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:42.76 +42:10:08.9: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065709433491933056,2461300.8736,12.61,0.05,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 2065709433491933056 20260917.3736 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 17.3736 2461300.8736 12.39 20:57:14.97 +41:18:18.2
83.02319 -2.74407 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.3120+41.3050 | 20:57:14.97 +41:18:18.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.458+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:14.97 +41:18:18.2: 13.79 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:14.97 +41:18:18.2: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 J314.3120+41.3050,2461300.8736,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.3120+41.3050 20260917.3736 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 17.3736 2461300.8736 12.79 22:16:21.27 +44:53:24.2
96.17668 -9.77512 galactic Lac Second-epoch detections are separated by 1.1" and 4.7 pix
The object was found in VSX 2" Gaia DR3 1962204741746125184
Type: ROT
# Max. Min./Amp. JD0 Period
13.470 G 13.500 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:21.27 +44:53:24.2: 13.79 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:21.27 +44:53:24.2: 13.77 +/- 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
Gaia DR3 1962204741746125184,2461300.8736,12.79,0.05,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 1962204741746125184 20260917.3736 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 17.3736 2461300.8736 12.62 20:56:07.02 +41:36:52.7
83.12130 -2.38178 galactic Cyg Second-epoch detections are separated by 1.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:07.02 +41:36:52.7 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.037 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:07.02 +41:36:52.7: 13.77 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:07.02 +41:36:52.7: 13.97 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.62,0.05,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
target 20260917.3736 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 17.3736 2461300.8736 10.97 20:56:31.82 +42:27:20.9
83.81217 -1.89514 galactic Cyg Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2065929713773214592 | 20:56:31.77 +42:27:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:31.82 +42:27:20.9: 11.92 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:31.82 +42:27:20.9: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2065929713773214592,2461300.8736,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2065929713773214592 20260917.3736 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.81 22:03:22.76 +42:04:04.9
92.55862 -10.68183 galactic Lac Second-epoch detections are separated by 1.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:03:22.76 +42:04:04.9 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:03:22.76 +42:04:04.9: 13.77 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:03:22.76 +42:04:04.9: 13.75 +/- 0.05 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,2461300.8736,12.81,0.05,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 20260917.3736 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BL Lac,2461300.8736,12.79,0.05,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
BL Lac 20260917.3736 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 17.3736 2461300.8736 12.37 20:55:18.80 +41:21:47.9
82.83200 -2.42942 galactic Cyg Second-epoch detections are separated by 4.4" 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 | 20:55:18.80 +41:21:47.9 (user input) | T | P | (position from user input) J-Ks=0.700+/-0.036 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:18.80 +41:21:47.9: 13.75 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:18.80 +41:21:47.9: 13.89 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461300.8736,12.37,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.80 22:17:04.89 +44:29:51.5
96.05992 -10.17193 galactic Lac Second-epoch detections are separated by 0.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:04.89 +44:29:51.5 (user input) | T | P | (position from user input) J-Ks=0.854+/-0.027 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:04.89 +44:29:51.5: 13.79 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:04.89 +44:29:51.5: 13.80 +/- 0.05 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,2461300.8736,12.80,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.82 22:02:39.55 +42:13:38.8
92.54915 -10.47411 galactic Lac Second-epoch detections are separated by 0.3" and 4.8 pix
The object was found in VSX 1" Gaia DR3 1960065538793802368
Type: ROT
# Max. Min./Amp. JD0 Period
13.460 G 13.500 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:02:39.55 +42:13:38.8: 13.77 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:02:39.55 +42:13:38.8: 13.71 +/- 0.05 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
Gaia DR3 1960065538793802368,2461300.8736,12.82,0.05,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 1960065538793802368 20260917.3736 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 17.3736 2461300.8736 12.82 22:15:49.53 +44:55:51.3
96.12183 -9.68840 galactic Lac Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:15:49.53 +44:55:51.3 (user input) | T | P | (position from user input) J-Ks=0.555+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:49.53 +44:55:51.3: 13.76 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:49.53 +44:55:51.3: 13.89 +/- 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,2461300.8736,12.82,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.60 22:19:04.35 +44:57:51.0
96.62299 -9.98393 galactic Lac Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:19:04.35 +44:57:51.0 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:04.35 +44:57:51.0: 13.60 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:04.35 +44:57:51.0: 13.57 +/- 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
target,2461300.8736,12.60,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.53 20:55:45.50 +41:25:46.6
82.93662 -2.45029 galactic Cyg Second-epoch detections are separated by 0.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:45.50 +41:25:46.6 (user input) | T | P | (position from user input) J-Ks=1.076+/-0.033 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:45.50 +41:25:46.6: 13.77 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:45.50 +41:25:46.6: 13.89 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.82 +/- 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,2461300.8736,12.53,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.72 22:15:51.63 +44:56:13.3
96.13052 -9.68688 galactic Lac Second-epoch detections are separated by 1.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:15:51.63 +44:56:13.3 (user input) | T | P | (position from user input) J-Ks=0.648+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:51.63 +44:56:13.3: 13.75 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:51.63 +44:56:13.3: 13.72 +/- 0.05 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,2461300.8736,12.72,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.81 22:17:15.59 +44:14:54.1
95.94380 -10.39576 galactic Lac Second-epoch detections are separated by 1.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:15.59 +44:14:54.1 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:15.59 +44:14:54.1: 13.75 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:15.59 +44:14:54.1: 13.70 +/- 0.05 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,2461300.8736,12.81,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.62 20:58:38.12 +42:05:08.8
83.78477 -2.43162 galactic Cyg Second-epoch detections are separated by 3.4" and 5.2 pix
The object was found in VSX15" ZTF J205838.40+420522.9
Type: EW
# Max. Min./Amp. JD0 Period
19.539 r Y 0.654 r 2458257.96970 0.309638400000
ATTENTION: measured mag 12.62 is 6.3 mag brighter than the VSX record maximum brightness 18.89 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:38.12 +42:05:08.8: 13.76 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:38.12 +42:05:08.8: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 J205838.40+420522.9,2461300.8736,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205838.40+420522.9 20260917.3736 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 17.3736 2461300.8736 12.48 20:58:52.88 +41:42:54.9
83.53398 -2.70842 galactic Cyg Second-epoch detections are separated by 1.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.7208+41.7150 | 20:58:52.88 +41:42:54.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=11.917+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:52.88 +41:42:54.9: 13.78 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:52.88 +41:42:54.9: 13.70 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 J314.7208+41.7150,2461300.8736,12.48,0.05,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 J314.7208+41.7150 20260917.3736 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 17.3736 2461300.8736 12.54 20:55:30.14 +41:46:55.3
83.17482 -2.18602 galactic Cyg Second-epoch detections are separated by 1.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.8809+41.7813 | 20:55:30.14 +41:46:55.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.477+/-0.031 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:30.14 +41:46:55.3: 13.76 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:30.14 +41:46:55.3: 13.82 +/- 0.07 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
ATO J313.8809+41.7813,2461300.8736,12.54,0.05,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 J313.8809+41.7813 20260917.3736 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 17.3736 2461300.8736 12.72 22:04:41.67 +41:58:08.1
92.69572 -10.90844 galactic Lac Second-epoch detections are separated by 0.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:04:41.67 +41:58:08.1 (user input) | T | P | (position from user input) J-Ks=0.609+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:04:41.67 +41:58:08.1: 13.78 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:04:41.67 +41:58:08.1: 13.64 +/- 0.05 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,2461300.8736,12.72,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.70 22:15:51.51 +44:54:15.5
96.11140 -9.71363 galactic Lac Second-epoch detections are separated by 1.3" 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 | 22:15:51.51 +44:54:15.5 (user input) | T | P | (position from user input) J-Ks=0.309+/-0.042 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:51.51 +44:54:15.5: 13.73 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:51.51 +44:54:15.5: 13.67 +/- 0.05 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,2461300.8736,12.70,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.77 22:16:24.96 +45:01:12.4
96.26038 -9.67399 galactic Lac Second-epoch detections are separated by 0.1" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:24.96 +45:01:12.4 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:24.96 +45:01:12.4: 13.75 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:24.96 +45:01:12.4: 13.72 +/- 0.05 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,2461300.8736,12.77,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.88 22:16:30.09 +49:13:41.6
98.66281 -6.20287 galactic Lac Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.1320+49.2362 | 22:16:30.09 +49:13:41.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.812+/-0.032 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:30.09 +49:13:41.6: 13.73 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:30.09 +49:13:41.6: 13.79 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J334.1320+49.2362,2461300.8736,12.88,0.05,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 J334.1320+49.2362 20260917.3736 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 17.3736 2461300.8736 12.82 22:05:17.26 +42:00:40.3
92.81128 -10.94102 galactic Lac Second-epoch detections are separated by 0.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:05:17.26 +42:00:40.3 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:05:17.26 +42:00:40.3: 13.72 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:05:17.26 +42:00:40.3: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.82,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.52 20:55:50.51 +41:25:45.2
82.94645 -2.46248 galactic Cyg Second-epoch detections are separated by 3.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9626+41.4395 | 20:55:50.51 +41:25:45.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.431+/-0.036 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:50.51 +41:25:45.2: 13.75 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:50.51 +41:25:45.2: 13.81 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 J313.9626+41.4395,2461300.8736,12.52,0.05,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
ATO J313.9626+41.4395 20260917.3736 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 17.3736 2461300.8736 12.48 20:56:12.50 +42:07:04.6
83.51613 -2.06880 galactic Cyg Second-epoch detections are separated by 0.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.0522+42.1178 | 20:56:12.50 +42:07:04.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.392+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:12.50 +42:07:04.6: 13.70 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:12.50 +42:07:04.6: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.0522+42.1178,2461300.8736,12.48,0.05,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 J314.0522+42.1178 20260917.3736 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 17.3736 2461300.8736 12.39 20:57:33.93 +41:56:54.1
83.55081 -2.37058 galactic Cyg Second-epoch detections are separated by 1.6" 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 | 20:57:33.93 +41:56:54.1 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:33.93 +41:56:54.1: 13.69 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:33.93 +41:56:54.1: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8736,12.39,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.66 21:00:28.20 +41:55:55.9
83.89224 -2.78969 galactic Cyg Second-epoch detections are separated by 1.2" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:28.20 +41:55:55.9 (user input) | T | P | (position from user input) J-Ks=1.125+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:28.20 +41:55:55.9: 13.77 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:28.20 +41:55:55.9: 13.81 +/- 0.07 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
target,2461300.8736,12.66,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.71 22:14:52.03 +45:01:26.9
96.03413 -9.51538 galactic Lac Second-epoch detections are separated by 1.3" 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 | 22:14:52.03 +45:01:26.9 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:14:52.03 +45:01:26.9: 13.70 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:14:52.03 +45:01:26.9: 13.65 +/- 0.05 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,2461300.8736,12.71,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.81 22:22:45.89 +49:07:56.0
99.46938 -6.84685 galactic Lac Second-epoch detections are separated by 2.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.6741+49.1309 | 22:22:45.89 +49:07:56.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:22:45.89 +49:07:56.0: 13.72 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:22:45.89 +49:07:56.0: 13.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 J335.6741+49.1309,2461300.8736,12.81,0.05,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 J335.6741+49.1309 20260917.3736 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 17.3736 2461300.8736 13.00 20:58:34.48 +41:47:17.0
83.55174 -2.61755 galactic Cyg Second-epoch detections are separated by 4.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6352+41.7956 | 20:58:34.48 +41:47:17.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.455+/-0.082 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:34.48 +41:47:17.0: 14.64 +/- 0.16 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:34.48 +41:47:17.0: 14.46 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J314.6352+41.7956,2461300.8736,13.00,0.05,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 J314.6352+41.7956 20260917.3736 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 17.3736 2461300.8736 12.68 22:03:16.20 +42:03:28.4
92.53594 -10.67758 galactic Lac Second-epoch detections are separated by 1.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.8211+42.0555 | 22:03:16.20 +42:03:28.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.779+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:03:16.20 +42:03:28.4: 13.69 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:03:16.20 +42:03:28.4: 13.63 +/- 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
ATO J330.8211+42.0555,2461300.8736,12.68,0.05,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
ATO J330.8211+42.0555 20260917.3736 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 17.3736 2461300.8736 12.59 22:17:39.58 +45:05:15.5
96.48309 -9.74192 galactic Lac Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1962213396099160064 | 22:17:37.60 +45:05:36.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:39.58 +45:05:15.5: 13.65 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:39.58 +45:05:15.5: 13.60 +/- 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
Gaia DR3 1962213396099160064,2461300.8736,12.59,0.05,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
Gaia DR3 1962213396099160064 20260917.3736 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 17.3736 2461300.8736 12.62 22:16:54.53 +45:04:04.1
96.36059 -9.68375 galactic Lac Second-epoch detections are separated by 0.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:16:54.53 +45:04:04.1 (user input) | T | P | (position from user input) J-Ks=0.819+/-0.026 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:54.53 +45:04:04.1: 13.70 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:54.53 +45:04:04.1: 13.66 +/- 0.05 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,2461300.8736,12.62,0.05,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
target 20260917.3736 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 17.3736 2461300.8736 12.59 20:59:32.64 +41:49:20.6
83.69604 -2.73172 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:59:32.64 +41:49:20.6 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:32.64 +41:49:20.6: 13.68 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:32.64 +41:49:20.6: 13.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.59,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.66 20:59:00.06 +42:17:21.6
83.98326 -2.34980 galactic Cyg Second-epoch detections are separated by 2.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.7493+42.2892 | 20:59:00.06 +42:17:21.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.662+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:00.06 +42:17:21.6: 13.70 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:00.06 +42:17:21.6: 13.90 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 J314.7493+42.2892,2461300.8736,12.66,0.05,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 J314.7493+42.2892 20260917.3736 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 17.3736 2461300.8736 12.48 20:57:31.72 +41:59:11.6
83.57538 -2.34052 galactic Cyg Second-epoch detections are separated by 0.8" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:31.72 +41:59:11.6 (user input) | T | P | (position from user input) J-Ks=1.156+/-0.033 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:31.72 +41:59:11.6: 13.68 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:31.72 +41:59:11.6: 13.70 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461300.8736,12.48,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.63 22:15:50.18 +44:59:33.3
96.15889 -9.63869 galactic Lac Second-epoch detections are separated by 1.3" 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 | Gaia DR3 1962218520001182720 | 22:15:50.83 +45:00:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.212+/-0.035 (F)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:15:50.18 +44:59:33.3: 13.65 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:15:50.18 +44:59:33.3: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 1962218520001182720,2461300.8736,12.63,0.05,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 1962218520001182720 20260917.3736 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 17.3736 2461300.8736 12.29 20:55:08.26 +41:50:37.6
83.17810 -2.09426 galactic Cyg Second-epoch detections are separated by 1.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:08.26 +41:50:37.6 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:08.26 +41:50:37.6: 13.65 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:08.26 +41:50:37.6: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.74 22:17:23.94 +44:50:07.2
96.30047 -9.92470 galactic Lac Second-epoch detections are separated by 0.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:17:23.94 +44:50:07.2 (user input) | T | P | (position from user input) J-Ks=0.848+/-0.028 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:17:23.94 +44:50:07.2: 13.66 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:17:23.94 +44:50:07.2: 13.69 +/- 0.05 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,2461300.8736,12.74,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.63 21:02:52.05 +41:58:13.3
84.21562 -3.09931 galactic Cyg Second-epoch detections are separated by 1.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J315.7252+41.9752 | 21:02:52.05 +41:58:13.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.382+/-0.032 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:02:52.05 +41:58:13.3: 13.65 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:02:52.05 +41:58:13.3: 13.69 +/- 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
ATO J315.7252+41.9752,2461300.8736,12.63,0.05,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
ATO J315.7252+41.9752 20260917.3736 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 17.3736 2461300.8736 12.40 20:55:11.46 +41:51:15.8
83.19263 -2.09500 galactic Cyg Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:11.46 +41:51:15.8 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:11.46 +41:51:15.8: 13.64 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:11.46 +41:51:15.8: 13.93 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.48 20:58:33.80 +42:24:01.0
84.01436 -2.21607 galactic Cyg Second-epoch detections are separated by 0.8" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:33.80 +42:24:01.0 (user input) | T | P | (position from user input) J-Ks=0.496+/-0.034 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:33.80 +42:24:01.0: 13.66 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:33.80 +42:24:01.0: 13.63 +/- 0.05 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,2461300.8736,12.48,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.37 20:58:03.26 +41:47:34.5
83.49209 -2.54088 galactic Cyg Second-epoch detections are separated by 1.1" and 4.9 pix
The object was found in VSX 1" ASASSN-V J205803.18+414734.2
Type: L
# Max. Min./Amp. JD0 Period
14.360 V 14.460 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:03.26 +41:47:34.5: 13.65 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:03.26 +41:47:34.5: 13.76 +/- 0.06 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
ASASSN-V J205803.18+414734.2,2461300.8736,12.37,0.05,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
ASASSN-V J205803.18+414734.2 20260917.3736 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 17.3736 2461300.8736 12.71 22:20:05.22 +48:57:52.8
99.00700 -6.74784 galactic Lac Second-epoch detections are separated by 2.5" and 4.8 pix
The object was found in VSX17" Gaia DR3 1999654279592618240
Type: ROT
# Max. Min./Amp. JD0 Period
14.960 G 15.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:20:05.22 +48:57:52.8: 13.66 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:20:05.22 +48:57:52.8: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 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 1999654279592618240,2461300.8736,12.71,0.05,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 1999654279592618240 20260917.3736 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 17.3736 2461300.8736 12.71 22:16:47.66 +45:02:24.0
96.32774 -9.69532 galactic Lac Second-epoch detections are separated by 0.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.1989+45.0402 | 22:16:47.66 +45:02:24.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.744+/-0.028 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:16:47.66 +45:02:24.0: 13.65 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:16:47.66 +45:02:24.0: 13.72 +/- 0.05 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
ATO J334.1989+45.0402,2461300.8736,12.71,0.05,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 J334.1989+45.0402 20260917.3736 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 17.3736 2461300.8736 12.28 20:58:30.43 +42:28:43.7
84.06709 -2.15693 galactic Cyg Second-epoch detections are separated by 1.4" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6261+42.4786 | 20:58:30.25 +42:28:43.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.953+/-0.031 (Very red!)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:30.43 +42:28:43.7: 13.67 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:30.43 +42:28:43.7: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.6261+42.4786,2461300.8736,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.6261+42.4786 20260917.3736 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 17.3736 2461300.8736 12.32 20:59:28.53 +42:08:26.4
83.92836 -2.51354 galactic Cyg Second-epoch detections are separated by 0.7" and 4.6 pix
The object was found in VSX 2" ASASSN-V J205928.38+420826.2
Type: SR
# Max. Min./Amp. JD0 Period
15.680 g Y 0.250 g 2459307.07700 123.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:28.53 +42:08:26.4: 13.64 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:28.53 +42:08:26.4: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 J205928.38+420826.2,2461300.8736,12.32,0.05,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
ASASSN-V J205928.38+420826.2 20260917.3736 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 17.3736 2461300.8736 12.36 20:56:57.84 +41:50:56.1
83.40236 -2.35018 galactic Cyg Second-epoch detections are separated by 2.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:56:57.84 +41:50:56.1 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.030 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:57.84 +41:50:56.1: 13.64 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:57.84 +41:50:56.1: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 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,2461300.8736,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.78 22:20:46.67 +48:54:36.8
99.07243 -6.85561 galactic Lac Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J335.1949+48.9104 | 22:20:46.67 +48:54:36.8 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.168+/-0.024 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:20:46.67 +48:54:36.8: 13.62 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:20:46.67 +48:54:36.8: 13.70 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J335.1949+48.9104,2461300.8736,12.78,0.05,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 J335.1949+48.9104 20260917.3736 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 17.3736 2461300.8736 12.51 22:19:33.02 +44:58:22.4
96.69921 -10.02374 galactic Lac Second-epoch detections are separated by 1.7" 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 | 22:19:33.02 +44:58:22.4 (user input) | T | P | (position from user input) J-Ks=0.775+/-0.029 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:19:33.02 +44:58:22.4: 13.59 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:19:33.02 +44:58:22.4: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.62 20:59:20.44 +41:55:44.3
83.75183 -2.63330 galactic Cyg Second-epoch detections are separated by 1.9" and 4.7 pix
The object was found in VSX 1" V1717 Cyg
Type: UV
# Max. Min./Amp. JD0 Period
16.500 U 18.100 U
ATTENTION: measured mag 12.62 is 3.9 mag brighter than the VSX record maximum brightness 16.50 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:20.44 +41:55:44.3: 13.60 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:20.44 +41:55:44.3: 13.63 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.61 +/- 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
V1717 Cyg,2461300.8736,12.62,0.05,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
V1717 Cyg 20260917.3736 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 17.3736 2461300.8736 12.51 21:03:56.38 +41:06:07.5
83.69853 -3.82578 galactic Cyg Second-epoch detections are separated by 2.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:03:56.38 +41:06:07.5 (user input) | T | P | (position from user input) J-Ks=1.163+/-0.030 (M)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:03:56.38 +41:06:07.5: 13.61 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:03:56.38 +41:06:07.5: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8736,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.46 20:55:10.53 +42:17:24.8
83.52386 -1.81150 galactic Cyg Second-epoch detections are separated by 2.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:55:10.53 +42:17:24.8 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.033 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:10.53 +42:17:24.8: 13.59 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:10.53 +42:17:24.8: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461300.8736,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3736 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 17.3736 2461300.8736 12.57 20:57:45.60 +42:29:05.7
83.98180 -2.04853 galactic Cyg Second-epoch detections are separated by 1.4" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:57:45.60 +42:29:05.7 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.035 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:45.60 +42:29:05.7: 13.60 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:45.60 +42:29:05.7: 13.65 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461300.8736,12.57,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.38 20:58:29.24 +41:37:09.4
83.41311 -2.71540 galactic Cyg Second-epoch detections are separated by 2.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.6333+41.6164 | 20:58:29.24 +41:37:09.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.401+/-0.028 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:29.24 +41:37:09.4: 13.59 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:29.24 +41:37:09.4: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.6333+41.6164,2461300.8736,12.38,0.05,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 J314.6333+41.6164 20260917.3736 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 17.3736 2461300.8736 12.12 20:55:23.39 +41:48:56.1
83.18690 -2.14834 galactic Cyg Second-epoch detections are separated by 1.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.8474+41.8150 | 20:55:23.39 +41:48:56.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.483+/-0.030 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:23.39 +41:48:56.1: 13.60 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:23.39 +41:48:56.1: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 J313.8474+41.8150,2461300.8736,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.8474+41.8150 20260917.3736 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3736 2461300.8736 12.45 20:58:09.17 +42:30:29.3
84.04666 -2.08830 galactic Cyg Second-epoch detections are separated by 2.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.5504+42.5169 | 20:58:09.17 +42:30:29.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.487+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:09.17 +42:30:29.3: 13.58 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:09.17 +42:30:29.3: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 J314.5504+42.5169,2461300.8736,12.45,0.05,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 J314.5504+42.5169 20260917.3736 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 17.3736 2461300.8736 12.48 20:58:59.60 +41:49:02.6
83.62501 -2.65743 galactic Cyg Second-epoch detections are separated by 1.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:58:59.60 +41:49:02.6 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.029 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:59.60 +41:49:02.6: 13.54 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:59.60 +41:49:02.6: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461300.8736,12.48,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.65 22:18:34.42 +45:02:50.2
96.59582 -9.86576 galactic Lac Second-epoch detections are separated by 1.2" and 4.7 pix
The object was found in VSX10" Gaia DR3 1962115505207706112
Type: ROT
# Max. Min./Amp. JD0 Period
16.120 G 16.180 G K
ATTENTION: measured mag 12.65 is 3.5 mag brighter than the VSX record maximum brightness 16.12 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:18:34.42 +45:02:50.2: 13.57 +/- 0.04 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:18:34.42 +45:02:50.2: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1962115505207706112,2461300.8736,12.65,0.05,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
Gaia DR3 1962115505207706112 20260917.3736 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 17.3736 2461300.8736 12.61 21:00:17.17 +42:26:32.0
84.25459 -2.42877 galactic Cyg Second-epoch detections are separated by 4.5" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:00:17.17 +42:26:32.0 (user input) | T | P | (position from user input) J-Ks=0.572+/-0.033 (K)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:00:17.17 +42:26:32.0: 13.56 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:00:17.17 +42:26:32.0: 13.56 +/- 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,2461300.8736,12.61,0.05,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 20260917.3736 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 17.3736 2461300.8736 12.60 20:59:38.56 +41:54:57.8
83.77891 -2.68420 galactic Cyg Second-epoch detections are separated by 1.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.9109+41.9157 | 20:59:38.56 +41:54:57.8 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.398+/-0.026 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:59:38.56 +41:54:57.8: 13.59 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:59:38.56 +41:54:57.8: 13.60 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 J314.9109+41.9157,2461300.8736,12.60,0.05,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 J314.9109+41.9157 20260917.3736 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 17.3736 2461300.8736 12.65 21:08:02.59 +41:33:52.5
84.55987 -4.08822 galactic Cyg Second-epoch detections are separated by 1.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.0034+41.5597 | 21:08:02.74 +41:33:08.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 21:08:02.59 +41:33:52.5: 13.57 +/- 0.05 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 21:08:02.59 +41:33:52.5: 13.55 +/- 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 J317.0034+41.5597,2461300.8736,12.65,0.05,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
ATO J317.0034+41.5597 20260917.3736 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 17.3736 2461300.8736 12.22 20:55:54.55 +41:46:31.5
83.21884 -2.24815 galactic Cyg Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J313.9779+41.7752 | 20:55:54.55 +41:46:31.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.376+/-0.031 (G)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:54.55 +41:46:31.5: 13.57 +/- 0.06 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:54.55 +41:46:31.5: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 J313.9779+41.7752,2461300.8736,12.22,0.05,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
ATO J313.9779+41.7752 20260917.3736 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 17.3736 2461300.8736 12.68 22:22:35.19 +49:53:48.0
99.86150 -6.18849 galactic Lac Second-epoch detections are separated by 1.6" and 4.6 pix
The object was found in VSX 1" Gaia DR3 1999838791389857024
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.360 G 13.400 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 22:22:35.19 +49:53:48.0: 13.58 +/- 0.07 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 22:22:35.19 +49:53:48.0: 13.60 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 1999838791389857024,2461300.8736,12.68,0.05,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 1999838791389857024 20260917.3736 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461245.82532353 24.07.2026 07:48:17.953 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
First image: 2461245.82532353 24.07.2026 07:48:17.953 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Last image: 2461300.87383428 17.09.2026 08:58:09.282 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 99
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
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): 32364
Objects passed selection criteria: 32160
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 20268.5
Average stars matched: 19569.2 (96.5501 %)
Memory usage VmPeak: 256036 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: 2461245.82532353 24.07.2026 07:48:17.953 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
First image: 2461245.82532353 24.07.2026 07:48:17.953 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Last image: 2461300.87383428 17.09.2026 08:58:09.282 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1152
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 63 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): 241639
Objects passed selection criteria: 240834
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: 158214
Average stars matched: 151367 (95.672 %)
Memory usage VmPeak: 696808 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 04:03:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
SExtractor catalog cache: saved Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.cat to cache
SExtractor catalog cache: saved Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.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: 2461300.87329296
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-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits exists and is non-empty
wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits exists and is non-empty
wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits exists and is non-empty
wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits (1st reference image)
verification OK: wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:36:03.270 +46:00:36.57 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits (1st new image)
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
Image size: 941.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:36:19.390 +46:00:22.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:36:03.270 +46:00:36.57
Second-epoch image center 21:36:19.390 +46:00:22.47
Angular distance between the image centers 0.0468 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits (2nd new image)
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
Image size: 941.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:36:16.957 +46:00:13.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:36:03.270 +46:00:36.57
Second-epoch image center 21:36:16.957 +46:00:13.36
Angular distance between the image centers 0.0401 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:36:19.390 +46:00:22.47
Second-epoch second image center 21:36:16.957 +46:00:13.36
Angular distance between the image centers 0.00748 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits &> /tmp/tmp.3barlnAlTv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits &> /tmp/tmp.lpBbTOA40S
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits &> /tmp/tmp.rgbqYdQqQj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits &> /tmp/tmp.MxO27LYcda
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits and wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits and wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
Found non-empty wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits and wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
The reference image (wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits) and catalog (wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat) found
'wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat' -> 'wcsmag.cat'
Read 34895 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 311.6628 to 336.3203 deg, Dec +40.3089 to +51.2694 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 311.6628 to 336.3203 deg, Dec 40.3089 to 51.2694 deg
Loaded 22786 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 15376 out of 17092 total matches.
Matched with Tycho-2 17092 out of 34895 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.639650
a=0.000000 b=1.000000 c=22.639650
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.12
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.12
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34895 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 311.6628 to 336.3203 deg, Dec +40.3089 to +51.2694 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 311.6628 to 336.3203 deg, Dec 40.3089 to 51.2694 deg
Loaded 22786 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 15376 out of 17092 total matches.
Matched with Tycho-2 17092 out of 34895 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Forced-photometry filter: calibrated wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits -> calib.txt_param_ref_wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits (aperture=6.3)
Read 34846 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 311.6977 to 336.3366 deg, Dec +40.3085 to +51.2755 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 311.6977 to 336.3366 deg, Dec 40.3085 to 51.2755 deg
Loaded 22774 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 15460 out of 17160 total matches.
Matched with Tycho-2 17160 out of 34846 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
Forced-photometry filter: calibrated wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits -> calib.txt_param_ref_wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 76 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
2.2 pix Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
2.6 pix fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
2.6 pix fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
Limiting magnitude estimates:
15.1 mag. Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
15.1 mag. Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
13.3 mag. fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
13.3 mag. fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
All-image limiting magnitude estimate: 13.3 (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.3barlnAlTv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits' -> 'wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
Checking if the catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat corresponding to the image wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits
WCS catalog name: wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4028, bad_region=0, passed=34895
Got 34895 stars (including 30831 good ones) from the SExtractor catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 34895 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 4927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 34895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 34895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 34895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4925 stars left (next iteration limit 5419)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits N_match=4925 sigma_overall_arcsec=0.629 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.750 sigma_q3_arcsec=0.574 sigma_q4_arcsec=0.725 n_q1=1127 n_q2=1072 n_q3=1228 n_q4=1498 worst_quadrant_to_overall_ratio=1.191
The image catalog is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits -region wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.lpBbTOA40S (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits' -> 'wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
WCS-calibrated image found: wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
Checking if the catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat corresponding to the image wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat corresponding to the image wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits
WCS catalog name: wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3993, bad_region=0, passed=34846
Got 34846 stars (including 30830 good ones) from the SExtractor catalog wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat
util/solve_plate_with_UCAC5 got 34846 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 4923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 34846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 34846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 34846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 4922 stars left (next iteration limit 5415)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits N_match=4922 sigma_overall_arcsec=0.616 sigma_q1_arcsec=0.460 sigma_q2_arcsec=0.738 sigma_q3_arcsec=0.548 sigma_q4_arcsec=0.693 n_q1=1113 n_q2=1072 n_q3=1245 n_q4=1492 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits -region wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.rgbqYdQqQj (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-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.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-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
Checking if the catalog wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits.wcscat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits.wcscat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.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-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
WCS catalog name: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.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=282, bad_region=2, passed=6016
Got 6016 stars (including 5726 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits.wcscat
util/solve_plate_with_UCAC5 got 6016 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 51.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 4882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 6010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 51.3)
Done reading UCAC5 zone files...
Matched 4936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 6010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 6010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4882 stars left (next iteration limit 5371)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4882 robust_rms=13.615 arcsec worst_quadrant_rms=22.814 arcsec
SIP_REFIT: SIP order 3 trial: matched=4882 robust_rms=0.513 arcsec worst_quadrant_rms=0.574 arcsec
SIP_REFIT: SIP order 5 trial: matched=4882 robust_rms=0.373 arcsec worst_quadrant_rms=0.501 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4882 robust_rms_before=0.723 arcsec robust_rms_before_corrected=0.457 arcsec robust_rms_after=0.373 arcsec worst_quadrant_rms_before=0.648 worst_quadrant_rms_after=0.501
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
Image size: 941.4'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: 21:36:19.417 +46:00:22.57 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 6016 stars ###
'wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/correct_sextractor_wcs_catalog_usingxy2sky912911.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.723 -> 0.373 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4882 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 4700 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4700 pairs (4882 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4700 robust_rms=12.857 arcsec worst_quadrant_rms=23.290 arcsec
SIP_REFIT: SIP order 3 trial: matched=4700 robust_rms=0.508 arcsec worst_quadrant_rms=0.557 arcsec
SIP_REFIT: SIP order 5 trial: matched=4700 robust_rms=0.365 arcsec worst_quadrant_rms=0.497 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4700 robust_rms_before=0.368 arcsec robust_rms_before_corrected=0.368 arcsec robust_rms_after=0.365 arcsec worst_quadrant_rms_before=0.494 worst_quadrant_rms_after=0.497
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.497 vs 0.494 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: 4700 matched stars entering correct_measured_positions(), 6010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4700 matched stars entering correct_measured_positions(), 6009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WCS_QUALITY_DIAG: file=fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits N_match=4700 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.424 sigma_q2_arcsec=0.506 sigma_q3_arcsec=0.328 sigma_q4_arcsec=0.351 n_q1=1847 n_q2=542 n_q3=1035 n_q4=1276 worst_quadrant_to_overall_ratio=1.305
The image catalog is written to wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits -region wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.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.MxO27LYcda (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-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.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-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
WCS-calibrated image found: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
Checking if the catalog wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat corresponding to the image wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.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-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
WCS catalog name: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.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=285, bad_region=0, passed=5844
Got 5844 stars (including 5551 good ones) from the SExtractor catalog wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat
util/solve_plate_with_UCAC5 got 5844 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 51.3)
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: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 5844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 51.3)
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: 4885 matched stars entering correct_measured_positions(), 5844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 5844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4885 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4885 robust_rms=15.331 arcsec worst_quadrant_rms=17.168 arcsec
SIP_REFIT: SIP order 3 trial: matched=4885 robust_rms=0.530 arcsec worst_quadrant_rms=0.576 arcsec
SIP_REFIT: SIP order 5 trial: matched=4885 robust_rms=0.383 arcsec worst_quadrant_rms=0.497 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4885 robust_rms_before=0.740 arcsec robust_rms_before_corrected=0.446 arcsec robust_rms_after=0.383 arcsec worst_quadrant_rms_before=0.665 worst_quadrant_rms_after=0.497
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
verification OK: wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
Image size: 941.4'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: 21:36:16.985 +46:00:13.51 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5844 stars ###
'wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/correct_sextractor_wcs_catalog_usingxy2sky912860.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.740 -> 0.383 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4885 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 51.3)
Done reading UCAC5 zone files...
Matched 4684 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4684 pairs (4885 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4684 robust_rms=14.946 arcsec worst_quadrant_rms=16.837 arcsec
SIP_REFIT: SIP order 3 trial: matched=4684 robust_rms=0.518 arcsec worst_quadrant_rms=0.555 arcsec
SIP_REFIT: SIP order 5 trial: matched=4684 robust_rms=0.377 arcsec worst_quadrant_rms=0.479 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4684 robust_rms_before=0.377 arcsec robust_rms_before_corrected=0.377 arcsec robust_rms_after=0.377 arcsec worst_quadrant_rms_before=0.478 worst_quadrant_rms_after=0.479
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.479 vs 0.478 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: 4684 matched stars entering correct_measured_positions(), 5844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4684 matched stars entering correct_measured_positions(), 5842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WCS_QUALITY_DIAG: file=fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits N_match=4684 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.512 sigma_q3_arcsec=0.319 sigma_q4_arcsec=0.368 n_q1=1665 n_q2=602 n_q3=1058 n_q4=1359 worst_quadrant_to_overall_ratio=1.302
The image catalog is written to wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits -region wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits to local_wcs_cache/
'wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits'
Saving the final (post-refit) wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits to local_wcs_cache/
'wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits' -> 'local_wcs_cache/wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits'
Saving the final (post-refit) wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits'
Saving the final (post-refit) wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits to local_wcs_cache/
'wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits' -> 'local_wcs_cache/wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits sigma_overall=0.629 worst_q_ratio=1.191
ref2=Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits sigma_overall=0.616 worst_q_ratio=1.197
new1=fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits sigma_overall=0.388 worst_q_ratio=1.305
new2=fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits sigma_overall=0.393 worst_q_ratio=1.302
reference average sigma_overall=0.6225 worst_q_ratio=1.194
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132_astrometric_residuals.png (4925 matched stars from wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.55 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133_astrometric_residuals.png (4922 matched stars from wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010_astrometric_residuals.png (4700 matched stars from wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011_astrometric_residuals.png (4684 matched stars from wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits'
Saving fully-calibrated image wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits'
Preparing the HTML report for the field Cyg-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:37.91 +41:58:56.6: 11.74 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:37.91 +41:58:56.6: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry filter KEPT candidate at 20:57:37.91 +41:58:56.6: ref_mag=11.75 +/- 0.01 new_mean_mag=10.6843 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:15.37 +41:41:22.2: 12.00 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:02.87 +41:31:54.4: 12.03 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:38.89 +41:41:51.0: 12.01 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:56:07.05 +42:02:47.1: 11.98 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:47.89 +41:37:34.8: 11.98 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:15.37 +41:41:22.2: 11.99 +/- 0.02 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:02.87 +41:31:54.4: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 20:55:15.37 +41:41:22.2: ref_mag=12.00 +/- 0.01 new_mean_mag=10.8038 delta=1.19 (need > 0.90)
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter KEPT candidate at 20:55:02.87 +41:31:54.4: ref_mag=12.04 +/- 0.01 new_mean_mag=10.8527 delta=1.18 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:38.89 +41:41:51.0: 12.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter KEPT candidate at 20:55:38.89 +41:41:51.0: ref_mag=12.04 +/- 0.01 new_mean_mag=10.7081 delta=1.33 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:56:07.05 +42:02:47.1: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter KEPT candidate at 20:56:07.05 +42:02:47.1: ref_mag=11.96 +/- 0.01 new_mean_mag=10.8660 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:47.89 +41:37:34.8: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 20:55:47.89 +41:37:34.8: ref_mag=12.00 +/- 0.01 new_mean_mag=10.8059 delta=1.19 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:58:10.77 +42:28:39.4: 11.83 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:58:10.77 +42:28:39.4: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry filter KEPT candidate at 20:58:10.77 +42:28:39.4: ref_mag=11.83 +/- 0.01 new_mean_mag=10.8183 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:57:25.13 +41:55:56.1: 11.78 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:57:25.13 +41:55:56.1: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry filter KEPT candidate at 20:57:25.13 +41:55:56.1: ref_mag=11.78 +/- 0.01 new_mean_mag=10.6988 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:28.11 +41:17:39.5: 11.71 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:28.11 +41:17:39.5: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Forced photometry filter KEPT candidate at 20:55:28.11 +41:17:39.5: ref_mag=11.72 +/- 0.01 new_mean_mag=10.6151 delta=1.11 (need > 0.90)
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-48-17_20.00sec_4.90C_LIGHT_0132.fits at 20:55:34.56 +41:36:48.0: 11.67 +/- 0.01 detection
Forced photometry on wcs_Cyg-04-Q1b1x1_2026-07-24_02-49-06_20.00sec_4.90C_LIGHT_0133.fits at 20:55:34.56 +41:36:48.0: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Forced photometry filter KEPT candidate at 20:55:34.56 +41:36:48.0: ref_mag=11.67 +/- 0.01 new_mean_mag=10.5198 delta=1.15 (need > 0.90)
Adding exclusion_list_local.txt__out02636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05569.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 5s
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Considering the candidate 52621_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 52621_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:03.35 +41:10:49.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 52637_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 52637_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:15.18 +41:08:42.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 02504_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02504_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:12.11 +41:17:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02291_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02291_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:41.39 +41:12:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02864_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02864_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:09.57 +41:26:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02565_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02565_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:57.64 +41:16:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02446_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02446_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:33.77 +41:13:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06396_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 06396_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:54:18.95 +42:41:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04274_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 04274_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 03292_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03292_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:09.05 +41:33:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03837_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03837_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:26.70 +41:48:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02047_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02047_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:01.12 +41:08:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04028_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04028_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:31.49 +41:53:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03899_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03899_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:59.93 +41:52:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04562_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04562_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:21.11 +42:02:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03879_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03879_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:59.46 +41:50:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04514_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04514_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:46.72 +42:04:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02061_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02061_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:20.92 +41:05:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02900_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02900_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:59.76 +41:30:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03472_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03472_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:35.86 +41:39:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02957_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02957_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:29.75 +41:29:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03271_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03271_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:28.93 +41:32:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04400_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04400_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:41.93 +42:00:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02141_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02141_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:29.21 +41:08:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03267_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 03267_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 03667_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 03667_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 03330_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03330_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:51.01 +41:35:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04799_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04799_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:10.75 +42:08:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03855_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03855_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:54:53.19 +41:46:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03655_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 03655_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 04529_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 04529_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 01936_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 01936_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:57.35 +41:05:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09428_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 09428_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:48:42.19 +44:14:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03459_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 03459_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 03565_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03565_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:33.67 +41:44:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03933_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03933_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:40.93 +41:52:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02653_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02653_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:05.54 +41:18:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03957_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03957_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:33.20 +41:53:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03467_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03467_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:03.32 +41:39:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02185_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02185_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:57.83 +41:08:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02956_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02956_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:17.62 +41:31:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02281_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02281_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:58.88 +41:12:11.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 03498_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03498_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:29.23 +41:43:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02771_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02771_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:37.71 +41:22:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05569_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 05569_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 02804_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02804_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:36.91 +41:23:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01717_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 01717_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:32.53 +40:58:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02564_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02564_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:46.73 +41:21:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04611_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04611_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:15.59 +42:10:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01862_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 01862_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:37.60 +41:01:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04159_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 04159_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 02166_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02166_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:29.94 +41:12:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04326_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04326_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:07.99 +41:56:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02873_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02873_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:25.84 +41:26:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05467_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 05467_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:54:33.85 +42:22:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03175_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03175_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:04.59 +41:32:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02636_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 02636_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 02454_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02454_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:57.80 +41:14:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03702_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03702_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:38.26 +41:49:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03443_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 03443_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 01727_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 01727_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:09.59 +41:02:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03488_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03488_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:10.99 +41:43:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02323_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02323_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:09.15 +41:12:51.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 04518_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04518_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:43.09 +42:03:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05507_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 05507_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:11.69 +42:28:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02491_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02491_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:09.56 +41:15:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05027_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 05027_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:59.82 +42:18:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02736_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02736_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:32.83 +41:20:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04436_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 04436_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:01.58 +42:06:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03700_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03700_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:40.03 +41:46:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03153_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03153_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:32.73 +41:35:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03581_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03581_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:34.39 +41:45:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06021_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 06021_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:25.22 +42:39:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02740_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 02740_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:25.10 +41:24:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03013_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03013_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:38.82 +41:32:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03511_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 03511_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
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Considering the candidate 299236_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299236_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 299246_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299246_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299255_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299255_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299258_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299258_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
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Considering the candidate 299265_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299265_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299269_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299269_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:15:26.75 +49:07:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299294_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299294_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299300_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299300_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299302_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299302_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:15:49.49 +48:56:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299312_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299312_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:19:48.45 +44:56:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299335_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299335_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299340_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299340_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299342_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299342_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:10:56.11 +49:51:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299354_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299354_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299355_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299355_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299361_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299361_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:15:09.62 +49:04:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299363_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299363_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299364_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299364_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:19:03.59 +48:52:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299371_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299371_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299372_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299372_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299373_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299373_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:23:30.59 +49:34:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 0.342 1999769625234761600 335.87732737119 +49.57081852677 13.6279 12.7911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 299375_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299375_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299380_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299380_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 299384_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299384_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:19:58.41 +49:07:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299386_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299386_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:22:29.57 +49:46:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299393_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299393_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:08:53.34 +41:13:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299394_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299394_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299398_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299398_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:10:33.04 +50:10:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299399_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299399_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299404_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299404_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299411_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299411_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:07:30.66 +41:21:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299414_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299414_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299415_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299415_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299416_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299416_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 299417_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299417_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:18:44.42 +49:09:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299418_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299418_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.2") between the two second-epoch detections
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Considering the candidate 299419_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299419_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299428_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299428_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:14:37.28 +50:20:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299431_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299431_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:17:33.51 +49:16:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:21:51.80 +49:56:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299440_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299440_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299496_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299496_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 299497_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299497_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
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Considering the candidate 299660_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299660_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 299696_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299696_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 299704_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299704_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 299721_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299721_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 299722_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299722_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299728_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299728_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 299752_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299752_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 299805_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299805_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 299811_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299811_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 299842_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299842_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:14.32 +42:31:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299859_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299859_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 299874_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299874_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 299881_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299881_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 299963_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299963_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 299977_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299977_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 299983_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299983_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
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Considering the candidate 299984_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 299984_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 300018_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300018_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 300024_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300024_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 300088_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300088_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 300129_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300129_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 300132_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300132_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:10:08.84 +43:59:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300164_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300164_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 300166_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300166_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 300174_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300174_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 300227_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300227_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 300228_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300228_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 300260_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300260_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 300270_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300270_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
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Considering the candidate 300287_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300287_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 300291_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300291_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 300301_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300301_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 300311_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300311_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 300324_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300324_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 300326_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300326_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 300342_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300342_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 300363_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300363_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 300367_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300367_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 300372_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300372_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 300396_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300396_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.2") between the two second-epoch detections
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Considering the candidate 300405_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300405_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 300409_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300409_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 300416_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300416_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 300429_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300429_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 300449_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300449_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:10:25.99 +47:08:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300454_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300454_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 300459_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300459_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:54:21.36 +45:19:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300478_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300478_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:21:13.43 +46:32:45.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 300479_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300479_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 300502_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300502_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:15:06.31 +49:51:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300504_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300504_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 300520_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300520_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 300576_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300576_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 300584_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300584_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 300596_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300596_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 300603_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300603_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:54:10.17 +45:07:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300605_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300605_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 300612_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300612_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
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Considering the candidate 300618_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300618_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:14:19.01 +49:55:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300631_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300631_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 300644_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300644_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:50.70 +47:23:45.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 300679_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300679_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 300685_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300685_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:24:05.70 +49:28:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.931 1999778971083909120 336.02456694766 +49.47017425478 13.5440 12.6856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 300697_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300697_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:15:52.91 +49:56:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300701_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300701_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (30.8") between the two second-epoch detections
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Considering the candidate 300737_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300737_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 300768_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300768_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:05.00 +42:43:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300776_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300776_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:08:33.05 +45:45:12.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 300784_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300784_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:16:17.35 +45:29:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300796_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300796_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 300813_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300813_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 300816_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300816_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 300834_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300834_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 300842_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300842_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 300871_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300871_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 300872_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300872_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 300879_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300879_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 300884_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300884_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 300888_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300888_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 300900_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300900_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 300921_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300921_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 300932_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300932_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 300938_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300938_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 300962_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300962_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:05:43.90 +45:06:57.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 300981_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300981_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
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Considering the candidate 300997_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 300997_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 301001_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301001_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:19:52.33 +44:56:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.694 1962105098504477312 334.96812008692 +44.94634305721 13.9459 13.1966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 301029_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301029_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 301032_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301032_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:15:43.92 +47:57:21.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 301035_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301035_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 301065_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301065_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 301071_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301071_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 301073_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301073_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 301104_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301104_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 301211_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301211_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 301214_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301214_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 301256_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301256_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 301259_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301259_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 301306_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301306_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 301329_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301329_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 301335_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301335_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 301351_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301351_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 301365_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301365_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:30.69 +47:30:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 301406_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301406_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 301431_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301431_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 301437_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301437_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 301441_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301441_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 301458_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301458_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 301465_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301465_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 301476_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301476_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 301487_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301487_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 301489_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301489_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 301507_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301507_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 301510_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301510_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 301512_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301512_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 301548_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301548_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 301558_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301558_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 301567_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301567_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:45:31.43 +43:55:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 301571_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301571_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 301586_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301586_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 301591_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301591_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:20:34.43 +48:55:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.384 1999647888681312256 335.14390521492 +48.92058129150 14.0979 13.2874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 301594_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301594_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 301598_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301598_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 301628_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301628_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 301660_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301660_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 301673_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301673_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 301678_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301678_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 301683_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301683_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 301695_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301695_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 301710_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301710_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 301713_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301713_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 301721_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301721_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 301728_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301728_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 301732_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301732_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
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Considering the candidate 301733_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301733_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 301741_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 301741_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 19395_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19395_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:01.16 +41:27:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23098_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23098_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:09.05 +41:33:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10381_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10381_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:24.80 +41:02:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23986_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23986_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 31455_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 31455_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24182_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24182_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:03.33 +41:39:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243137_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 243137_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 28219_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28219_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14521_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14521_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:29.25 +41:08:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22465_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22465_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:28.93 +41:32:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24594_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24594_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:27.38 +41:40:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28031_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28031_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 159255_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 159255_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 16826_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16826_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:51.52 +41:18:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17091_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17091_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:12.11 +41:17:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19497_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19497_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:09.56 +41:26:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 15435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18500_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18500_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:32.82 +41:20:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11541_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11541_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:09.56 +41:02:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17294_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17294_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:57.66 +41:16:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15534_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15534_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:09.12 +41:12:51.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 18782_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18782_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:37.70 +41:22:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25183_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25183_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:15.32 +41:41:22.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 22584_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22584_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:50.97 +41:35:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19818_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19818_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:34.57 +41:26:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24090_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24090_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:26.85 +41:44:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25641_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25641_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32262_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32262_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20183_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20183_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:55.38 +41:35:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103114_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 103114_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 28041_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28041_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24724_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 24724_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 51243_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 51243_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18637_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18637_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:20.47 +41:23:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40157_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40157_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 10978_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10978_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:21.09 +41:02:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20568_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20568_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:14.55 +41:31:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14981_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14981_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:00.85 +41:13:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30041_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30041_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 123592_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 123592_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 16215_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16215_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:08.52 +41:17:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27108_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 27108_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:43.61 +41:52:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23341_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23341_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 22989_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22989_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:40.45 +41:41:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20401_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 20401_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14729_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14729_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:41.56 +41:09:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24976_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 24976_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 39255_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39255_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29091_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29091_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25242_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25242_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:25.82 +41:48:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10687_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10687_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:42.42 +41:02:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30113_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30113_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23635_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23635_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:50.69 +41:42:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19787_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19787_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:13.64 +41:31:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19023_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19023_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:43.94 +41:27:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35989_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 35989_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25444_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25444_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 15506_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15506_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:00.68 +41:15:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27076_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 27076_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:54.77 +41:52:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19499_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19499_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:09.81 +41:25:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32946_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32946_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27314_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 27314_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:18.55 +41:54:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20668_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20668_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:02.74 +41:29:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26718_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26718_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:03.84 +41:52:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32165_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32165_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19299_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19299_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11250_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11250_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:15.23 +40:59:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41595_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 41595_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12707_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12707_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:56.96 +41:07:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16667_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16667_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:50.28 +41:17:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24789_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24789_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:15.40 +41:44:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22106_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22106_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 100765_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 100765_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:15:51.52 +44:57:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.542 1962218142044068224 333.96595479583 +44.95235198104 13.9432 13.0906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 30911_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30911_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12197_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12197_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:02.60 +41:04:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30500_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30500_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16218_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16218_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:59.56 +41:18:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38355_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 38355_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 31697_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 31697_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17217_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17217_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 37036_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 37036_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 47583_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 47583_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19233_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19233_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:42.25 +41:32:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244536_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 244536_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 47904_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 47904_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 39425_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39425_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 33185_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33185_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25886_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25886_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:20.74 +41:51:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285369_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 285369_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
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Considering the candidate 21968_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 21968_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 34608_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 34608_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 99114_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99114_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 44118_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 44118_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 33473_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33473_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18479_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 18479_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29106_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29106_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26790_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26790_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:10.29 +41:52:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.364 2065655832299486208 314.79236613700 +41.87602130412 13.3307 11.9890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 17049_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17049_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:11.65 +41:18:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35062_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 35062_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21295_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 21295_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23316_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23316_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 10359_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10359_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:22.15 +40:58:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23143_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23143_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 297424_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 297424_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 27435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18150_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18150_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:18.09 +41:23:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46851_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 46851_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19507_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19507_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:53.21 +41:32:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20819_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20819_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:14.88 +41:32:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10380_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10380_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:05.80 +41:01:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16545_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16545_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:23.07 +41:21:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242992_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 242992_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 35118_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 35118_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14712_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 14712_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20219_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20219_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:53.84 +41:34:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105676_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 105676_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13074_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13074_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:05.73 +41:03:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20088_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20088_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:34.27 +41:33:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28110_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28110_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 28833_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28833_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 83619_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 83619_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 100849_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 100849_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 291620_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 291620_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 34356_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 34356_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29332_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29332_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25941_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25941_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:57.77 +41:52:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25647_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25647_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:01.24 +41:51:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52202_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 52202_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:10.63 +43:01:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14434_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14434_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:36.99 +41:14:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24552_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24552_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:46.58 +41:46:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42495_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 42495_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16069_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 16069_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23766_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23766_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:01.96 +41:45:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23451_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23451_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25440_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25440_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26395_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26395_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29326_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29326_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11174_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11174_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:23.49 +41:04:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26245_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26245_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:38.15 +41:51:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289033_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 289033_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18238_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18238_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:25.17 +41:23:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53637_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 53637_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21713_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21713_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:47.67 +41:35:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28187_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28187_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 40060_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40060_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19170_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19170_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 46152_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 46152_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:53.82 +42:45:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105154_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 105154_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14990_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 14990_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 105103_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 105103_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 287726_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 287726_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:16:38.74 +45:02:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.388 1962223845760826880 334.16140518682 +45.04074647003 14.4364 13.9262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 48625_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 48625_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24434_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 24434_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29826_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29826_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16404_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 16404_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30238_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30238_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19341_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19341_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 15687_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15687_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:29.42 +41:15:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28116_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28116_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 40406_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40406_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20703_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20703_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:19.40 +41:34:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14819_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14819_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:00.15 +41:14:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29378_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29378_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 40574_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40574_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 43366_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 43366_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17889_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17889_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:08.54 +41:22:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17345_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17345_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30747_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30747_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 38606_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 38606_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12479_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12479_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:19.97 +41:08:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27083_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27083_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 100020_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 100020_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26432_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26432_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:34.51 +41:50:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30147_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30147_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 33466_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33466_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13450_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13450_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:50.14 +41:08:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36168_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 36168_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 284045_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 284045_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:18.78 +41:33:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.096 2065643909469913984 314.57765049990 +41.55898366242 13.5864 12.2268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 19212_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19212_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 40771_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40771_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14673_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14673_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:52.00 +41:10:07.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 99783_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99783_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 15846_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15846_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:51.17 +41:15:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28917_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28917_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24862_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24862_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:50.69 +41:49:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99545_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99545_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 37164_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 37164_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 107162_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 107162_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12681_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12681_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:01.43 +41:06:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32235_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32235_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32582_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32582_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 104967_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 104967_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 45771_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 45771_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 281969_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 281969_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:16.99 +41:08:02.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 13688_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 13688_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 39231_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39231_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 101124_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 101124_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21811_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21811_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:55.00 +41:35:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11490_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11490_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:26.28 +41:01:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35830_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 35830_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 22015_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22015_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 280845_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 280845_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:48.69 +41:34:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30521_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30521_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30066_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30066_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24346_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24346_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:28.03 +41:45:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 280435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 280435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:19:02.18 +44:57:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.900 1962111966153266304 334.75907106154 +44.96161137960 13.8630 13.0353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 14188_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 14188_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 191777_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 191777_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 23560_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23560_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:01.30 +41:43:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102461_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 102461_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30264_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30264_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32385_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32385_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30387_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30387_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18460_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 18460_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25674_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25674_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21156_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 21156_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14700_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14700_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:02.60 +41:09:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25437_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25437_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 33864_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33864_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27238_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27238_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21310_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 21310_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17863_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17863_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20300_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 20300_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 51735_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 51735_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 248086_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 248086_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 29125_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29125_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 35218_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 35218_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 34134_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 34134_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 10932_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10932_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:02.76 +41:01:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29788_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29788_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21682_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21682_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:57.43 +41:37:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24400_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24400_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:13.41 +41:46:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22351_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22351_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32289_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 32289_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:21.30 +42:08:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17727_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17727_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12490_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12490_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:15.78 +41:05:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50422_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 50422_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 28320_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28320_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21688_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21688_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:03.92 +41:35:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29766_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29766_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 33095_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33095_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21428_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 21428_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27075_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27075_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 28715_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28715_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29857_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29857_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11057_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 11057_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 22652_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22652_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:54.49 +41:38:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27259_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27259_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 99817_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99817_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 102845_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 102845_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 34245_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 34245_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 33638_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33638_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21074_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21074_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:27.38 +41:37:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102562_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 102562_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20698_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20698_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:09.96 +41:30:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44980_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 44980_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19576_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19576_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:03.71 +41:32:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13976_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13976_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:17.42 +41:13:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29673_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29673_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20947_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 20947_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 104061_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 104061_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25750_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25750_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 99529_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99529_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26549_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26549_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 22234_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22234_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 48119_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 48119_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16850_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16850_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:24.34 +41:22:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31410_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 31410_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17491_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17491_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:05.53 +41:22:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29939_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29939_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18776_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18776_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:48.09 +41:25:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101712_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 101712_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26464_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26464_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:00.18 +41:50:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22839_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22839_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:41.29 +41:42:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39912_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39912_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 40356_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40356_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 231835_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 231835_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 22:22:18.97 +49:17:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24852_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 24852_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14960_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14960_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:36.79 +41:10:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22731_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22731_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:28.09 +41:36:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18508_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18508_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:07.66 +41:23:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99924_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99924_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27878_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27878_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 105623_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 105623_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 45588_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 45588_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 16433_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16433_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:19.44 +41:22:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24383_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24383_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:37.12 +41:46:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27674_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27674_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29046_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 29046_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:28.34 +42:00:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34475_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 34475_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 22276_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22276_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 100461_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 100461_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 47750_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 47750_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 38107_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 38107_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20853_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20853_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:04.08 +41:36:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18151_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18151_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:23.92 +41:27:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16307_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16307_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:38.62 +41:17:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33199_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 33199_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:11.54 +42:13:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20895_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 20895_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27046_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27046_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11563_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11563_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:00.06 +41:00:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27666_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27666_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 33748_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33748_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14159_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14159_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:57.21 +41:12:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38811_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 38811_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 100215_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 100215_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25742_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25742_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19423_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19423_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23076_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23076_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20896_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 20896_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25112_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25112_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17496_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17496_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27822_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 27822_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:14.22 +41:56:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23731_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23731_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:40.20 +41:41:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29343_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29343_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 10653_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10653_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:38.01 +40:58:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21498_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 21498_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19026_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19026_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:35.63 +41:25:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102569_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 102569_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30123_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30123_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29162_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 29162_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:16.08 +42:00:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30436_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30436_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29947_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29947_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32454_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32454_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29582_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29582_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 31448_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 31448_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18973_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18973_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:02.83 +41:27:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23417_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23417_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:54.98 +41:43:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99066_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99066_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32428_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32428_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11412_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11412_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:33.57 +41:04:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19387_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19387_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:24.31 +41:28:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 35213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30202_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30202_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18038_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18038_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:09.17 +41:26:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26434_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26434_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:42.14 +41:52:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13518_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13518_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:32.57 +41:04:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22560_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22560_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:53.10 +41:35:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12734_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12734_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:54.90 +41:02:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21504_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21504_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:39.93 +41:33:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102760_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 102760_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26057_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26057_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:42.64 +41:47:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19113_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19113_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:15.73 +41:28:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30912_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30912_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25854_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25854_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:37.55 +41:48:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30546_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30546_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32095_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32095_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14466_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 14466_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25838_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25838_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27627_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27627_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 40767_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 40767_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 53304_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 53304_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 41685_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 41685_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14975_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 14975_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:37.48 +41:22:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96594_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 96594_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24618_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 24618_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 15189_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15189_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:20.04 +41:15:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19292_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19292_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:11.66 +41:30:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33795_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33795_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 42852_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 42852_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19107_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19107_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:18.28 +41:25:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21368_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21368_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:22.30 +41:36:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13557_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13557_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:48.93 +41:05:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28297_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 28297_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:02.37 +41:59:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38666_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 38666_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23865_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23865_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:49.83 +41:44:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24215_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24215_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:11.67 +41:39:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40364_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40364_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19293_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19293_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:41.74 +41:30:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14129_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14129_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:43.67 +41:13:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13787_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13787_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:08.33 +41:11:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31418_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 31418_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:16.53 +42:06:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51613_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 51613_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 15279_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15279_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:12.15 +41:13:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26742_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26742_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:45.04 +41:50:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30111_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30111_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29024_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29024_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18185_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18185_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:36.61 +41:24:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32017_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32017_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 99601_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99601_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17661_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17661_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 36013_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 36013_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29678_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 29678_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:39.08 +42:02:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18034_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 18034_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 34246_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 34246_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13049_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 13049_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17855_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17855_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14927_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14927_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:40.73 +41:13:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20269_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20269_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:28.58 +41:32:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23762_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23762_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:56.85 +41:41:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97046_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 97046_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25082_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25082_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:30.81 +41:44:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09989_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 09989_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:56.86 +41:00:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16867_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 16867_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25475_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25475_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:57.84 +41:47:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38347_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 38347_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12788_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12788_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:25.36 +41:06:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18671_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18671_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:01.29 +41:24:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22310_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22310_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13039_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13039_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:37.41 +41:08:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30676_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30676_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16782_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16782_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:52.08 +41:15:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26194_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26194_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:31.42 +41:50:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11077_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11077_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:18.34 +40:58:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20273_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20273_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:54.27 +41:26:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39709_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39709_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17631_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17631_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:49.74 +41:24:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21710_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21710_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:59.20 +41:38:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25644_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25644_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30736_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30736_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 28991_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28991_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19147_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19147_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18691_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 18691_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21841_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21841_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:51.55 +41:35:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28433_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28433_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11173_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11173_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:50.28 +41:00:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103587_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 103587_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 31509_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 31509_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:42.62 +42:06:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27986_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27986_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18663_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18663_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:20.61 +41:21:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11328_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11328_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:10.85 +41:01:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10440_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10440_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:54.75 +41:01:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26918_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26918_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 81142_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 81142_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20671_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 20671_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 33228_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 33228_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19997_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19997_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:41.79 +41:31:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24731_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 24731_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14877_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14877_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:10.11 +41:15:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24918_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 24918_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 43530_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 43530_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 41748_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 41748_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 80395_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 80395_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 22653_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22653_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:40.80 +41:39:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30647_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 30647_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:52.35 +42:03:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43469_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 43469_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17526_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17526_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:29.59 +41:26:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23621_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23621_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18066_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18066_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:45.54 +41:21:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43337_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 43337_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20533_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20533_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:00.26 +41:32:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107085_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 107085_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29660_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 29660_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 16751_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16751_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:17.08 +41:16:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36521_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 36521_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14792_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 14792_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27443_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27443_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14041_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14041_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:26.39 +41:05:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10506_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10506_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:20.91 +41:00:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 15277_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15277_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:45.80 +41:17:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40288_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40288_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32416_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32416_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18184_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18184_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:37.40 +41:21:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10267_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10267_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:43.86 +41:00:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09988_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 09988_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:57.46 +40:58:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104013_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 104013_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26663_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26663_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20058_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20058_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:42.54 +41:30:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28716_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 28716_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:19.84 +41:56:55.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29785_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29785_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17695_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 17695_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17913_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17913_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:58.10 +41:19:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22809_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22809_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:27.45 +41:41:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30887_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30887_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29171_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29171_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11168_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11168_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:05.80 +41:02:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29231_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29231_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 95668_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 95668_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 239515_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 239515_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24518_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24518_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:25.22 +41:45:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26388_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26388_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12269_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12269_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:20.80 +41:04:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97796_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 97796_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12650_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12650_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:21.59 +41:06:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21013_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 21013_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16593_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16593_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:51.47 +41:23:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24444_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 24444_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19025_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19025_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:59.20 +41:22:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17352_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17352_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:12.49 +41:19:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104010_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 104010_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29270_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29270_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21274_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21274_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:58:37.06 +41:46:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243177_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 243177_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 28913_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28913_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20636_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20636_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:34.90 +41:30:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15925_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15925_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:59.64 +41:14:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98582_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 98582_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 39633_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39633_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 31573_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 31573_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 19211_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19211_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29795_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29795_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 96444_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 96444_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 239336_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 239336_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12516_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12516_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:00.24 +41:02:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27744_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27744_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30880_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30880_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:29.20 +41:32:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12890_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12890_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:42.44 +41:05:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26985_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26985_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12446_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12446_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:46.51 +41:02:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37494_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 37494_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 22648_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22648_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11006_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11006_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:07.88 +40:56:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30142_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30142_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 261804_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 261804_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 31662_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 31662_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 15910_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15910_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:36.51 +41:19:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23802_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23802_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13009_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13009_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:31.85 +41:06:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23504_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23504_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:46.35 +41:42:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19855_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19855_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:04.81 +41:28:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102745_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 102745_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25798_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25798_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16405_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16405_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:28.98 +41:20:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10745_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 10745_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:20.61 +40:56:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12757_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12757_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:29.41 +41:05:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26803_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26803_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18441_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18441_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:03.12 +41:26:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244409_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 244409_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 45298_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 45298_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 40051_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 40051_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27708_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27708_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16909_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16909_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:45.86 +41:17:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29291_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29291_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24550_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24550_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:20.16 +41:46:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18855_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18855_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:48.24 +41:26:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16338_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16338_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:58.12 +41:16:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24022_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24022_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:38.44 +41:42:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39513_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39513_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 38570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 38570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14848_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14848_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:58.80 +41:11:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25652_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25652_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26751_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26751_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 246277_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 246277_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 37258_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 37258_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21350_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 21350_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 238827_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 238827_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23907_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23907_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25612_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25612_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27572_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27572_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 243080_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 243080_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 16090_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16090_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:28.67 +41:20:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99375_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99375_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14123_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14123_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:02.92 +41:08:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15336_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15336_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:41.37 +41:12:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10576_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 10576_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30649_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30649_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20394_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20394_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:49.67 +41:33:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15993_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15993_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:27.46 +41:16:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38062_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 38062_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13712_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13712_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:20.90 +41:05:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23582_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23582_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:01.02 +41:41:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22548_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22548_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 106638_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 106638_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30070_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30070_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25698_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25698_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 22181_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22181_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:02.85 +41:31:54.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 227352_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 227352_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
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Considering the candidate 19996_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 19996_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:29.73 +41:29:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25327_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25327_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:38.88 +41:41:51.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 25975_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25975_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:08.89 +41:49:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18283_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18283_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:50.67 +41:20:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20923_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20923_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:21.86 +41:33:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82905_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 82905_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23735_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23735_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:47.86 +41:37:34.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 103564_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 103564_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 103073_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 103073_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25962_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25962_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:08.10 +41:47:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34071_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 34071_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 17753_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17753_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:05.53 +41:18:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31759_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 31759_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:07.04 +42:02:47.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 16951_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 16951_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 31846_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 31846_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:36.61 +42:08:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14261_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14261_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:00.88 +41:08:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23174_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23174_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 39819_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39819_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13079_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13079_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:32.89 +41:05:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27375_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27375_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21288_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21288_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:41.31 +41:33:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31195_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 31195_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20057_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20057_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:17.62 +41:31:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12233_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12233_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:46.00 +41:05:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14196_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14196_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:51.31 +41:11:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18815_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 18815_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 88746_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 88746_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 30215_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 30215_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 18970_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18970_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:36.91 +41:23:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30538_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 30538_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:08.01 +41:56:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236241_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 236241_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 31830_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 31830_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:01.56 +42:06:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100230_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 100230_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 39539_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 39539_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:10.75 +42:28:39.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 103456_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 103456_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 216841_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 216841_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 19933_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19933_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 210745_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 210745_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 26585_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26585_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:41.05 +41:52:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14489_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14489_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:29.94 +41:12:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100413_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 100413_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 29011_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 29011_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:25.12 +41:55:56.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 82313_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 82313_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 31236_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 31236_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23960_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 23960_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21571_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21571_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:04.60 +41:32:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29932_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 29932_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:37.89 +41:58:56.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 17790_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17790_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:28.10 +41:17:39.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 16396_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16396_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:57.80 +41:14:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24479_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24479_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:53.30 +41:49:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16337_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16337_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:33.75 +41:13:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26626_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26626_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 23629_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23629_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:34.54 +41:36:47.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 39574_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 39574_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:11.67 +42:28:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25924_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25924_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20095_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20095_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:39.04 +41:32:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99437_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 99437_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14004_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14004_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:08.11 +41:08:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21856_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21856_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:56.52 +41:38:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103115_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 103115_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16811_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16811_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:09.56 +41:15:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236673_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 236673_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 26813_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26813_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13109_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13109_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:11.62 +41:10:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39484_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 39484_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:04.00 +42:30:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19833_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 19833_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32806_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32806_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20125_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20125_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:22.51 +41:32:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26681_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26681_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:40.37 +41:54:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28962_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28962_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25670_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 25670_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:40.00 +41:46:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27466_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27466_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21570_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:32.71 +41:35:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18250_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18250_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:28.63 +41:25:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102191_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 102191_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 43416_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 43416_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:25.21 +42:39:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73928_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 73928_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:48:42.18 +44:14:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18698_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18698_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:25.08 +41:24:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20633_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20633_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:38.82 +41:32:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235268_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 235268_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25423_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25423_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27221_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27221_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24211_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24211_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:41.60 +41:42:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106000_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 106000_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 16435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16435_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:58.13 +41:21:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11965_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11965_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:01.45 +41:06:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104914_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 104914_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14195_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14195_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:47.22 +41:09:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23919_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23919_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:35.85 +41:39:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30943_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 30943_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:41.94 +42:00:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25856_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25856_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27419_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 27419_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:59.44 +41:50:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27279_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 27279_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:54:53.16 +41:46:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227212_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 227212_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
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Considering the candidate 35088_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 35088_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11774_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11774_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:48.92 +41:05:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32132_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 32132_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:21.11 +42:02:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29686_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 29686_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 12148_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12148_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:25.32 +41:02:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13103_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13103_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:57.37 +41:05:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27658_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 27658_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:40.92 +41:52:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18816_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18816_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:29.23 +41:27:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26685_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 26685_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:03:09.32 +41:56:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101996_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 101996_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27750_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 27750_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:33.17 +41:53:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27892_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27892_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 98345_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 98345_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 27346_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27346_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 14912_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14912_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:57.84 +41:08:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18783_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18783_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:39.18 +41:28:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13524_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13524_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:09:57.18 +41:19:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28118_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 28118_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 15531_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 15531_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:58.87 +41:12:11.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 37497_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 37497_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 25810_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25810_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 24721_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24721_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:29.23 +41:43:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13745_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13745_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:17.64 +41:11:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 241071_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 241071_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 104115_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 104115_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 11793_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 11793_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:32.54 +40:58:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13101_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13101_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:55:37.59 +41:01:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17431_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17431_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:46.73 +41:21:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17920_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 17920_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:39.26 +41:25:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39259_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39259_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 32012_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 32012_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 20024_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20024_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:25.83 +41:26:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24067_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24067_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:15.21 +41:45:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27233_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27233_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 242118_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 242118_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 104056_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 104056_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 21429_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21429_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:06.59 +41:36:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22390_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22390_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:06.63 +41:36:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22149_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 22149_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:05.85 +41:31:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27827_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27827_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
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Considering the candidate 13471_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 13471_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:57:11.87 +41:06:31.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 11084_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 11084_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36743_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 36743_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16629_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16629_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:56:36.29 +41:16:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16259_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 16259_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:03:20.74 +41:23:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14584_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 14584_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:02:06.73 +41:16:01.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24551_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 24551_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:30.24 +41:46:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21157_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21157_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:03.12 +41:34:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39613_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39613_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20512_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20512_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:21.53 +41:32:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22398_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 22398_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27394_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27394_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39951_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 39951_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21131_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 21131_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:44.50 +41:33:20.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25891_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 25891_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18353_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18353_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:20.87 +41:26:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28543_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 28543_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:04:07.59 +42:02:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23501_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 23501_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:01:46.02 +41:44:28.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105568_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 105568_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37684_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 37684_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12225_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 12225_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:58:57.48 +41:04:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27520_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 27520_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18309_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 18309_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26279_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 26279_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 20213_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 20:59:35.92 +41:31:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216944_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
Preparing report for the candidate 216944_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18777_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011
The candidate 18777_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011 did not pass the final checks
**** FOUND 21:00:26.93 +41:27:45.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 24s
make_report_in_HTML.sh TOTAL: 669s
Prepared the HTML report for the field Cyg-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:55:28.11 +41:17:39.5
20:55:02.87 +41:31:54.4
20:55:34.56 +41:36:48.0
20:55:47.89 +41:37:34.8
20:55:38.89 +41:41:51.0
20:55:15.37 +41:41:22.2
20:57:25.13 +41:55:56.1
20:57:37.91 +41:58:56.6
20:56:07.05 +42:02:47.1
20:58:10.77 +42:28:39.4
22:16:03.15 +44:55:13.3
22:19:25.06 +44:51:13.3
22:15:49.53 +44:55:51.3
22:15:51.63 +44:56:13.3
22:16:45.86 +44:55:37.8
22:19:19.10 +44:52:39.4
22:17:03.89 +44:56:05.7
22:18:37.57 +44:55:40.4
22:15:50.18 +44:59:33.3
22:14:52.03 +45:01:26.9
22:17:44.94 +44:57:56.2
22:18:47.29 +44:55:33.8
22:16:46.95 +44:58:33.9
22:15:50.94 +45:01:14.9
22:15:41.47 +45:01:41.4
22:16:39.87 +45:00:05.2
22:17:55.41 +44:59:01.8
22:16:24.96 +45:01:12.4
22:19:04.35 +44:57:51.0
22:16:05.80 +45:02:12.7
22:19:18.17 +44:58:06.3
22:16:19.95 +45:03:03.1
22:19:08.95 +44:59:11.4
22:19:33.02 +44:58:22.4
22:19:39.17 +44:58:06.5
22:16:47.66 +45:02:24.0
22:16:54.53 +45:04:04.1
22:17:20.92 +45:03:21.2
22:19:33.89 +45:00:34.7
22:19:03.86 +45:01:23.1
22:18:34.42 +45:02:50.2
22:17:08.62 +45:04:57.8
22:19:28.94 +45:01:49.1
21:02:22.17 +41:02:48.4
22:17:39.58 +45:05:15.5
22:17:58.52 +45:06:01.8
22:16:04.85 +45:09:26.9
22:17:07.59 +45:08:30.6
21:02:26.39 +41:04:28.0
21:03:56.38 +41:06:07.5
20:57:26.05 +41:05:44.1
21:00:20.06 +41:11:05.9
20:55:57.25 +41:07:24.2
20:56:15.78 +41:08:56.4
20:58:39.87 +41:12:46.8
20:56:12.00 +41:09:26.8
20:58:05.81 +41:12:50.1
21:00:09.79 +41:15:21.8
20:56:13.45 +41:11:51.7
20:58:05.62 +41:16:45.6
20:55:37.91 +41:14:30.9
20:58:11.77 +41:19:28.3
20:57:14.97 +41:18:18.2
20:55:39.24 +41:16:53.8
20:57:12.63 +41:19:22.5
20:57:49.24 +41:20:12.2
20:58:50.42 +41:22:12.9
20:55:36.69 +41:18:26.2
20:57:18.20 +41:20:55.9
20:59:37.07 +41:23:51.2
20:58:05.35 +41:21:50.6
20:58:54.10 +41:23:20.7
20:55:40.61 +41:19:25.0
21:08:02.59 +41:33:52.5
20:57:52.04 +41:24:13.7
20:59:18.39 +41:25:47.8
20:57:22.47 +41:24:18.3
20:55:18.80 +41:21:47.9
20:55:19.89 +41:23:02.8
20:55:33.80 +41:23:10.8
20:55:24.79 +41:23:33.5
21:00:48.91 +41:30:11.0
21:01:49.12 +41:30:48.4
20:56:55.24 +41:25:51.6
20:57:13.03 +41:26:00.0
21:04:49.29 +41:34:45.2
20:55:50.51 +41:25:45.2
20:55:45.50 +41:25:46.6
20:55:49.47 +41:27:16.5
20:57:54.21 +41:29:55.4
20:58:36.39 +41:31:56.9
20:57:22.42 +41:31:07.2
20:57:45.49 +41:31:36.4
20:56:40.49 +41:29:56.6
20:55:36.08 +41:29:00.1
20:56:31.05 +41:30:42.7
20:58:52.65 +41:34:31.1
20:59:56.09 +41:35:19.7
20:55:08.17 +41:29:45.3
20:56:56.89 +41:32:20.4
20:59:07.64 +41:35:10.4
22:22:35.19 +49:53:48.0
20:58:09.81 +41:35:31.6
21:04:41.86 +41:42:31.5
20:58:30.53 +41:36:40.8
20:57:47.57 +41:34:46.0
20:58:36.15 +41:37:09.6
20:57:57.64 +41:36:27.6
20:56:57.52 +41:35:33.4
20:58:29.24 +41:37:09.4
20:56:29.07 +41:34:44.9
20:56:47.92 +41:35:44.9
20:56:45.10 +41:37:22.7
20:59:14.01 +41:40:39.5
20:56:07.02 +41:36:52.7
22:04:37.92 +41:49:51.5
20:56:00.82 +41:37:23.6
20:57:50.13 +41:39:32.6
20:56:28.62 +41:38:12.5
22:22:45.89 +49:07:56.0
20:55:38.01 +41:37:59.2
22:16:30.09 +49:13:41.6
20:57:14.89 +41:40:24.7
22:20:07.45 +49:05:58.0
20:59:57.93 +41:43:57.0
22:16:02.48 +49:08:31.7
22:22:00.39 +49:00:11.1
20:58:52.88 +41:42:54.9
20:56:00.95 +41:39:08.1
22:20:05.22 +48:57:52.8
22:20:46.67 +48:54:36.8
22:16:36.44 +48:58:57.5
22:16:10.06 +48:59:32.8
20:58:06.27 +41:43:25.6
22:14:28.69 +48:58:26.0
20:56:39.36 +41:41:51.3
22:16:29.09 +48:56:17.5
20:57:39.93 +41:43:10.6
22:15:30.89 +48:53:41.0
20:58:02.84 +41:43:33.4
20:57:28.30 +41:43:39.1
22:04:45.95 +41:55:14.0
20:57:22.01 +41:43:35.2
20:57:57.16 +41:45:02.9
20:56:13.24 +41:42:57.4
20:58:34.48 +41:47:17.0
22:05:02.12 +41:56:05.9
20:55:54.50 +41:43:32.9
20:54:56.93 +41:42:29.6
20:59:20.43 +41:48:03.8
20:57:20.29 +41:45:28.2
20:58:59.80 +41:47:43.1
20:58:09.01 +41:47:11.2
22:04:42.22 +41:56:40.1
22:04:21.21 +41:57:52.9
20:55:53.60 +41:44:23.8
20:58:58.13 +41:48:30.3
20:55:08.60 +41:43:07.0
20:58:03.26 +41:47:34.5
20:58:30.68 +41:48:13.2
20:59:32.64 +41:49:20.6
20:58:59.60 +41:49:02.6
22:04:41.67 +41:58:08.1
22:11:15.49 +50:23:25.0
20:55:54.55 +41:46:31.5
20:58:18.48 +41:49:25.8
20:57:38.66 +41:49:09.2
22:03:36.58 +42:00:42.4
20:55:30.14 +41:46:55.3
20:55:43.66 +41:47:36.0
20:56:55.74 +41:48:40.8
20:57:30.68 +41:49:39.4
22:05:17.26 +42:00:40.3
20:57:53.52 +41:51:09.7
20:57:27.17 +41:51:06.5
22:03:39.75 +42:03:06.8
20:57:49.40 +41:51:20.1
22:02:15.24 +42:04:09.9
22:03:16.20 +42:03:28.4
20:56:57.84 +41:50:56.1
22:03:36.22 +42:03:43.3
20:58:16.67 +41:52:25.6
21:02:52.05 +41:58:13.3
22:03:22.76 +42:04:04.9
20:55:23.39 +41:48:56.1
21:00:18.52 +41:55:39.7
20:55:52.48 +41:50:26.5
21:00:28.20 +41:55:55.9
20:59:38.56 +41:54:57.8
22:05:10.90 +42:03:02.0
20:58:22.97 +41:53:43.5
20:59:00.38 +41:54:16.0
20:58:29.51 +41:54:14.2
22:03:00.63 +42:05:24.9
20:58:40.23 +41:54:51.6
20:59:20.44 +41:55:44.3
20:56:28.25 +41:51:52.0
20:55:08.26 +41:50:37.6
20:59:12.41 +41:55:47.1
20:57:47.79 +41:54:10.7
22:03:57.63 +42:05:36.8
20:56:46.94 +41:53:07.6
22:04:08.55 +42:05:35.9
20:55:11.46 +41:51:15.8
20:56:11.15 +41:52:46.1
20:54:56.51 +41:51:13.5
22:04:06.63 +42:06:29.3
21:00:08.60 +41:58:28.7
20:58:12.68 +41:56:45.2
20:55:02.24 +41:53:13.0
22:17:39.81 +44:53:29.3
20:56:23.77 +41:54:31.7
22:04:07.37 +42:07:51.6
20:57:33.93 +41:56:54.1
20:55:28.89 +41:54:16.6
20:56:23.70 +41:55:38.1
20:58:42.80 +41:58:57.7
20:54:49.58 +41:53:51.6
22:04:04.04 +42:08:35.6
20:55:50.22 +41:55:20.1
20:58:06.79 +41:57:19.2
20:57:41.85 +41:57:59.0
20:56:48.88 +41:56:10.1
20:57:55.44 +41:58:48.0
22:03:25.35 +42:10:18.6
20:57:40.11 +41:57:04.3
20:55:54.94 +41:55:53.9
20:56:09.14 +41:56:56.9
22:02:15.09 +42:11:54.7
20:57:31.72 +41:59:11.6
22:02:05.98 +42:12:46.5
20:55:34.05 +41:56:30.8
21:00:31.35 +42:02:48.8
20:57:59.10 +42:00:04.5
22:04:00.87 +42:11:01.3
20:59:06.45 +42:01:23.2
20:56:27.78 +41:58:25.6
20:55:23.75 +41:57:15.6
21:00:30.78 +42:03:49.4
22:02:00.14 +42:13:18.8
20:58:14.62 +42:01:00.4
22:02:42.05 +42:13:03.4
20:56:36.13 +41:59:18.3
22:01:11.78 +42:14:35.7
20:57:54.05 +42:00:31.7
20:58:00.70 +42:01:11.8
20:54:54.95 +41:57:11.0
22:02:39.55 +42:13:38.8
21:00:37.22 +42:04:36.4
20:55:12.11 +41:58:00.1
20:57:01.53 +42:00:44.6
22:01:38.84 +42:14:35.6
20:59:12.48 +42:03:33.2
20:58:05.54 +42:02:32.7
20:57:14.11 +42:01:20.3
22:02:10.73 +42:15:16.6
20:58:34.61 +42:03:26.2
20:59:54.32 +42:04:51.2
20:55:22.28 +41:59:48.4
20:57:19.80 +42:02:12.1
22:02:14.46 +42:15:55.0
20:55:07.49 +41:59:27.1
20:57:49.40 +42:02:53.3
20:58:38.12 +42:05:08.8
20:58:43.11 +42:05:30.7
21:00:42.16 +42:08:09.5
20:58:47.59 +42:06:12.1
20:58:55.59 +42:06:13.4
20:58:50.88 +42:06:26.9
20:59:40.06 +42:07:32.2
20:59:28.53 +42:08:26.4
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20:55:05.67 +42:03:37.2
21:00:53.90 +42:10:19.1
20:55:03.71 +42:03:54.8
21:00:06.38 +42:10:03.6
20:56:24.99 +42:05:10.5
20:54:40.82 +42:03:30.7
20:57:35.05 +42:07:09.9
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22:19:28.79 +44:49:14.8
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Source monitoring: measuring positions from /data_ssd/NMW-TexasTech/workdir/img_2026-09-17_CI_Cyg-04-Q1b1x1_035909_TTUQ1b1x1_837614_Ls9WMewG/monitoring_positions.txt
Source monitoring: positions closer than 100 pix to a frame edge are recorded as edge
Read 54138 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 312.1982 to 336.8258 deg, Dec +39.9228 to +51.3827 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 312.1982 to 336.8258 deg, Dec 39.9228 to 51.3827 deg
Loaded 23772 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): 13969 out of 14857 total matches.
Matched with Tycho-2 14857 out of 54138 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits
Observation time (mid-exposure, UTC): JD 2461300.87329 (FITS header)
Observing site: lat= +33.748056 deg lon= -101.958333 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 324.08217 deg Dec= +46.00705 deg
Frame center: alt= +40.307 deg az= 299.838 deg airmass= 1.5428
Header cross-check: CENTALT= 40.412 deg (difference -0.106 deg)
Header cross-check: AIRMASS= 1.5405 (we compute 1.5428)
Airmass zero-point fit: REJECT_NOISY_FIT k= +0.9214 +/- 0.0720 mag/airmass N= 5099 airmass span 1.3222-1.9048 scatter 0.8192 mag
Source monitoring: airmass zero-point for wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits: REJECT_NOISY_FIT +1.854414 -0.921410 1.5428 +0.9214 5099 0.5826 0.8192 1.3222 1.9048
Edge margin: 100.0 pix (FORCED_PHOTOMETRY_EDGE_MARGIN_PIX)
Forced photometry (list mode): image=wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits list=monitoring_pixlist854387.tmp aperture=5.0
Image size: 9576 x 6388
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).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 20.719000
Forced photometry: center=(4000.17, 4598.28) aperture=5.0
Annulus: inner=10.00 outer=25.00 edge margin=100.00
Background annulus: 1649 pixels
Iterative clipping converged after 4 iterations, 1612/1649 pixels remain
SExtractor background: mode=786.53 median=786.50 mean=786.48 sigma=41.74 -> bg=786.53 (1612 pixels)
Aperture sum=25166.56 N_eff=19.6350
Net flux=9722.99 noise=184.96 SNR=52.57
Instrumental magnitude: -9.9695
Calibrated magnitude: 10.7495
Source monitoring: 1 position(s) measured on wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-57-22_20.00sec_-0.00C_LIGHTs_0010.fits (aperture 5.0 pix)
Read 52332 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 312.1221 to 336.8253 deg, Dec +39.8309 to +51.3807 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 312.1221 to 336.8253 deg, Dec 39.8309 to 51.3807 deg
Loaded 24048 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): 13822 out of 14731 total matches.
Matched with Tycho-2 14731 out of 52332 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits via Tycho-2
util/pixel_flux_airmass_correction processing wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits
Observation time (mid-exposure, UTC): JD 2461300.87383 (FITS header)
Observing site: lat= +33.748056 deg lon= -101.958333 deg east-positive (SITELAT/SITELONG FITS header keywords)
Frame center (pixel 4788.5 3194.5): RA= 324.07204 deg Dec= +46.00453 deg
Frame center: alt= +40.166 deg az= 299.865 deg airmass= 1.5472
Header cross-check: CENTALT= 40.281 deg (difference -0.115 deg)
Header cross-check: AIRMASS= 1.5446 (we compute 1.5472)
Airmass zero-point fit: REJECT_NOISY_FIT k= +0.6849 +/- 0.0710 mag/airmass N= 5228 airmass span 1.3263-1.9122 scatter 0.8266 mag
Source monitoring: airmass zero-point for wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits: REJECT_NOISY_FIT +1.481260 -0.684859 1.5472 +0.6849 5228 0.5860 0.8266 1.3263 1.9122
Edge margin: 100.0 pix (FORCED_PHOTOMETRY_EDGE_MARGIN_PIX)
Forced photometry (list mode): image=wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits list=monitoring_pixlist854387.tmp aperture=5.0
Image size: 9576 x 6388
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).
Saturation level: 57000.0
Calibration (from calib.txt_param_monitoring, fit_function=3): cal_mag = 0.000000 * x^2 + 1.000000 * x + 20.701000
Forced photometry: center=(3995.86, 4596.38) aperture=5.0
Annulus: inner=10.00 outer=25.00 edge margin=100.00
Background annulus: 1648 pixels
Iterative clipping converged after 4 iterations, 1605/1648 pixels remain
SExtractor background: mode=727.85 median=728.00 mean=728.10 sigma=44.28 -> bg=727.85 (1605 pixels)
Aperture sum=27887.93 N_eff=19.6350
Net flux=13596.62 noise=196.23 SNR=69.29
Instrumental magnitude: -10.3336
Calibrated magnitude: 10.3674
Source monitoring: 1 position(s) measured on wcs_fd_Cyg-04-Q1b1x1_2026-09-17_03-58-09_20.00sec_-0.00C_LIGHTs_0011.fits (aperture 5.0 pix)
########### Completed Cyg-04-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
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20:59:56.09 +41:35:19.7
20:58:54.10 +41:23:20.7
20:55:49.47 +41:27:16.5
20:57:14.99 +42:59:56.5
22:04:04.04 +42:08:35.6
20:55:45.50 +42:13:26.2
21:00:59.48 +42:16:48.9
21:00:31.35 +42:02:48.8
20:56:57.52 +41:35:33.4
20:59:37.07 +41:23:51.2
20:55:07.44 +42:54:33.0
22:04:06.63 +42:06:29.3
22:02:05.98 +42:12:46.5
21:01:07.05 +42:13:22.9
20:56:56.89 +41:32:20.4
20:57:49.40 +41:51:20.1
20:58:12.68 +41:56:45.2
20:59:06.45 +42:01:23.2
21:02:26.39 +41:04:28.0
20:58:16.67 +41:52:25.6
22:16:49.85 +44:53:45.0
22:16:39.87 +45:00:05.2
20:55:49.15 +42:10:30.4
20:57:47.51 +42:11:08.9
22:18:47.29 +44:55:33.8
20:57:41.47 +42:43:43.1
22:02:15.09 +42:11:54.7
20:56:40.49 +41:29:56.6
22:19:39.17 +44:58:06.5
20:58:58.13 +41:48:30.3
22:16:38.46 +44:52:58.0
22:03:36.58 +42:00:42.4
20:57:47.57 +41:34:46.0
20:56:46.73 +42:50:45.8
20:58:43.11 +42:05:30.7
20:56:27.78 +41:58:25.6
22:18:37.57 +44:55:40.4
20:59:34.26 +42:31:52.8
20:58:18.93 +42:31:21.1
22:04:45.95 +41:55:14.0
22:16:58.49 +44:53:47.8
20:56:28.25 +41:51:52.0
22:17:08.62 +45:04:57.8
20:58:29.51 +41:54:14.2
20:59:16.63 +42:15:24.9
20:58:36.15 +41:37:09.6
22:16:45.86 +44:55:37.8
20:55:56.05 +42:48:25.4
20:56:41.50 +42:23:13.5
20:57:22.42 +41:31:07.2
22:03:39.75 +42:03:06.8
20:59:00.38 +41:54:16.0
20:59:39.77 +42:13:37.8
20:59:31.38 +42:28:23.5
22:19:25.06 +44:51:13.3
20:55:53.60 +41:44:23.8
22:04:37.92 +41:49:51.5
20:57:13.03 +41:26:00.0
20:56:45.10 +41:37:22.7
20:57:45.49 +41:31:36.4
20:56:13.24 +41:42:57.4
20:58:50.42 +41:22:12.9
20:57:40.11 +41:57:04.3
20:59:07.64 +41:35:10.4
22:16:46.95 +44:58:33.9
22:01:11.78 +42:14:35.7
22:01:38.84 +42:14:35.6
20:55:23.75 +41:57:15.6
20:57:02.78 +42:06:31.1
20:56:09.14 +41:56:56.9
21:00:42.16 +42:08:09.5
22:16:31.78 +44:52:39.1
20:59:33.37 +42:10:02.5
20:59:22.47 +42:17:42.2
20:54:54.95 +41:57:11.0
22:15:41.47 +45:01:41.4
20:57:49.40 +42:02:53.3
20:57:14.11 +42:01:20.3
20:55:05.67 +42:03:37.2
20:56:15.78 +41:08:56.4
20:58:30.68 +41:48:13.2
20:58:22.97 +41:53:43.5
20:58:23.91 +42:35:14.8
20:58:05.81 +41:12:50.1
22:17:51.75 +44:46:13.2
20:57:39.93 +41:43:10.6
20:56:39.61 +42:10:22.7
20:58:40.93 +42:38:54.0
20:57:38.63 +42:25:57.3
20:54:56.38 +42:27:16.4
20:54:10.89 +42:56:21.0
22:02:42.05 +42:13:03.4
20:56:23.70 +41:55:38.1
20:59:15.00 +42:08:08.2
22:18:09.88 +44:51:41.6
20:55:36.69 +41:18:26.2
20:58:44.69 +42:19:33.4
20:55:40.61 +41:19:25.0
20:58:14.27 +42:13:28.4
20:57:26.05 +41:05:44.1
20:58:05.35 +41:21:50.6
22:16:20.00 +44:49:09.2
20:58:11.77 +41:19:28.3
20:55:27.68 +42:22:06.2
20:57:57.64 +41:36:27.6
20:58:34.61 +42:03:26.2
20:58:10.26 +42:29:24.0
20:58:59.80 +41:47:43.1
20:59:54.32 +42:04:51.2
20:55:28.89 +41:54:16.6
20:55:19.89 +41:23:02.8
20:57:22.47 +41:24:18.3
21:00:08.60 +41:58:28.7
22:19:18.17 +44:58:06.3
20:59:12.41 +41:55:47.1
20:57:53.52 +41:51:09.7
22:17:34.86 +44:11:40.0
20:58:36.39 +41:31:56.9
20:54:40.40 +42:05:49.7
20:57:28.30 +41:43:39.1
20:57:22.01 +41:43:35.2
20:55:12.97 +42:36:18.6
20:56:27.57 +42:32:59.9
20:57:59.10 +42:39:28.6
20:55:38.01 +41:37:59.2
20:58:40.76 +42:40:09.5
22:16:04.85 +45:09:26.9
20:55:25.87 +42:16:36.2
20:56:12.00 +41:09:26.8
20:55:52.48 +41:50:26.5
20:55:39.24 +41:16:53.8
20:57:51.63 +42:30:51.2
20:57:35.05 +42:07:09.9
22:19:08.95 +44:59:11.4
20:55:43.66 +41:47:36.0
20:55:34.05 +41:56:30.8
20:57:18.20 +41:20:55.9
22:02:14.46 +42:15:55.0
20:55:50.22 +41:55:20.1
20:58:06.79 +41:57:19.2
22:17:33.54 +44:44:40.8
22:22:00.39 +49:00:11.1
20:58:18.48 +41:49:25.8
22:17:23.38 +44:48:46.1
20:55:36.08 +41:29:00.1
20:56:39.36 +41:41:51.3
22:16:19.95 +45:03:03.1
20:57:41.85 +41:57:59.0
22:16:10.06 +48:59:32.8
20:56:23.77 +41:54:31.7
22:17:16.10 +44:50:48.6
20:55:52.55 +42:24:33.7
20:58:55.59 +42:06:13.4
20:55:24.79 +41:23:33.5
20:57:59.10 +42:00:04.5
22:15:56.35 +44:48:17.6
22:16:02.48 +49:08:31.7
20:58:40.23 +41:54:51.6
20:57:19.80 +42:02:12.1
20:57:27.17 +41:51:06.5
20:55:35.04 +42:19:43.9
20:56:47.92 +41:35:44.9
20:57:54.05 +42:00:31.7
22:11:15.49 +50:23:25.0
20:58:50.88 +42:06:26.9
20:57:14.89 +41:40:24.7
22:15:50.94 +45:01:14.9
20:55:08.60 +41:43:07.0
20:57:30.68 +41:49:39.4
22:14:28.69 +48:58:26.0
20:54:41.77 +42:39:36.0
20:56:04.72 +42:27:40.4
22:03:00.63 +42:05:24.9
20:56:48.88 +41:56:10.1
20:58:42.53 +42:29:45.5
20:58:49.44 +42:27:20.7
20:58:09.01 +41:47:11.2
20:56:55.74 +41:48:40.8
22:15:30.89 +48:53:41.0
21:00:31.81 +42:23:51.2
20:55:08.17 +41:29:45.3
22:20:07.45 +49:05:58.0
20:59:57.93 +41:43:57.0
20:59:20.43 +41:48:03.8
22:05:10.90 +42:03:02.0
22:17:26.71 +44:51:59.7
21:02:22.17 +41:02:48.4
22:02:10.73 +42:15:16.6
20:56:31.29 +42:22:22.9
20:56:29.07 +41:34:44.9
22:17:58.52 +45:06:01.8
20:58:14.62 +42:01:00.4
22:04:21.21 +41:57:52.9
22:18:12.34 +44:15:00.6
22:16:05.80 +45:02:12.7
22:17:55.41 +44:59:01.8
20:55:42.76 +42:10:08.9
20:57:14.97 +41:18:18.2
22:16:21.27 +44:53:24.2
20:56:07.02 +41:36:52.7
20:56:31.82 +42:27:20.9
22:03:22.76 +42:04:04.9
22:02:43.35 +42:16:39.4
20:55:18.80 +41:21:47.9
22:17:04.89 +44:29:51.5
22:02:39.55 +42:13:38.8
22:15:49.53 +44:55:51.3
22:19:04.35 +44:57:51.0
20:55:45.50 +41:25:46.6
22:15:51.63 +44:56:13.3
22:17:15.59 +44:14:54.1
20:58:38.12 +42:05:08.8
20:58:52.88 +41:42:54.9
20:55:30.14 +41:46:55.3
22:04:41.67 +41:58:08.1
22:15:51.51 +44:54:15.5
22:16:24.96 +45:01:12.4
22:16:30.09 +49:13:41.6
22:05:17.26 +42:00:40.3
20:55:50.51 +41:25:45.2
20:56:12.50 +42:07:04.6
20:57:33.93 +41:56:54.1
21:00:28.20 +41:55:55.9
22:14:52.03 +45:01:26.9
22:22:45.89 +49:07:56.0
20:58:34.48 +41:47:17.0
22:03:16.20 +42:03:28.4
22:17:39.58 +45:05:15.5
22:16:54.53 +45:04:04.1
20:59:32.64 +41:49:20.6
20:59:00.06 +42:17:21.6
20:57:31.72 +41:59:11.6
22:15:50.18 +44:59:33.3
20:55:08.26 +41:50:37.6
22:17:23.94 +44:50:07.2
21:02:52.05 +41:58:13.3
20:55:11.46 +41:51:15.8
20:58:33.80 +42:24:01.0
20:58:03.26 +41:47:34.5
22:20:05.22 +48:57:52.8
22:16:47.66 +45:02:24.0
20:58:30.43 +42:28:43.7
20:59:28.53 +42:08:26.4
20:56:57.84 +41:50:56.1
22:20:46.67 +48:54:36.8
22:19:33.02 +44:58:22.4
20:59:20.44 +41:55:44.3
21:03:56.38 +41:06:07.5
20:55:10.53 +42:17:24.8
20:57:45.60 +42:29:05.7
20:58:29.24 +41:37:09.4
20:55:23.39 +41:48:56.1
20:58:09.17 +42:30:29.3
20:58:59.60 +41:49:02.6
22:18:34.42 +45:02:50.2
21:00:17.17 +42:26:32.0
20:59:38.56 +41:54:57.8
21:08:02.59 +41:33:52.5
20:55:54.55 +41:46:31.5
22:22:35.19 +49:53:48.0
###################################################################################
20:57:37.91 +41:58:56.6 -- not an asteroid (will add it to exclusion list)
20:55:02.87 +41:31:54.4 -- not an asteroid (will add it to exclusion list)
20:55:15.37 +41:41:22.2 -- not an asteroid (will add it to exclusion list)
20:55:38.89 +41:41:51.0 -- not an asteroid (will add it to exclusion list)
20:56:07.05 +42:02:47.1 -- not an asteroid (will add it to exclusion list)
20:55:47.89 +41:37:34.8 -- not an asteroid (will add it to exclusion list)
20:58:10.77 +42:28:39.4 -- not an asteroid (will add it to exclusion list)
20:57:25.13 +41:55:56.1 -- not an asteroid (will add it to exclusion list)
20:55:28.11 +41:17:39.5 -- not an asteroid (will add it to exclusion list)
20:55:34.56 +41:36:48.0 -- not an asteroid (will add it to exclusion list)
20:56:00.95 +41:39:08.1 -- not an asteroid (will add it to exclusion list)
20:58:47.59 +42:06:12.1 -- not an asteroid (will add it to exclusion list)
22:16:36.44 +48:58:57.5 -- not an asteroid (will add it to exclusion list)
20:54:56.51 +41:51:13.5 -- not an asteroid (will add it to exclusion list)
20:57:47.79 +41:54:10.7 -- not an asteroid (will add it to exclusion list)
20:56:13.45 +41:11:51.7 -- not an asteroid (will add it to exclusion list)
20:57:20.29 +41:45:28.2 -- not an asteroid (will add it to exclusion list)
20:56:24.99 +42:05:10.5 -- not an asteroid (will add it to exclusion list)
22:03:57.63 +42:05:36.8 -- not an asteroid (will add it to exclusion list)
20:58:02.84 +41:43:33.4 -- not an asteroid (will add it to exclusion list)
20:54:06.44 +42:55:11.7 -- not an asteroid (will add it to exclusion list)
20:56:00.61 +42:27:51.7 -- not an asteroid (will add it to exclusion list)
21:00:30.78 +42:03:49.4 -- not an asteroid (will add it to exclusion list)
20:57:50.13 +41:39:32.6 -- not an asteroid (will add it to exclusion list)
20:57:54.21 +41:29:55.4 -- not an asteroid (will add it to exclusion list)
20:57:57.16 +41:45:02.9 -- not an asteroid (will add it to exclusion list)
20:54:53.52 +42:23:51.1 -- not an asteroid (will add it to exclusion list)
20:58:42.80 +41:58:57.7 -- not an asteroid (will add it to exclusion list)
20:56:36.13 +41:59:18.3 -- not an asteroid (will add it to exclusion list)
20:54:57.53 +42:14:38.4 -- not an asteroid (will add it to exclusion list)
20:54:56.93 +41:42:29.6 -- not an asteroid (will add it to exclusion list)
20:58:15.98 +42:09:49.5 -- not an asteroid (will add it to exclusion list)
21:00:53.90 +42:10:19.1 -- not an asteroid (will add it to exclusion list)
21:01:49.12 +41:30:48.4 -- not an asteroid (will add it to exclusion list)
20:58:06.85 +42:34:52.3 -- not an asteroid (will add it to exclusion list)
20:58:30.53 +41:36:40.8 -- not an asteroid (will add it to exclusion list)
20:55:07.49 +41:59:27.1 -- not an asteroid (will add it to exclusion list)
20:59:12.48 +42:03:33.2 -- not an asteroid (will add it to exclusion list)
20:59:36.46 +42:27:28.7 -- not an asteroid (will add it to exclusion list)
20:59:40.06 +42:07:32.2 -- not an asteroid (will add it to exclusion list)
20:57:12.63 +41:19:22.5 -- not an asteroid (will add it to exclusion list)
21:00:09.14 +42:24:01.6 -- not an asteroid (will add it to exclusion list)
20:56:45.71 +42:49:04.9 -- not an asteroid (will add it to exclusion list)
22:16:29.09 +48:56:17.5 -- not an asteroid (will add it to exclusion list)
20:55:08.53 +42:47:47.7 -- not an asteroid (will add it to exclusion list)
20:56:18.03 +42:26:25.4 -- not an asteroid (will add it to exclusion list)
20:54:56.22 +42:06:30.3 -- not an asteroid (will add it to exclusion list)
20:58:09.81 +41:35:31.6 -- not an asteroid (will add it to exclusion list)
20:59:54.48 +42:17:01.5 -- not an asteroid (will add it to exclusion list)
22:15:24.17 +44:54:45.4 -- not an asteroid (will add it to exclusion list)
20:54:28.06 +42:37:09.9 -- not an asteroid (will add it to exclusion list)
20:59:52.64 +42:13:39.7 -- not an asteroid (will add it to exclusion list)
20:59:18.39 +41:25:47.8 -- not an asteroid (will add it to exclusion list)
20:54:49.58 +41:53:51.6 -- not an asteroid (will add it to exclusion list)
21:00:48.42 +42:19:23.1 -- not an asteroid (will add it to exclusion list)
20:58:52.65 +41:34:31.1 -- not an asteroid (will add it to exclusion list)
20:56:00.82 +41:37:23.6 -- not an asteroid (will add it to exclusion list)
20:59:14.01 +41:40:39.5 -- not an asteroid (will add it to exclusion list)
21:00:18.52 +41:55:39.7 -- not an asteroid (will add it to exclusion list)
21:04:49.29 +41:34:45.2 -- not an asteroid (will add it to exclusion list)
20:55:43.24 +42:45:59.4 -- not an asteroid (will add it to exclusion list)
20:56:33.34 +42:14:09.4 -- not an asteroid (will add it to exclusion list)
20:58:39.87 +41:12:46.8 -- not an asteroid (will add it to exclusion list)
22:19:28.94 +45:01:49.1 -- not an asteroid (will add it to exclusion list)
20:56:46.94 +41:53:07.6 -- not an asteroid (will add it to exclusion list)
20:55:02.24 +41:53:13.0 -- not an asteroid (will add it to exclusion list)
22:17:52.11 +44:17:05.3 -- not an asteroid (will add it to exclusion list)
22:19:19.10 +44:52:39.4 -- not an asteroid (will add it to exclusion list)
20:56:32.08 +42:12:05.9 -- not an asteroid (will add it to exclusion list)
22:03:25.35 +42:10:18.6 -- not an asteroid (will add it to exclusion list)
20:59:06.17 +42:38:30.9 -- not an asteroid (will add it to exclusion list)
20:58:05.62 +41:16:45.6 -- not an asteroid (will add it to exclusion list)
20:56:28.62 +41:38:12.5 -- not an asteroid (will add it to exclusion list)
20:55:54.50 +41:43:32.9 -- not an asteroid (will add it to exclusion list)
20:57:38.66 +41:49:09.2 -- not an asteroid (will add it to exclusion list)
20:57:55.44 +41:58:48.0 -- not an asteroid (will add it to exclusion list)
22:17:39.81 +44:53:29.3 -- not an asteroid (will add it to exclusion list)
20:54:55.65 +43:02:37.1 -- not an asteroid (will add it to exclusion list)
20:55:03.71 +42:03:54.8 -- not an asteroid (will add it to exclusion list)
20:56:11.15 +41:52:46.1 -- not an asteroid (will add it to exclusion list)
20:59:34.34 +42:32:30.0 -- not an asteroid (will add it to exclusion list)
20:55:33.80 +41:23:10.8 -- not an asteroid (will add it to exclusion list)
22:19:03.86 +45:01:23.1 -- not an asteroid (will add it to exclusion list)
21:00:09.79 +41:15:21.8 -- not an asteroid (will add it to exclusion list)
22:19:33.89 +45:00:34.7 -- not an asteroid (will add it to exclusion list)
20:54:26.88 +42:48:48.8 -- not an asteroid (will add it to exclusion list)
20:58:06.27 +41:43:25.6 -- not an asteroid (will add it to exclusion list)
22:04:00.87 +42:11:01.3 -- not an asteroid (will add it to exclusion list)
20:55:37.91 +41:14:30.9 -- not an asteroid (will add it to exclusion list)
21:00:37.22 +42:04:36.4 -- not an asteroid (will add it to exclusion list)
20:56:55.24 +41:25:51.6 -- not an asteroid (will add it to exclusion list)
22:04:08.55 +42:05:35.9 -- not an asteroid (will add it to exclusion list)
21:01:34.59 +42:35:32.2 -- not an asteroid (will add it to exclusion list)
20:55:54.94 +41:55:53.9 -- not an asteroid (will add it to exclusion list)
20:59:08.34 +42:33:13.3 -- not an asteroid (will add it to exclusion list)
20:54:42.67 +42:35:24.6 -- not an asteroid (will add it to exclusion list)
20:57:49.24 +41:20:12.2 -- not an asteroid (will add it to exclusion list)
20:55:22.28 +41:59:48.4 -- not an asteroid (will add it to exclusion list)
20:55:03.80 +42:22:40.6 -- not an asteroid (will add it to exclusion list)
22:02:15.24 +42:04:09.9 -- not an asteroid (will add it to exclusion list)
22:16:03.15 +44:55:13.3 -- not an asteroid (will add it to exclusion list)
20:58:00.70 +42:01:11.8 -- not an asteroid (will add it to exclusion list)
20:58:35.06 +42:11:54.0 -- not an asteroid (will add it to exclusion list)
20:58:30.99 +42:19:45.7 -- not an asteroid (will add it to exclusion list)
21:00:48.91 +41:30:11.0 -- not an asteroid (will add it to exclusion list)
21:00:21.34 +42:35:11.4 -- not an asteroid (will add it to exclusion list)
22:14:44.34 +44:56:23.1 -- not an asteroid (will add it to exclusion list)
22:04:07.37 +42:07:51.6 -- not an asteroid (will add it to exclusion list)
22:19:28.79 +44:49:14.8 -- not an asteroid (will add it to exclusion list)
20:55:22.31 +42:18:43.0 -- not an asteroid (will add it to exclusion list)
22:17:07.59 +45:08:30.6 -- not an asteroid (will add it to exclusion list)
21:00:06.38 +42:10:03.6 -- not an asteroid (will add it to exclusion list)
20:56:14.98 +42:06:14.1 -- not an asteroid (will add it to exclusion list)
22:17:20.92 +45:03:21.2 -- not an asteroid (will add it to exclusion list)
20:56:04.61 +42:43:29.8 -- not an asteroid (will add it to exclusion list)
21:00:20.06 +41:11:05.9 -- not an asteroid (will add it to exclusion list)
20:58:02.99 +42:28:18.1 -- not an asteroid (will add it to exclusion list)
22:17:03.89 +44:56:05.7 -- not an asteroid (will add it to exclusion list)
21:00:01.86 +42:20:43.6 -- not an asteroid (will add it to exclusion list)
21:04:41.86 +41:42:31.5 -- not an asteroid (will add it to exclusion list)
20:58:05.54 +42:02:32.7 -- not an asteroid (will add it to exclusion list)
22:02:00.14 +42:13:18.8 -- not an asteroid (will add it to exclusion list)
20:55:57.25 +41:07:24.2 -- not an asteroid (will add it to exclusion list)
22:17:44.94 +44:57:56.2 -- not an asteroid (will add it to exclusion list)
20:55:12.11 +41:58:00.1 -- not an asteroid (will add it to exclusion list)
20:54:40.82 +42:03:30.7 -- not an asteroid (will add it to exclusion list)
20:57:01.53 +42:00:44.6 -- not an asteroid (will add it to exclusion list)
20:57:52.04 +41:24:13.7 -- not an asteroid (will add it to exclusion list)
22:04:42.22 +41:56:40.1 -- not an asteroid (will add it to exclusion list)
20:56:31.05 +41:30:42.7 -- not an asteroid (will add it to exclusion list)
22:05:02.12 +41:56:05.9 -- not an asteroid (will add it to exclusion list)
20:55:00.46 +42:08:23.8 -- not an asteroid (will add it to exclusion list)
22:03:36.22 +42:03:43.3 -- not an asteroid (will add it to exclusion list)
20:59:56.09 +41:35:19.7 -- not an asteroid (will add it to exclusion list)
20:58:54.10 +41:23:20.7 -- not an asteroid (will add it to exclusion list)
20:55:49.47 +41:27:16.5 -- not an asteroid (will add it to exclusion list)
20:57:14.99 +42:59:56.5 -- not an asteroid (will add it to exclusion list)
22:04:04.04 +42:08:35.6 -- not an asteroid (will add it to exclusion list)
20:55:45.50 +42:13:26.2 -- not an asteroid (will add it to exclusion list)
21:00:59.48 +42:16:48.9 -- not an asteroid (will add it to exclusion list)
21:00:31.35 +42:02:48.8 -- not an asteroid (will add it to exclusion list)
20:56:57.52 +41:35:33.4 -- not an asteroid (will add it to exclusion list)
20:59:37.07 +41:23:51.2 -- not an asteroid (will add it to exclusion list)
20:55:07.44 +42:54:33.0 -- not an asteroid (will add it to exclusion list)
22:04:06.63 +42:06:29.3 -- not an asteroid (will add it to exclusion list)
22:02:05.98 +42:12:46.5 -- not an asteroid (will add it to exclusion list)
21:01:07.05 +42:13:22.9 -- not an asteroid (will add it to exclusion list)
20:56:56.89 +41:32:20.4 -- not an asteroid (will add it to exclusion list)
20:57:49.40 +41:51:20.1 -- not an asteroid (will add it to exclusion list)
20:58:12.68 +41:56:45.2 -- not an asteroid (will add it to exclusion list)
20:59:06.45 +42:01:23.2 -- not an asteroid (will add it to exclusion list)
21:02:26.39 +41:04:28.0 -- not an asteroid (will add it to exclusion list)
20:58:16.67 +41:52:25.6 -- not an asteroid (will add it to exclusion list)
22:16:49.85 +44:53:45.0 -- not an asteroid (will add it to exclusion list)
22:16:39.87 +45:00:05.2 -- not an asteroid (will add it to exclusion list)
20:55:49.15 +42:10:30.4 -- not an asteroid (will add it to exclusion list)
20:57:47.51 +42:11:08.9 -- not an asteroid (will add it to exclusion list)
22:18:47.29 +44:55:33.8 -- not an asteroid (will add it to exclusion list)
20:57:41.47 +42:43:43.1 -- not an asteroid (will add it to exclusion list)
22:02:15.09 +42:11:54.7 -- not an asteroid (will add it to exclusion list)
20:56:40.49 +41:29:56.6 -- not an asteroid (will add it to exclusion list)
22:19:39.17 +44:58:06.5 -- not an asteroid (will add it to exclusion list)
20:58:58.13 +41:48:30.3 -- not an asteroid (will add it to exclusion list)
22:16:38.46 +44:52:58.0 -- not an asteroid (will add it to exclusion list)
22:03:36.58 +42:00:42.4 -- not an asteroid (will add it to exclusion list)
20:57:47.57 +41:34:46.0 -- not an asteroid (will add it to exclusion list)
20:56:46.73 +42:50:45.8 -- not an asteroid (will add it to exclusion list)
20:58:43.11 +42:05:30.7 -- not an asteroid (will add it to exclusion list)
20:56:27.78 +41:58:25.6 -- not an asteroid (will add it to exclusion list)
22:18:37.57 +44:55:40.4 -- not an asteroid (will add it to exclusion list)
20:59:34.26 +42:31:52.8 -- not an asteroid (will add it to exclusion list)
20:58:18.93 +42:31:21.1 -- not an asteroid (will add it to exclusion list)
22:04:45.95 +41:55:14.0 -- not an asteroid (will add it to exclusion list)
22:16:58.49 +44:53:47.8 -- not an asteroid (will add it to exclusion list)
20:56:28.25 +41:51:52.0 -- not an asteroid (will add it to exclusion list)
22:17:08.62 +45:04:57.8 -- not an asteroid (will add it to exclusion list)
20:58:29.51 +41:54:14.2 -- not an asteroid (will add it to exclusion list)
20:59:16.63 +42:15:24.9 -- not an asteroid (will add it to exclusion list)
20:58:36.15 +41:37:09.6 -- not an asteroid (will add it to exclusion list)
22:16:45.86 +44:55:37.8 -- not an asteroid (will add it to exclusion list)
20:55:56.05 +42:48:25.4 -- not an asteroid (will add it to exclusion list)
20:56:41.50 +42:23:13.5 -- not an asteroid (will add it to exclusion list)
20:57:22.42 +41:31:07.2 -- not an asteroid (will add it to exclusion list)
22:03:39.75 +42:03:06.8 -- not an asteroid (will add it to exclusion list)
20:59:00.38 +41:54:16.0 -- not an asteroid (will add it to exclusion list)
20:59:39.77 +42:13:37.8 -- not an asteroid (will add it to exclusion list)
20:59:31.38 +42:28:23.5 -- not an asteroid (will add it to exclusion list)
22:19:25.06 +44:51:13.3 -- not an asteroid (will add it to exclusion list)
20:55:53.60 +41:44:23.8 -- not an asteroid (will add it to exclusion list)
22:04:37.92 +41:49:51.5 -- not an asteroid (will add it to exclusion list)
20:57:13.03 +41:26:00.0 -- not an asteroid (will add it to exclusion list)
20:56:45.10 +41:37:22.7 -- not an asteroid (will add it to exclusion list)
20:57:45.49 +41:31:36.4 -- not an asteroid (will add it to exclusion list)
20:56:13.24 +41:42:57.4 -- not an asteroid (will add it to exclusion list)
20:58:50.42 +41:22:12.9 -- not an asteroid (will add it to exclusion list)
20:57:40.11 +41:57:04.3 -- not an asteroid (will add it to exclusion list)
20:59:07.64 +41:35:10.4 -- not an asteroid (will add it to exclusion list)
22:16:46.95 +44:58:33.9 -- not an asteroid (will add it to exclusion list)
22:01:11.78 +42:14:35.7 -- not an asteroid (will add it to exclusion list)
22:01:38.84 +42:14:35.6 -- not an asteroid (will add it to exclusion list)
20:55:23.75 +41:57:15.6 -- not an asteroid (will add it to exclusion list)
20:57:02.78 +42:06:31.1 -- not an asteroid (will add it to exclusion list)
20:56:09.14 +41:56:56.9 -- not an asteroid (will add it to exclusion list)
21:00:42.16 +42:08:09.5 -- not an asteroid (will add it to exclusion list)
22:16:31.78 +44:52:39.1 -- not an asteroid (will add it to exclusion list)
20:59:33.37 +42:10:02.5 -- not an asteroid (will add it to exclusion list)
20:59:22.47 +42:17:42.2 -- not an asteroid (will add it to exclusion list)
20:54:54.95 +41:57:11.0 -- not an asteroid (will add it to exclusion list)
22:15:41.47 +45:01:41.4 -- not an asteroid (will add it to exclusion list)
20:57:49.40 +42:02:53.3 -- not an asteroid (will add it to exclusion list)
20:57:14.11 +42:01:20.3 -- not an asteroid (will add it to exclusion list)
20:55:05.67 +42:03:37.2 -- not an asteroid (will add it to exclusion list)
20:56:15.78 +41:08:56.4 -- not an asteroid (will add it to exclusion list)
20:58:30.68 +41:48:13.2 -- not an asteroid (will add it to exclusion list)
20:58:22.97 +41:53:43.5 -- not an asteroid (will add it to exclusion list)
20:58:23.91 +42:35:14.8 -- not an asteroid (will add it to exclusion list)
20:58:05.81 +41:12:50.1 -- not an asteroid (will add it to exclusion list)
22:17:51.75 +44:46:13.2 -- not an asteroid (will add it to exclusion list)
20:57:39.93 +41:43:10.6 -- not an asteroid (will add it to exclusion list)
20:56:39.61 +42:10:22.7 -- not an asteroid (will add it to exclusion list)
20:58:40.93 +42:38:54.0 -- not an asteroid (will add it to exclusion list)
20:57:38.63 +42:25:57.3 -- not an asteroid (will add it to exclusion list)
20:54:56.38 +42:27:16.4 -- not an asteroid (will add it to exclusion list)
20:54:10.89 +42:56:21.0 -- not an asteroid (will add it to exclusion list)
22:02:42.05 +42:13:03.4 -- not an asteroid (will add it to exclusion list)
20:56:23.70 +41:55:38.1 -- not an asteroid (will add it to exclusion list)
20:59:15.00 +42:08:08.2 -- not an asteroid (will add it to exclusion list)
22:18:09.88 +44:51:41.6 -- not an asteroid (will add it to exclusion list)
20:55:36.69 +41:18:26.2 -- not an asteroid (will add it to exclusion list)
20:58:44.69 +42:19:33.4 -- not an asteroid (will add it to exclusion list)
20:55:40.61 +41:19:25.0 -- not an asteroid (will add it to exclusion list)
20:58:14.27 +42:13:28.4 -- not an asteroid (will add it to exclusion list)
20:57:26.05 +41:05:44.1 -- not an asteroid (will add it to exclusion list)
20:58:05.35 +41:21:50.6 -- not an asteroid (will add it to exclusion list)
22:16:20.00 +44:49:09.2 -- not an asteroid (will add it to exclusion list)
20:58:11.77 +41:19:28.3 -- not an asteroid (will add it to exclusion list)
20:55:27.68 +42:22:06.2 -- not an asteroid (will add it to exclusion list)
20:57:57.64 +41:36:27.6 -- not an asteroid (will add it to exclusion list)
20:58:34.61 +42:03:26.2 -- not an asteroid (will add it to exclusion list)
20:58:10.26 +42:29:24.0 -- not an asteroid (will add it to exclusion list)
20:58:59.80 +41:47:43.1 -- not an asteroid (will add it to exclusion list)
20:59:54.32 +42:04:51.2 -- not an asteroid (will add it to exclusion list)
20:55:28.89 +41:54:16.6 -- not an asteroid (will add it to exclusion list)
20:55:19.89 +41:23:02.8 -- not an asteroid (will add it to exclusion list)
20:57:22.47 +41:24:18.3 -- not an asteroid (will add it to exclusion list)
21:00:08.60 +41:58:28.7 -- not an asteroid (will add it to exclusion list)
22:19:18.17 +44:58:06.3 -- not an asteroid (will add it to exclusion list)
20:59:12.41 +41:55:47.1 -- not an asteroid (will add it to exclusion list)
20:57:53.52 +41:51:09.7 -- not an asteroid (will add it to exclusion list)
22:17:34.86 +44:11:40.0 -- not an asteroid (will add it to exclusion list)
20:58:36.39 +41:31:56.9 -- not an asteroid (will add it to exclusion list)
20:54:40.40 +42:05:49.7 -- not an asteroid (will add it to exclusion list)
20:57:28.30 +41:43:39.1 -- not an asteroid (will add it to exclusion list)
20:57:22.01 +41:43:35.2 -- not an asteroid (will add it to exclusion list)
20:55:12.97 +42:36:18.6 -- not an asteroid (will add it to exclusion list)
20:56:27.57 +42:32:59.9 -- not an asteroid (will add it to exclusion list)
20:57:59.10 +42:39:28.6 -- not an asteroid (will add it to exclusion list)
20:55:38.01 +41:37:59.2 -- not an asteroid (will add it to exclusion list)
20:58:40.76 +42:40:09.5 -- not an asteroid (will add it to exclusion list)
22:16:04.85 +45:09:26.9 -- not an asteroid (will add it to exclusion list)
20:55:25.87 +42:16:36.2 -- not an asteroid (will add it to exclusion list)
20:56:12.00 +41:09:26.8 -- not an asteroid (will add it to exclusion list)
20:55:52.48 +41:50:26.5 -- not an asteroid (will add it to exclusion list)
20:55:39.24 +41:16:53.8 -- not an asteroid (will add it to exclusion list)
20:57:51.63 +42:30:51.2 -- not an asteroid (will add it to exclusion list)
20:57:35.05 +42:07:09.9 -- not an asteroid (will add it to exclusion list)
22:19:08.95 +44:59:11.4 -- not an asteroid (will add it to exclusion list)
20:55:43.66 +41:47:36.0 -- not an asteroid (will add it to exclusion list)
20:55:34.05 +41:56:30.8 -- not an asteroid (will add it to exclusion list)
20:57:18.20 +41:20:55.9 -- not an asteroid (will add it to exclusion list)
22:02:14.46 +42:15:55.0 -- not an asteroid (will add it to exclusion list)
20:55:50.22 +41:55:20.1 -- not an asteroid (will add it to exclusion list)
20:58:06.79 +41:57:19.2 -- not an asteroid (will add it to exclusion list)
22:17:33.54 +44:44:40.8 -- not an asteroid (will add it to exclusion list)
22:22:00.39 +49:00:11.1 -- not an asteroid (will add it to exclusion list)
20:58:18.48 +41:49:25.8 -- not an asteroid (will add it to exclusion list)
22:17:23.38 +44:48:46.1 -- not an asteroid (will add it to exclusion list)
20:55:36.08 +41:29:00.1 -- not an asteroid (will add it to exclusion list)
20:56:39.36 +41:41:51.3 -- not an asteroid (will add it to exclusion list)
22:16:19.95 +45:03:03.1 -- not an asteroid (will add it to exclusion list)
20:57:41.85 +41:57:59.0 -- not an asteroid (will add it to exclusion list)
22:16:10.06 +48:59:32.8 -- not an asteroid (will add it to exclusion list)
20:56:23.77 +41:54:31.7 -- not an asteroid (will add it to exclusion list)
22:17:16.10 +44:50:48.6 -- not an asteroid (will add it to exclusion list)
20:55:52.55 +42:24:33.7 -- not an asteroid (will add it to exclusion list)
20:58:55.59 +42:06:13.4 -- not an asteroid (will add it to exclusion list)
20:55:24.79 +41:23:33.5 -- not an asteroid (will add it to exclusion list)
20:57:59.10 +42:00:04.5 -- not an asteroid (will add it to exclusion list)
22:15:56.35 +44:48:17.6 -- not an asteroid (will add it to exclusion list)
22:16:02.48 +49:08:31.7 -- not an asteroid (will add it to exclusion list)
20:58:40.23 +41:54:51.6 -- not an asteroid (will add it to exclusion list)
20:57:19.80 +42:02:12.1 -- not an asteroid (will add it to exclusion list)
20:57:27.17 +41:51:06.5 -- not an asteroid (will add it to exclusion list)
20:55:35.04 +42:19:43.9 -- not an asteroid (will add it to exclusion list)
20:56:47.92 +41:35:44.9 -- not an asteroid (will add it to exclusion list)
20:57:54.05 +42:00:31.7 -- not an asteroid (will add it to exclusion list)
22:11:15.49 +50:23:25.0 -- not an asteroid (will add it to exclusion list)
20:58:50.88 +42:06:26.9 -- not an asteroid (will add it to exclusion list)
20:57:14.89 +41:40:24.7 -- not an asteroid (will add it to exclusion list)
22:15:50.94 +45:01:14.9 -- not an asteroid (will add it to exclusion list)
20:55:08.60 +41:43:07.0 -- not an asteroid (will add it to exclusion list)
20:57:30.68 +41:49:39.4 -- not an asteroid (will add it to exclusion list)
22:14:28.69 +48:58:26.0 -- not an asteroid (will add it to exclusion list)
20:54:41.77 +42:39:36.0 -- not an asteroid (will add it to exclusion list)
20:56:04.72 +42:27:40.4 -- not an asteroid (will add it to exclusion list)
22:03:00.63 +42:05:24.9 -- not an asteroid (will add it to exclusion list)
20:56:48.88 +41:56:10.1 -- not an asteroid (will add it to exclusion list)
20:58:42.53 +42:29:45.5 -- not an asteroid (will add it to exclusion list)
20:58:49.44 +42:27:20.7 -- not an asteroid (will add it to exclusion list)
20:58:09.01 +41:47:11.2 -- not an asteroid (will add it to exclusion list)
20:56:55.74 +41:48:40.8 -- not an asteroid (will add it to exclusion list)
22:15:30.89 +48:53:41.0 -- not an asteroid (will add it to exclusion list)
21:00:31.81 +42:23:51.2 -- not an asteroid (will add it to exclusion list)
20:55:08.17 +41:29:45.3 -- not an asteroid (will add it to exclusion list)
22:20:07.45 +49:05:58.0 -- not an asteroid (will add it to exclusion list)
20:59:57.93 +41:43:57.0 -- not an asteroid (will add it to exclusion list)
20:59:20.43 +41:48:03.8 -- not an asteroid (will add it to exclusion list)
22:05:10.90 +42:03:02.0 -- not an asteroid (will add it to exclusion list)
22:17:26.71 +44:51:59.7 -- not an asteroid (will add it to exclusion list)
21:02:22.17 +41:02:48.4 -- not an asteroid (will add it to exclusion list)
22:02:10.73 +42:15:16.6 -- not an asteroid (will add it to exclusion list)
20:56:31.29 +42:22:22.9 -- not an asteroid (will add it to exclusion list)
20:56:29.07 +41:34:44.9 -- not an asteroid (will add it to exclusion list)
22:17:58.52 +45:06:01.8 -- not an asteroid (will add it to exclusion list)
20:58:14.62 +42:01:00.4 -- not an asteroid (will add it to exclusion list)
22:04:21.21 +41:57:52.9 -- not an asteroid (will add it to exclusion list)
22:18:12.34 +44:15:00.6 -- not an asteroid (will add it to exclusion list)
22:16:05.80 +45:02:12.7 -- not an asteroid (will add it to exclusion list)
22:17:55.41 +44:59:01.8 -- not an asteroid (will add it to exclusion list)
20:55:42.76 +42:10:08.9 -- not an asteroid (will add it to exclusion list)
20:57:14.97 +41:18:18.2 -- not an asteroid (will add it to exclusion list)
22:16:21.27 +44:53:24.2 -- not an asteroid (will add it to exclusion list)
20:56:07.02 +41:36:52.7 -- not an asteroid (will add it to exclusion list)
20:56:31.82 +42:27:20.9 -- not an asteroid (will add it to exclusion list)
22:03:22.76 +42:04:04.9 -- not an asteroid (will add it to exclusion list)
22:02:43.35 +42:16:39.4 -- listed in neverexclude_list.txt (will NOT add it to exclusion list)
20:55:18.80 +41:21:47.9 -- not an asteroid (will add it to exclusion list)
22:17:04.89 +44:29:51.5 -- not an asteroid (will add it to exclusion list)
22:02:39.55 +42:13:38.8 -- not an asteroid (will add it to exclusion list)
22:15:49.53 +44:55:51.3 -- not an asteroid (will add it to exclusion list)
22:19:04.35 +44:57:51.0 -- not an asteroid (will add it to exclusion list)
20:55:45.50 +41:25:46.6 -- not an asteroid (will add it to exclusion list)
22:15:51.63 +44:56:13.3 -- not an asteroid (will add it to exclusion list)
22:17:15.59 +44:14:54.1 -- not an asteroid (will add it to exclusion list)
20:58:38.12 +42:05:08.8 -- not an asteroid (will add it to exclusion list)
20:58:52.88 +41:42:54.9 -- not an asteroid (will add it to exclusion list)
20:55:30.14 +41:46:55.3 -- not an asteroid (will add it to exclusion list)
22:04:41.67 +41:58:08.1 -- not an asteroid (will add it to exclusion list)
22:15:51.51 +44:54:15.5 -- not an asteroid (will add it to exclusion list)
22:16:24.96 +45:01:12.4 -- not an asteroid (will add it to exclusion list)
22:16:30.09 +49:13:41.6 -- not an asteroid (will add it to exclusion list)
22:05:17.26 +42:00:40.3 -- not an asteroid (will add it to exclusion list)
20:55:50.51 +41:25:45.2 -- not an asteroid (will add it to exclusion list)
20:56:12.50 +42:07:04.6 -- not an asteroid (will add it to exclusion list)
20:57:33.93 +41:56:54.1 -- not an asteroid (will add it to exclusion list)
21:00:28.20 +41:55:55.9 -- not an asteroid (will add it to exclusion list)
22:14:52.03 +45:01:26.9 -- not an asteroid (will add it to exclusion list)
22:22:45.89 +49:07:56.0 -- not an asteroid (will add it to exclusion list)
20:58:34.48 +41:47:17.0 -- not an asteroid (will add it to exclusion list)
22:03:16.20 +42:03:28.4 -- not an asteroid (will add it to exclusion list)
22:17:39.58 +45:05:15.5 -- not an asteroid (will add it to exclusion list)
22:16:54.53 +45:04:04.1 -- not an asteroid (will add it to exclusion list)
20:59:32.64 +41:49:20.6 -- not an asteroid (will add it to exclusion list)
20:59:00.06 +42:17:21.6 -- not an asteroid (will add it to exclusion list)
20:57:31.72 +41:59:11.6 -- not an asteroid (will add it to exclusion list)
22:15:50.18 +44:59:33.3 -- not an asteroid (will add it to exclusion list)
20:55:08.26 +41:50:37.6 -- not an asteroid (will add it to exclusion list)
22:17:23.94 +44:50:07.2 -- not an asteroid (will add it to exclusion list)
21:02:52.05 +41:58:13.3 -- not an asteroid (will add it to exclusion list)
20:55:11.46 +41:51:15.8 -- not an asteroid (will add it to exclusion list)
20:58:33.80 +42:24:01.0 -- not an asteroid (will add it to exclusion list)
20:58:03.26 +41:47:34.5 -- not an asteroid (will add it to exclusion list)
22:20:05.22 +48:57:52.8 -- not an asteroid (will add it to exclusion list)
22:16:47.66 +45:02:24.0 -- not an asteroid (will add it to exclusion list)
20:58:30.43 +42:28:43.7 -- not an asteroid (will add it to exclusion list)
20:59:28.53 +42:08:26.4 -- not an asteroid (will add it to exclusion list)
20:56:57.84 +41:50:56.1 -- not an asteroid (will add it to exclusion list)
22:20:46.67 +48:54:36.8 -- not an asteroid (will add it to exclusion list)
22:19:33.02 +44:58:22.4 -- not an asteroid (will add it to exclusion list)
20:59:20.44 +41:55:44.3 -- not an asteroid (will add it to exclusion list)
21:03:56.38 +41:06:07.5 -- not an asteroid (will add it to exclusion list)
20:55:10.53 +42:17:24.8 -- not an asteroid (will add it to exclusion list)
20:57:45.60 +42:29:05.7 -- not an asteroid (will add it to exclusion list)
20:58:29.24 +41:37:09.4 -- not an asteroid (will add it to exclusion list)
20:55:23.39 +41:48:56.1 -- not an asteroid (will add it to exclusion list)
20:58:09.17 +42:30:29.3 -- not an asteroid (will add it to exclusion list)
20:58:59.60 +41:49:02.6 -- not an asteroid (will add it to exclusion list)
22:18:34.42 +45:02:50.2 -- not an asteroid (will add it to exclusion list)
21:00:17.17 +42:26:32.0 -- not an asteroid (will add it to exclusion list)
20:59:38.56 +41:54:57.8 -- not an asteroid (will add it to exclusion list)
21:08:02.59 +41:33:52.5 -- not an asteroid (will add it to exclusion list)
20:55:54.55 +41:46:31.5 -- not an asteroid (will add it to exclusion list)
22:22:35.19 +49:53:48.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:54:06.44 +42:55:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:10.89 +42:56:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:26.88 +42:48:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:28.06 +42:37:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:40.40 +42:05:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:40.82 +42:03:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:41.77 +42:39:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:42.67 +42:35:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:49.58 +41:53:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:53.52 +42:23:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:54.95 +41:57:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:55.65 +43:02:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:56.22 +42:06:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:56.38 +42:27:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:56.51 +41:51:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:56.93 +41:42:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:54:57.53 +42:14:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:00.46 +42:08:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:02.24 +41:53:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:02.87 +41:31:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:03.71 +42:03:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:03.80 +42:22:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:05.67 +42:03:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:07.44 +42:54:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:07.49 +41:59:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:08.17 +41:29:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:08.26 +41:50:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:08.53 +42:47:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:08.60 +41:43:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:10.53 +42:17:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:11.46 +41:51:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:12.11 +41:58:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:12.97 +42:36:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:15.37 +41:41:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:18.80 +41:21:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:19.89 +41:23:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:22.28 +41:59:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:22.31 +42:18:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:23.39 +41:48:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:23.75 +41:57:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:24.79 +41:23:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:25.87 +42:16:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:27.68 +42:22:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:28.11 +41:17:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:28.89 +41:54:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:30.14 +41:46:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:33.80 +41:23:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:34.05 +41:56:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:34.56 +41:36:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:35.04 +42:19:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:36.08 +41:29:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:36.69 +41:18:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:37.91 +41:14:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:38.01 +41:37:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:38.89 +41:41:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:39.24 +41:16:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:40.61 +41:19:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:42.76 +42:10:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:43.24 +42:45:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:43.66 +41:47:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:45.50 +41:25:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:45.50 +42:13:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:47.89 +41:37:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:49.15 +42:10:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:49.47 +41:27:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:50.22 +41:55:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:50.51 +41:25:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:52.48 +41:50:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:52.55 +42:24:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:53.60 +41:44:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:54.50 +41:43:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:54.55 +41:46:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:54.94 +41:55:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:56.05 +42:48:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:57.25 +41:07:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:00.61 +42:27:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:00.82 +41:37:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:00.95 +41:39:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:04.61 +42:43:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:04.72 +42:27:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:07.02 +41:36:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:07.05 +42:02:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:09.14 +41:56:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:11.15 +41:52:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:12.00 +41:09:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:12.50 +42:07:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:13.24 +41:42:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:13.45 +41:11:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:14.98 +42:06:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:15.78 +41:08:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:18.03 +42:26:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:23.70 +41:55:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:23.77 +41:54:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:24.99 +42:05:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:27.57 +42:32:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:27.78 +41:58:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:28.25 +41:51:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:28.62 +41:38:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:29.07 +41:34:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:31.05 +41:30:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:31.29 +42:22:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:31.82 +42:27:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:32.08 +42:12:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:33.34 +42:14:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:36.13 +41:59:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:39.36 +41:41:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:39.61 +42:10:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:40.49 +41:29:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:41.50 +42:23:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:45.10 +41:37:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:45.71 +42:49:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:46.73 +42:50:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:46.94 +41:53:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:47.92 +41:35:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:48.88 +41:56:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:55.24 +41:25:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:55.74 +41:48:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:56.89 +41:32:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:57.52 +41:35:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:57.84 +41:50:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:01.53 +42:00:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:02.78 +42:06:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:12.63 +41:19:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:13.03 +41:26:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:14.11 +42:01:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:14.89 +41:40:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:14.97 +41:18:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:14.99 +42:59:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:18.20 +41:20:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:19.80 +42:02:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:20.29 +41:45:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:22.01 +41:43:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:22.42 +41:31:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:22.47 +41:24:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:25.13 +41:55:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:26.05 +41:05:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:27.17 +41:51:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:28.30 +41:43:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:30.68 +41:49:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:31.72 +41:59:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:33.93 +41:56:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:35.05 +42:07:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:37.91 +41:58:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:38.63 +42:25:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:38.66 +41:49:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:39.93 +41:43:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:40.11 +41:57:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:41.47 +42:43:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:41.85 +41:57:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:45.49 +41:31:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:45.60 +42:29:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:47.51 +42:11:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:47.57 +41:34:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:47.79 +41:54:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:49.24 +41:20:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:49.40 +41:51:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:49.40 +42:02:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:50.13 +41:39:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:51.63 +42:30:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:52.04 +41:24:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:53.52 +41:51:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:54.05 +42:00:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:54.21 +41:29:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:55.44 +41:58:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:57.16 +41:45:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:57.64 +41:36:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:59.10 +42:00:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:59.10 +42:39:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:00.70 +42:01:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:02.84 +41:43:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:02.99 +42:28:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:03.26 +41:47:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:05.35 +41:21:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:05.54 +42:02:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:05.62 +41:16:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:05.81 +41:12:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:06.27 +41:43:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:06.79 +41:57:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:06.85 +42:34:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:09.01 +41:47:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:09.17 +42:30:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:09.81 +41:35:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:10.26 +42:29:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:10.77 +42:28:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:11.77 +41:19:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:12.68 +41:56:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:14.27 +42:13:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:14.62 +42:01:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:15.98 +42:09:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:16.67 +41:52:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:18.48 +41:49:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:18.93 +42:31:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:22.97 +41:53:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:23.91 +42:35:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:29.24 +41:37:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:29.51 +41:54:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:30.43 +42:28:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:30.53 +41:36:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:30.68 +41:48:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:30.99 +42:19:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:33.80 +42:24:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:34.48 +41:47:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:34.61 +42:03:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:35.06 +42:11:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:36.15 +41:37:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:36.39 +41:31:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:38.12 +42:05:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:39.87 +41:12:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:40.23 +41:54:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:40.76 +42:40:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:40.93 +42:38:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:42.53 +42:29:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:42.80 +41:58:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:43.11 +42:05:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:44.69 +42:19:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:47.59 +42:06:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:49.44 +42:27:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:50.42 +41:22:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:50.88 +42:06:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:52.65 +41:34:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:52.88 +41:42:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:54.10 +41:23:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:55.59 +42:06:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:58.13 +41:48:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:59.60 +41:49:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:59.80 +41:47:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:00.06 +42:17:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:00.38 +41:54:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:06.17 +42:38:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:06.45 +42:01:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:07.64 +41:35:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:08.34 +42:33:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:12.41 +41:55:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:12.48 +42:03:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:14.01 +41:40:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:15.00 +42:08:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:16.63 +42:15:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:18.39 +41:25:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:20.43 +41:48:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:20.44 +41:55:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:22.47 +42:17:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:28.53 +42:08:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:31.38 +42:28:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:32.64 +41:49:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:33.37 +42:10:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:34.26 +42:31:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:34.34 +42:32:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:36.46 +42:27:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:37.07 +41:23:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:38.56 +41:54:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:39.77 +42:13:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:40.06 +42:07:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:52.64 +42:13:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:54.32 +42:04:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:54.48 +42:17:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:56.09 +41:35:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:57.93 +41:43:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:01.86 +42:20:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:06.38 +42:10:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:08.60 +41:58:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:09.14 +42:24:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:09.79 +41:15:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:17.17 +42:26:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:18.52 +41:55:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:20.06 +41:11:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:21.34 +42:35:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:28.20 +41:55:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:30.78 +42:03:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:31.35 +42:02:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:31.81 +42:23:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:37.22 +42:04:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:42.16 +42:08:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:48.42 +42:19:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:48.91 +41:30:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:53.90 +42:10:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:00:59.48 +42:16:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:07.05 +42:13:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:34.59 +42:35:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:49.12 +41:30:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:22.17 +41:02:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:26.39 +41:04:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:52.05 +41:58:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:56.38 +41:06:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:41.86 +41:42:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:49.29 +41:34:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:02.59 +41:33:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:11.78 +42:14:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:01:38.84 +42:14:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:00.14 +42:13:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:05.98 +42:12:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:10.73 +42:15:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:14.46 +42:15:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:15.09 +42:11:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:15.24 +42:04:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:39.55 +42:13:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:42.05 +42:13:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:00.63 +42:05:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:16.20 +42:03:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:22.76 +42:04:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:25.35 +42:10:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:36.22 +42:03:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:36.58 +42:00:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:39.75 +42:03:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:03:57.63 +42:05:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:00.87 +42:11:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:04.04 +42:08:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:06.63 +42:06:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:07.37 +42:07:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:08.55 +42:05:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:21.21 +41:57:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:37.92 +41:49:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:41.67 +41:58:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:42.22 +41:56:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:45.95 +41:55:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:02.12 +41:56:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:10.90 +42:03:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:17.26 +42:00:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:15.49 +50:23:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:28.69 +48:58:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:44.34 +44:56:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:52.03 +45:01:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:24.17 +44:54:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:30.89 +48:53:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:41.47 +45:01:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:49.53 +44:55:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:50.18 +44:59:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:50.94 +45:01:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:51.51 +44:54:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:51.63 +44:56:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:15:56.35 +44:48:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:02.48 +49:08:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:03.15 +44:55:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:04.85 +45:09:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:05.80 +45:02:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:10.06 +48:59:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:19.95 +45:03:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:20.00 +44:49:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:21.27 +44:53:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:24.96 +45:01:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:29.09 +48:56:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:30.09 +49:13:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:31.78 +44:52:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:36.44 +48:58:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:38.46 +44:52:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:39.87 +45:00:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:45.86 +44:55:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:46.95 +44:58:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:47.66 +45:02:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:49.85 +44:53:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:54.53 +45:04:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:58.49 +44:53:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:03.89 +44:56:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:04.89 +44:29:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:07.59 +45:08:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:08.62 +45:04:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:15.59 +44:14:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:16.10 +44:50:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:20.92 +45:03:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:23.38 +44:48:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:23.94 +44:50:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:26.71 +44:51:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:33.54 +44:44:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:34.86 +44:11:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:39.58 +45:05:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:39.81 +44:53:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:44.94 +44:57:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:51.75 +44:46:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:52.11 +44:17:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:55.41 +44:59:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:58.52 +45:06:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:09.88 +44:51:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:12.34 +44:15:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:34.42 +45:02:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:37.57 +44:55:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:47.29 +44:55:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:03.86 +45:01:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:04.35 +44:57:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:08.95 +44:59:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:18.17 +44:58:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:19.10 +44:52:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:25.06 +44:51:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:28.79 +44:49:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:28.94 +45:01:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:33.02 +44:58:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:33.89 +45:00:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
22:19:39.17 +44:58:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:05.22 +48:57:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:07.45 +49:05:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:20:46.67 +48:54:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:00.39 +49:00:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:35.19 +49:53:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:45.89 +49:07:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
20:54:06.44 +42:55:11.7 -- not a known variable star
20:54:10.89 +42:56:21.0 -- not a known variable star
20:54:26.88 +42:48:48.8 -- not a known variable star
20:54:28.06 +42:37:09.9 -- not a known variable star
20:54:40.40 +42:05:49.7 -- not a known variable star
20:54:40.82 +42:03:30.7 -- not a known variable star
20:54:41.77 +42:39:36.0 -- a known variable star
20:54:42.67 +42:35:24.6 -- not a known variable star
20:54:49.58 +41:53:51.6 -- not a known variable star
20:54:53.52 +42:23:51.1 -- not a known variable star
20:54:54.95 +41:57:11.0 -- not a known variable star
20:54:55.65 +43:02:37.1 -- not a known variable star
20:54:56.22 +42:06:30.3 -- not a known variable star
20:54:56.38 +42:27:16.4 -- not a known variable star
20:54:56.51 +41:51:13.5 -- not a known variable star
20:54:56.93 +41:42:29.6 -- a known variable star
20:54:57.53 +42:14:38.4 -- not a known variable star
20:55:00.46 +42:08:23.8 -- not a known variable star
20:55:02.24 +41:53:13.0 -- not a known variable star
20:55:02.87 +41:31:54.4 -- not a known variable star
20:55:03.71 +42:03:54.8 -- not a known variable star
20:55:03.80 +42:22:40.6 -- a known variable star
20:55:05.67 +42:03:37.2 -- a known variable star
20:55:07.44 +42:54:33.0 -- not a known variable star
20:55:07.49 +41:59:27.1 -- not a known variable star
20:55:08.17 +41:29:45.3 -- not a known variable star
20:55:08.26 +41:50:37.6 -- not a known variable star
20:55:08.53 +42:47:47.7 -- a known variable star
20:55:08.60 +41:43:07.0 -- not a known variable star
20:55:10.53 +42:17:24.8 -- not a known variable star
20:55:11.46 +41:51:15.8 -- not a known variable star
20:55:12.11 +41:58:00.1 -- not a known variable star
20:55:12.97 +42:36:18.6 -- not a known variable star
20:55:15.37 +41:41:22.2 -- not a known variable star
20:55:18.80 +41:21:47.9 -- not a known variable star
20:55:19.89 +41:23:02.8 -- not a known variable star
20:55:22.28 +41:59:48.4 -- not a known variable star
20:55:22.31 +42:18:43.0 -- not a known variable star
20:55:23.39 +41:48:56.1 -- not a known variable star
20:55:23.75 +41:57:15.6 -- not a known variable star
20:55:24.79 +41:23:33.5 -- not a known variable star
20:55:25.87 +42:16:36.2 -- not a known variable star
20:55:27.68 +42:22:06.2 -- not a known variable star
20:55:28.11 +41:17:39.5 -- not a known variable star
20:55:28.89 +41:54:16.6 -- not a known variable star
20:55:30.14 +41:46:55.3 -- not a known variable star
20:55:33.80 +41:23:10.8 -- not a known variable star
20:55:34.05 +41:56:30.8 -- not a known variable star
20:55:34.56 +41:36:48.0 -- not a known variable star
20:55:35.04 +42:19:43.9 -- not a known variable star
20:55:36.08 +41:29:00.1 -- not a known variable star
20:55:36.69 +41:18:26.2 -- not a known variable star
20:55:37.91 +41:14:30.9 -- not a known variable star
20:55:38.01 +41:37:59.2 -- not a known variable star
20:55:38.89 +41:41:51.0 -- not a known variable star
20:55:39.24 +41:16:53.8 -- not a known variable star
20:55:40.61 +41:19:25.0 -- not a known variable star
20:55:42.76 +42:10:08.9 -- a known variable star
20:55:43.24 +42:45:59.4 -- not a known variable star
20:55:43.66 +41:47:36.0 -- not a known variable star
20:55:45.50 +41:25:46.6 -- not a known variable star
20:55:45.50 +42:13:26.2 -- not a known variable star
20:55:47.89 +41:37:34.8 -- not a known variable star
20:55:49.15 +42:10:30.4 -- not a known variable star
20:55:49.47 +41:27:16.5 -- not a known variable star
20:55:50.22 +41:55:20.1 -- not a known variable star
20:55:50.51 +41:25:45.2 -- not a known variable star
20:55:52.48 +41:50:26.5 -- a known variable star
20:55:52.55 +42:24:33.7 -- a known variable star
20:55:53.60 +41:44:23.8 -- not a known variable star
20:55:54.50 +41:43:32.9 -- not a known variable star
20:55:54.55 +41:46:31.5 -- not a known variable star
20:55:54.94 +41:55:53.9 -- not a known variable star
20:55:56.05 +42:48:25.4 -- not a known variable star
20:55:57.25 +41:07:24.2 -- not a known variable star
20:56:00.61 +42:27:51.7 -- not a known variable star
20:56:00.82 +41:37:23.6 -- not a known variable star
20:56:00.95 +41:39:08.1 -- not a known variable star
20:56:04.61 +42:43:29.8 -- not a known variable star
20:56:04.72 +42:27:40.4 -- not a known variable star
20:56:07.02 +41:36:52.7 -- not a known variable star
20:56:07.05 +42:02:47.1 -- not a known variable star
20:56:09.14 +41:56:56.9 -- not a known variable star
20:56:11.15 +41:52:46.1 -- not a known variable star
20:56:12.00 +41:09:26.8 -- not a known variable star
20:56:12.50 +42:07:04.6 -- not a known variable star
20:56:13.24 +41:42:57.4 -- not a known variable star
20:56:13.45 +41:11:51.7 -- not a known variable star
20:56:14.98 +42:06:14.1 -- not a known variable star
20:56:15.78 +41:08:56.4 -- not a known variable star
20:56:18.03 +42:26:25.4 -- not a known variable star
20:56:23.70 +41:55:38.1 -- not a known variable star
20:56:23.77 +41:54:31.7 -- not a known variable star
20:56:24.99 +42:05:10.5 -- not a known variable star
20:56:27.57 +42:32:59.9 -- a known variable star
20:56:27.78 +41:58:25.6 -- not a known variable star
20:56:28.25 +41:51:52.0 -- not a known variable star
20:56:28.62 +41:38:12.5 -- not a known variable star
20:56:29.07 +41:34:44.9 -- not a known variable star
20:56:31.05 +41:30:42.7 -- not a known variable star
20:56:31.29 +42:22:22.9 -- not a known variable star
20:56:31.82 +42:27:20.9 -- not a known variable star
20:56:32.08 +42:12:05.9 -- not a known variable star
20:56:33.34 +42:14:09.4 -- not a known variable star
20:56:36.13 +41:59:18.3 -- not a known variable star
20:56:39.36 +41:41:51.3 -- not a known variable star
20:56:39.61 +42:10:22.7 -- not a known variable star
20:56:40.49 +41:29:56.6 -- not a known variable star
20:56:41.50 +42:23:13.5 -- not a known variable star
20:56:45.10 +41:37:22.7 -- not a known variable star
20:56:45.71 +42:49:04.9 -- a known variable star
20:56:46.73 +42:50:45.8 -- not a known variable star
20:56:46.94 +41:53:07.6 -- not a known variable star
20:56:47.92 +41:35:44.9 -- not a known variable star
20:56:48.88 +41:56:10.1 -- not a known variable star
20:56:55.24 +41:25:51.6 -- not a known variable star
20:56:55.74 +41:48:40.8 -- not a known variable star
20:56:56.89 +41:32:20.4 -- not a known variable star
20:56:57.52 +41:35:33.4 -- not a known variable star
20:56:57.84 +41:50:56.1 -- not a known variable star
20:57:01.53 +42:00:44.6 -- not a known variable star
20:57:02.78 +42:06:31.1 -- not a known variable star
20:57:12.63 +41:19:22.5 -- a known variable star
20:57:13.03 +41:26:00.0 -- not a known variable star
20:57:14.11 +42:01:20.3 -- not a known variable star
20:57:14.89 +41:40:24.7 -- not a known variable star
20:57:14.97 +41:18:18.2 -- not a known variable star
20:57:14.99 +42:59:56.5 -- a known variable star
20:57:18.20 +41:20:55.9 -- not a known variable star
20:57:19.80 +42:02:12.1 -- not a known variable star
20:57:20.29 +41:45:28.2 -- not a known variable star
20:57:22.01 +41:43:35.2 -- a known variable star
20:57:22.42 +41:31:07.2 -- not a known variable star
20:57:22.47 +41:24:18.3 -- not a known variable star
20:57:25.13 +41:55:56.1 -- not a known variable star
20:57:26.05 +41:05:44.1 -- not a known variable star
20:57:27.17 +41:51:06.5 -- not a known variable star
20:57:28.30 +41:43:39.1 -- not a known variable star
20:57:30.68 +41:49:39.4 -- not a known variable star
20:57:31.72 +41:59:11.6 -- not a known variable star
20:57:33.93 +41:56:54.1 -- not a known variable star
20:57:35.05 +42:07:09.9 -- not a known variable star
20:57:37.91 +41:58:56.6 -- not a known variable star
20:57:38.63 +42:25:57.3 -- not a known variable star
20:57:38.66 +41:49:09.2 -- not a known variable star
20:57:39.93 +41:43:10.6 -- not a known variable star
20:57:40.11 +41:57:04.3 -- a known variable star
20:57:41.47 +42:43:43.1 -- not a known variable star
20:57:41.85 +41:57:59.0 -- not a known variable star
20:57:45.49 +41:31:36.4 -- not a known variable star
20:57:45.60 +42:29:05.7 -- not a known variable star
20:57:47.51 +42:11:08.9 -- a known variable star
20:57:47.57 +41:34:46.0 -- not a known variable star
20:57:47.79 +41:54:10.7 -- not a known variable star
20:57:49.24 +41:20:12.2 -- not a known variable star
20:57:49.40 +41:51:20.1 -- not a known variable star
20:57:49.40 +42:02:53.3 -- not a known variable star
20:57:50.13 +41:39:32.6 -- not a known variable star
20:57:51.63 +42:30:51.2 -- a known variable star
20:57:52.04 +41:24:13.7 -- not a known variable star
20:57:53.52 +41:51:09.7 -- not a known variable star
20:57:54.05 +42:00:31.7 -- not a known variable star
20:57:54.21 +41:29:55.4 -- not a known variable star
20:57:55.44 +41:58:48.0 -- not a known variable star
20:57:57.16 +41:45:02.9 -- a known variable star
20:57:57.64 +41:36:27.6 -- not a known variable star
20:57:59.10 +42:00:04.5 -- not a known variable star
20:57:59.10 +42:39:28.6 -- not a known variable star
20:58:00.70 +42:01:11.8 -- not a known variable star
20:58:02.84 +41:43:33.4 -- not a known variable star
20:58:02.99 +42:28:18.1 -- a known variable star
20:58:03.26 +41:47:34.5 -- a known variable star
20:58:05.35 +41:21:50.6 -- not a known variable star
20:58:05.54 +42:02:32.7 -- not a known variable star
20:58:05.62 +41:16:45.6 -- not a known variable star
20:58:05.81 +41:12:50.1 -- not a known variable star
20:58:06.27 +41:43:25.6 -- not a known variable star
20:58:06.79 +41:57:19.2 -- not a known variable star
20:58:06.85 +42:34:52.3 -- not a known variable star
20:58:09.01 +41:47:11.2 -- not a known variable star
20:58:09.17 +42:30:29.3 -- not a known variable star
20:58:09.81 +41:35:31.6 -- not a known variable star
20:58:10.26 +42:29:24.0 -- a known variable star
20:58:10.77 +42:28:39.4 -- not a known variable star
20:58:11.77 +41:19:28.3 -- not a known variable star
20:58:12.68 +41:56:45.2 -- a known variable star
20:58:14.27 +42:13:28.4 -- not a known variable star
20:58:14.62 +42:01:00.4 -- not a known variable star
20:58:15.98 +42:09:49.5 -- not a known variable star
20:58:16.67 +41:52:25.6 -- not a known variable star
20:58:18.48 +41:49:25.8 -- not a known variable star
20:58:18.93 +42:31:21.1 -- not a known variable star
20:58:22.97 +41:53:43.5 -- not a known variable star
20:58:23.91 +42:35:14.8 -- not a known variable star
20:58:29.24 +41:37:09.4 -- not a known variable star
20:58:29.51 +41:54:14.2 -- not a known variable star
20:58:30.43 +42:28:43.7 -- not a known variable star
20:58:30.53 +41:36:40.8 -- not a known variable star
20:58:30.68 +41:48:13.2 -- not a known variable star
20:58:30.99 +42:19:45.7 -- not a known variable star
20:58:33.80 +42:24:01.0 -- not a known variable star
20:58:34.48 +41:47:17.0 -- not a known variable star
20:58:34.61 +42:03:26.2 -- not a known variable star
20:58:35.06 +42:11:54.0 -- not a known variable star
20:58:36.15 +41:37:09.6 -- not a known variable star
20:58:36.39 +41:31:56.9 -- not a known variable star
20:58:38.12 +42:05:08.8 -- a known variable star
20:58:39.87 +41:12:46.8 -- not a known variable star
20:58:40.23 +41:54:51.6 -- a known variable star
20:58:40.76 +42:40:09.5 -- a known variable star
20:58:40.93 +42:38:54.0 -- not a known variable star
20:58:42.53 +42:29:45.5 -- not a known variable star
20:58:42.80 +41:58:57.7 -- not a known variable star
20:58:43.11 +42:05:30.7 -- not a known variable star
20:58:44.69 +42:19:33.4 -- not a known variable star
20:58:47.59 +42:06:12.1 -- not a known variable star
20:58:49.44 +42:27:20.7 -- not a known variable star
20:58:50.42 +41:22:12.9 -- not a known variable star
20:58:50.88 +42:06:26.9 -- not a known variable star
20:58:52.65 +41:34:31.1 -- not a known variable star
20:58:52.88 +41:42:54.9 -- not a known variable star
20:58:54.10 +41:23:20.7 -- not a known variable star
20:58:55.59 +42:06:13.4 -- not a known variable star
20:58:58.13 +41:48:30.3 -- not a known variable star
20:58:59.60 +41:49:02.6 -- not a known variable star
20:58:59.80 +41:47:43.1 -- not a known variable star
20:59:00.06 +42:17:21.6 -- not a known variable star
20:59:00.38 +41:54:16.0 -- not a known variable star
20:59:06.17 +42:38:30.9 -- a known variable star
20:59:06.45 +42:01:23.2 -- not a known variable star
20:59:07.64 +41:35:10.4 -- not a known variable star
20:59:08.34 +42:33:13.3 -- not a known variable star
20:59:12.41 +41:55:47.1 -- not a known variable star
20:59:12.48 +42:03:33.2 -- not a known variable star
20:59:14.01 +41:40:39.5 -- not a known variable star
20:59:15.00 +42:08:08.2 -- a known variable star
20:59:16.63 +42:15:24.9 -- a known variable star
20:59:18.39 +41:25:47.8 -- not a known variable star
20:59:20.43 +41:48:03.8 -- not a known variable star
20:59:20.44 +41:55:44.3 -- a known variable star
20:59:22.47 +42:17:42.2 -- not a known variable star
20:59:28.53 +42:08:26.4 -- a known variable star
20:59:31.38 +42:28:23.5 -- not a known variable star
20:59:32.64 +41:49:20.6 -- not a known variable star
20:59:33.37 +42:10:02.5 -- a known variable star
20:59:34.26 +42:31:52.8 -- not a known variable star
20:59:34.34 +42:32:30.0 -- not a known variable star
20:59:36.46 +42:27:28.7 -- not a known variable star
20:59:37.07 +41:23:51.2 -- not a known variable star
20:59:38.56 +41:54:57.8 -- not a known variable star
20:59:39.77 +42:13:37.8 -- not a known variable star
20:59:40.06 +42:07:32.2 -- not a known variable star
20:59:52.64 +42:13:39.7 -- not a known variable star
20:59:54.32 +42:04:51.2 -- not a known variable star
20:59:54.48 +42:17:01.5 -- not a known variable star
20:59:56.09 +41:35:19.7 -- a known variable star
20:59:57.93 +41:43:57.0 -- not a known variable star
21:00:01.86 +42:20:43.6 -- not a known variable star
21:00:06.38 +42:10:03.6 -- not a known variable star
21:00:08.60 +41:58:28.7 -- a known variable star
21:00:09.14 +42:24:01.6 -- not a known variable star
21:00:09.79 +41:15:21.8 -- not a known variable star
21:00:17.17 +42:26:32.0 -- not a known variable star
21:00:18.52 +41:55:39.7 -- not a known variable star
21:00:20.06 +41:11:05.9 -- not a known variable star
21:00:21.34 +42:35:11.4 -- not a known variable star
21:00:28.20 +41:55:55.9 -- not a known variable star
21:00:30.78 +42:03:49.4 -- not a known variable star
21:00:31.35 +42:02:48.8 -- not a known variable star
21:00:31.81 +42:23:51.2 -- not a known variable star
21:00:37.22 +42:04:36.4 -- not a known variable star
21:00:42.16 +42:08:09.5 -- a known variable star
21:00:48.42 +42:19:23.1 -- not a known variable star
21:00:48.91 +41:30:11.0 -- not a known variable star
21:00:53.90 +42:10:19.1 -- not a known variable star
21:00:59.48 +42:16:48.9 -- a known variable star
21:01:07.05 +42:13:22.9 -- a known variable star
21:01:34.59 +42:35:32.2 -- not a known variable star
21:01:49.12 +41:30:48.4 -- not a known variable star
21:02:22.17 +41:02:48.4 -- not a known variable star
21:02:26.39 +41:04:28.0 -- a known variable star
21:02:52.05 +41:58:13.3 -- not a known variable star
21:03:56.38 +41:06:07.5 -- not a known variable star
21:04:41.86 +41:42:31.5 -- not a known variable star
21:04:49.29 +41:34:45.2 -- a known variable star
21:08:02.59 +41:33:52.5 -- not a known variable star
22:01:11.78 +42:14:35.7 -- not a known variable star
22:01:38.84 +42:14:35.6 -- not a known variable star
22:02:00.14 +42:13:18.8 -- not a known variable star
22:02:05.98 +42:12:46.5 -- a known variable star
22:02:10.73 +42:15:16.6 -- not a known variable star
22:02:14.46 +42:15:55.0 -- not a known variable star
22:02:15.09 +42:11:54.7 -- not a known variable star
22:02:15.24 +42:04:09.9 -- not a known variable star
22:02:39.55 +42:13:38.8 -- a known variable star
22:02:42.05 +42:13:03.4 -- not a known variable star
22:03:00.63 +42:05:24.9 -- not a known variable star
22:03:16.20 +42:03:28.4 -- not a known variable star
22:03:22.76 +42:04:04.9 -- not a known variable star
22:03:25.35 +42:10:18.6 -- not a known variable star
22:03:36.22 +42:03:43.3 -- a known variable star
22:03:36.58 +42:00:42.4 -- not a known variable star
22:03:39.75 +42:03:06.8 -- not a known variable star
22:03:57.63 +42:05:36.8 -- not a known variable star
22:04:00.87 +42:11:01.3 -- not a known variable star
22:04:04.04 +42:08:35.6 -- a known variable star
22:04:06.63 +42:06:29.3 -- a known variable star
22:04:07.37 +42:07:51.6 -- not a known variable star
22:04:08.55 +42:05:35.9 -- not a known variable star
22:04:21.21 +41:57:52.9 -- not a known variable star
22:04:37.92 +41:49:51.5 -- not a known variable star
22:04:41.67 +41:58:08.1 -- not a known variable star
22:04:42.22 +41:56:40.1 -- not a known variable star
22:04:45.95 +41:55:14.0 -- not a known variable star
22:05:02.12 +41:56:05.9 -- not a known variable star
22:05:10.90 +42:03:02.0 -- not a known variable star
22:05:17.26 +42:00:40.3 -- not a known variable star
22:11:15.49 +50:23:25.0 -- a known variable star
22:14:28.69 +48:58:26.0 -- not a known variable star
22:14:44.34 +44:56:23.1 -- not a known variable star
22:14:52.03 +45:01:26.9 -- not a known variable star
22:15:24.17 +44:54:45.4 -- not a known variable star
22:15:30.89 +48:53:41.0 -- not a known variable star
22:15:41.47 +45:01:41.4 -- a known variable star
22:15:49.53 +44:55:51.3 -- not a known variable star
22:15:50.18 +44:59:33.3 -- not a known variable star
22:15:50.94 +45:01:14.9 -- not a known variable star
22:15:51.51 +44:54:15.5 -- not a known variable star
22:15:51.63 +44:56:13.3 -- not a known variable star
22:15:56.35 +44:48:17.6 -- not a known variable star
22:16:02.48 +49:08:31.7 -- a known variable star
22:16:03.15 +44:55:13.3 -- not a known variable star
22:16:04.85 +45:09:26.9 -- not a known variable star
22:16:05.80 +45:02:12.7 -- a known variable star
22:16:10.06 +48:59:32.8 -- not a known variable star
22:16:19.95 +45:03:03.1 -- not a known variable star
22:16:20.00 +44:49:09.2 -- not a known variable star
22:16:21.27 +44:53:24.2 -- a known variable star
22:16:24.96 +45:01:12.4 -- not a known variable star
22:16:29.09 +48:56:17.5 -- not a known variable star
22:16:30.09 +49:13:41.6 -- not a known variable star
22:16:31.78 +44:52:39.1 -- not a known variable star
22:16:36.44 +48:58:57.5 -- not a known variable star
22:16:38.46 +44:52:58.0 -- not a known variable star
22:16:39.87 +45:00:05.2 -- not a known variable star
22:16:45.86 +44:55:37.8 -- not a known variable star
22:16:46.95 +44:58:33.9 -- not a known variable star
22:16:47.66 +45:02:24.0 -- not a known variable star
22:16:49.85 +44:53:45.0 -- not a known variable star
22:16:54.53 +45:04:04.1 -- not a known variable star
22:16:58.49 +44:53:47.8 -- not a known variable star
22:17:03.89 +44:56:05.7 -- a known variable star
22:17:04.89 +44:29:51.5 -- not a known variable star
22:17:07.59 +45:08:30.6 -- not a known variable star
22:17:08.62 +45:04:57.8 -- a known variable star
22:17:15.59 +44:14:54.1 -- not a known variable star
22:17:16.10 +44:50:48.6 -- not a known variable star
22:17:20.92 +45:03:21.2 -- not a known variable star
22:17:23.38 +44:48:46.1 -- not a known variable star
22:17:23.94 +44:50:07.2 -- not a known variable star
22:17:26.71 +44:51:59.7 -- not a known variable star
22:17:33.54 +44:44:40.8 -- not a known variable star
22:17:34.86 +44:11:40.0 -- not a known variable star
22:17:39.58 +45:05:15.5 -- not a known variable star
22:17:39.81 +44:53:29.3 -- not a known variable star
22:17:44.94 +44:57:56.2 -- not a known variable star
22:17:51.75 +44:46:13.2 -- a known variable star
22:17:52.11 +44:17:05.3 -- not a known variable star
22:17:55.41 +44:59:01.8 -- a known variable star
22:17:58.52 +45:06:01.8 -- not a known variable star
22:18:09.88 +44:51:41.6 -- not a known variable star
22:18:12.34 +44:15:00.6 -- not a known variable star
22:18:34.42 +45:02:50.2 -- a known variable star
22:18:37.57 +44:55:40.4 -- not a known variable star
22:18:47.29 +44:55:33.8 -- not a known variable star
22:19:03.86 +45:01:23.1 -- not a known variable star
22:19:04.35 +44:57:51.0 -- not a known variable star
22:19:08.95 +44:59:11.4 -- not a known variable star
22:19:18.17 +44:58:06.3 -- not a known variable star
22:19:19.10 +44:52:39.4 -- not a known variable star
22:19:25.06 +44:51:13.3 -- not a known variable star
22:19:28.79 +44:49:14.8 -- not a known variable star
22:19:28.94 +45:01:49.1 -- a known variable star
22:19:33.02 +44:58:22.4 -- not a known variable star
22:19:33.89 +45:00:34.7 -- not a known variable star
22:19:39.17 +44:58:06.5 -- a known variable star
22:20:05.22 +48:57:52.8 -- a known variable star
22:20:07.45 +49:05:58.0 -- not a known variable star
22:20:46.67 +48:54:36.8 -- not a known variable star
22:22:00.39 +49:00:11.1 -- not a known variable star
22:22:35.19 +49:53:48.0 -- a known variable star
22:22:45.89 +49:07:56.0 -- not a known variable star
Found 336 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
392 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 392 (excluding asteroids and hot pixels, 336 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461300.87329296 -observatory V36
12:38:39.32 -04:12:45.6 Mercury (-0.4mag)
13:58:10.16 -17:56:49.8 Venus (-4.8mag)
07:40:43.09 +22:13:10.6 Mars (1.2mag)
09:17:08.81 +16:22:46.2 Jupiter (-1.8mag)
00:49:13.89 +02:21:15.9 Saturn (0.4mag)
04:13:37.89 +21:01:51.7 Uranus (5.7mag)
00:12:45.80 -00:09:48.9 Neptune (7.7mag)
20:24:58.29 -23:41:36.1 Pluto (14.5mag)
16:18:13.57 -26:52:24.8 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)2461300.87329296:
09:17:14.51 +16:22:18.1 Io (6.0mag)
09:17:14.49 +16:22:18.4 Europa (6.2mag)
09:16:55.38 +16:23:56.9 Ganymede (5.6mag)
09:17:25.73 +16:21:20.5 Callisto (6.8mag)
09:15:20.27 +16:42:59.4 Himalia (15.7mag)
09:17:12.82 +16:22:27.2 Thebe (16.5mag)
09:14:48.59 +16:37:08.6 Elara (17.7mag)
09:20:44.96 +15:47:43.6 Pasiphae (17.9mag)
09:17:29.85 +16:43:20.6 Carme (18.9mag)
00:49:24.76 +02:20:48.3 Titan (8.3mag)
00:49:13.92 +02:20:55.4 Rhea (9.6mag)
00:49:00.15 +02:22:16.7 Iapetus (11.0mag)
00:49:00.45 +02:21:30.7 Hyperion (14.3mag)
00:47:50.73 +02:10:08.8 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)2461300.87329296:
23:29:14.26 +10:52:22.6 JWST
16:46:48.39 +43:10:27.0 Chandra
12:05:46.92 -61:33:20.5 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)2461300.87329296 -observatory V36
03:45:14.40 +19:44:45.7 17.3mag P/1996 R2 (Lagerkvist)
18:07:22.64 -34:01:03.3 14.5mag P/2010 H2 (Vales)
07:26:41.48 -70:52:53.0 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:32.54 +33:58:06.1 17.7mag C/2017 K2 (PANSTARRS)
05:02:35.81 +46:47:00.8 16.2mag P/2021 N1 (ZTF)
22:05:46.85 +27:22:26.4 17.5mag C/2022 E2 (ATLAS)
07:17:23.37 +25:47:48.8 16.9mag C/2022 N2 (PANSTARRS)
10:58:43.32 +26:53:20.2 17.1mag C/2022 QE78 (ATLAS)
09:54:56.97 +05:10:33.9 18.0mag C/2022 R6 (PANSTARRS)
15:27:37.26 -16:31:45.4 15.0mag C/2023 R1 (PANSTARRS)
08:46:44.35 +33:33:42.3 15.9mag C/2024 E1 (Wierzchos)
15:08:14.58 +15:12:51.7 18.0mag C/2024 G6 (ATLAS)
18:28:32.22 +42:43:44.9 13.7mag C/2024 J3 (ATLAS)
20:13:11.52 +48:37:20.9 17.4mag C/2024 R4 (PANSTARRS)
05:40:23.55 -13:11:04.1 15.0mag C/2024 T5 (ATLAS)
07:14:26.90 +16:28:32.7 17.8mag C/2025 J1 (Borisov)
11:34:33.26 +17:58:07.9 16.6mag C/2025 V2 (Rankin)
13:28:13.16 -00:42:29.8 16.7mag C/2025 Y1 (ATLAS)
17:11:09.28 +72:11:14.6 15.9mag C/2026 A2 (Bok)
02:59:32.28 +45:41:19.9 17.5mag C/2026 B2 (Sun-Gao)
12:22:42.10 +12:06:29.8 17.6mag A/2026 E1
22:34:33.28 -35:08:41.0 13.6mag 10P/Tempel
01:35:10.48 +38:45:59.9 17.5mag 11P/Tempel-Swift-LINEAR
11:54:57.92 -06:14:21.4 16.3mag 29P/Schwassmann-Wachmann
12:28:51.39 -08:14:47.5 17.8mag 63P/Wild
06:58:06.46 +18:24:58.6 17.1mag 78P/Gehrels
03:16:09.07 +15:01:42.7 17.3mag 88P/Howell
06:12:29.80 +32:23:47.0 17.3mag 112P/Urata-Niijima
08:00:53.45 +22:02:52.3 17.8mag 114P/Wiseman-Skiff
10:50:08.87 +18:41:18.5 14.8mag 123P/West-Hartley
13:09:10.95 -24:46:31.5 17.5mag 124P/Mrkos
06:29:02.02 +20:17:50.9 15.8mag 128P/Shoemaker-Holt
01:38:27.98 -15:30:28.7 14.5mag 161P/Hartley-IRAS
09:32:31.58 +08:40:50.2 12.5mag 169P/NEAT
03:30:54.92 +07:31:26.2 14.6mag 220P/McNaught
05:14:14.13 +39:18:23.0 15.3mag 260P/McNaught
08:58:09.94 +34:32:54.2 17.3mag 295P/LINEAR
15:32:11.99 -01:22:10.0 17.9mag 391P/Kowalski
09:36:20.33 +16:20:25.8 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